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Clifford algebra Cl(0,6) approach to beyond the standard model and naturalness problems

Wei Lu
Abstract

Is there more to Dirac’s gamma matrices than meets the eye? It turns out that gamma zero can be factorized into a product of three operators. This revelation facilitates the expansion of Dirac’s space-time algebra to Clifford algebra Cl(0,6). The resultant rich geometric structure can be leveraged to establish a combined framework of the standard model and gravity, wherein a gravi-weak interaction between the extended vierbein field and the extended weak gauge field is allowed. In conjunction with the composite Higgs model, we examine the vierbein field as a Cooper-pair-like fermion-antifermion condensation. Quantum gravity is realized indirectly via the quantized standard model spinor fields which underlie the composite space-time metric. We propose that the fundamental energy scales of the universe including the Planck scale are emergent and resulted from quantum condensations, thus possibly addressing the cosmological constant problem through an unconventional multi-scale renormalization procedure for multiplications of divergent Feynman integrals. The Clifford algebra approach also permits a weaker form of charge conjugation without particle-antiparticle interchange, leading to a Majorana-type mass that conserves lepton number. Additionally, with reshuffling the traditional quark-lepton pairing pattern of three generations of fermions, we explore a three-Higgs-doublet model with Higgs VEVs 246 GeV, 42 GeV and 2.5 GeV which could explain the mass hierarchies of fermions.

keywords:
Clifford algebra; geometric algebra; beyond the standard model; quantum gravity; hierarchy problem; cosmological constant problem.
{history}

1 Introduction

The mathematical imaginary number ii is ubiquitous in physics theories. In the case of quantum mechanics, the imaginary number makes its appearance in the commutation relation of position operator X^\hat{X} and momentum operator P^\hat{P}

[X^,P^]=i,\displaystyle[\hat{X},\hat{P}]=i\hbar, (1)

where \hbar is the Planck constant. Consequently, the quantum wave function is complex-valued.

On the other hand, the imaginary number also shows up in the gauge transformation of a classical field

ψeiθψ,\displaystyle\psi\rightarrow e^{i\theta}\psi, (2)

which is essential in determining the electric charge property of ψ\psi.

We customarily treat the imaginary number ii in both examples as the same. It may come as a surprise that the imaginary number in the second case is different from the first one. The imaginary number in gauge transformation (2) is actually a unit pseudoscalar in disguise

I\displaystyle I =γ0γ1γ2γ3,\displaystyle=\gamma_{0}\gamma_{1}\gamma_{2}\gamma_{3}, (3)

where γa\gamma_{a} are no other than the celebrated gamma operators discovered by Paul Dirac in 1928. The Dirac gamma operators satisfy the Clifford algebra Cl(1,3)Cl(1,3) anticommutation relations

{γa,γb}=γaγb+γbγa=2ηab,\displaystyle\{\gamma_{a},\gamma_{b}\}=\gamma_{a}\gamma_{b}+\gamma_{b}\gamma_{a}=2\eta_{ab}, (4)

where ηab=diag(1,1,1,1)\eta_{ab}=diag(1,-1,-1,-1).

In view that I2=1I^{2}=-1, pseudoscalar II can be regarded as a surrogate for imaginary number ii. As we will learn later in this paper, replacing imaginary number ii with pseudoscalar II in gauge transformation (2) such as ψψeIθ\psi\rightarrow\psi e^{I\theta} leads to a novel definition of charge conjugation without particle-antiparticle interchange. And for that matter, the original imaginary number ii shall be banished from the definition of classical fields such as classical spinor and Higgs fields. Instead, imaginary number ii should be reserved for its proper domain which is field quantization.

Historically, the Dirac operators γa\gamma_{a} are represented as gamma matrices. Due to the dichotomy between fermion states as columns and operators as matrices in the conventional formalism of quantum field theory (QFT), the aforementioned association of pseudoscalar with imaginary number would run into inconsistencies. This identification can only be achieved in an unconventional way by forgoing the traditional matrix and column representation and enlisting the aid of the Clifford algebra approach [1, 2, 3, 4, 5, 6, 7, 8, 9, 10, 11, 13, 14, 15, 16, 12, 17, 18, 19, 20, 21, 22, 23, 24, 25, 26, 27, 28, 29, 30, 31, 32], whereby both the algebraic spinor states and Dirac’s gamma operators can be expressed in the same algebraic space. Note that we have already been using the Clifford algebraic non-matrix format, such as in Eq. (4).

Clifford algebra, also known as geometric algebra or space-time algebra for the specific case of Cl(1,3)Cl(1,3), is a potent mathematical tool that finds extensive applications in the physics arena. Remarkably, there is one more application of Clifford algebra Cl(1,3)Cl(1,3) unbeknownst to Paul Dirac in 1928 which is the Clifford algebra Cl(1,3)Cl(1,3) formalism of Lorentz gauge gravity. We know that gravity can be formulated as a Lorentz gauge theory [33, 34, 35, 36] in terms of vierbein (a.k.a. tetrad, co-frame, or soldering form) and spin connection (a.k.a. Lorentz connection). According to the Clifford algebra Cl(1,3)Cl(1,3) formalism of Lorentz gauge gravity [37, 38, 39], the vierbein e^μ\hat{e}_{\mu} and spin connection Lorentz gauge field ω^μ\hat{\omega}_{\mu} take values in the Clifford algebraic space
e^μ=eμaγa,\displaystyle\hat{e}_{\mu}=e_{\mu}^{a}\gamma_{a}, (5a)
ω^μ=14ωμabγaγb,\displaystyle\hat{\omega}_{\mu}=\frac{1}{4}\omega_{\mu}^{ab}\gamma_{a}\gamma_{b}, (5b)

where eμae_{\mu}^{a} and ωμab\omega_{\mu}^{ab} are real-valued, ωμab=ωμba\omega_{\mu}^{ab}=-\omega_{\mu}^{ba}, and a,b,μ=0,1,2,3a,b,\mu=0,1,2,3. Throughout this paper the summation convention for repeated indices is adopted. The four distinct {γa}\{\gamma_{a}\} and six distinct {γaγb;a<b}\{\gamma_{a}\gamma_{b};a<b\} are called vectors and bi-vectors of Clifford algebra. We denote vierbein as e^μ\hat{e}_{\mu} and spin connection as ω^μ\hat{\omega}_{\mu} rather than eμe_{\mu} and ωμ\omega_{\mu} to accentuate the fact that they are Clifford-valued.

The Lorentz gauge approach to gravity is also known as Einstein-Cartan gravity. The spin connection gauge field ω^μ\hat{\omega}_{\mu}, associated with the local Lorentz group SO(1,3)SO(1,3) (or Spin(1,3)Spin(1,3) when fermions are involved), plays the role of the gauge fields in Yang-Mills theory. In the gauge theory of gravity, the space-time metric gμνg_{\mu\nu} is defined as a composite field

gμν=e^μe^ν=eμaeνbηab,g_{\mu\nu}=\left\langle\hat{e}_{\mu}\hat{e}_{\nu}\right\rangle=e^{a}_{\mu}e^{b}_{\nu}\eta_{ab}, (6)

where \left\langle\ldots\right\rangle stands for the Clifford-scalar part of the enclosed expression. Thus vierbein e^μ\hat{e}_{\mu} can be deemed as the “square root” of metric.

Given that the gravity-related fields e^μ\hat{e}_{\mu} and ω^μ\hat{\omega}_{\mu} are vector-valued and bi-vector-valued respectively in the Clifford algebraic space of Cl(1,3)Cl(1,3), it’s tempting to wonder whether the other interactions in nature such as the electroweak and strong gauge fields can take values in the Clifford algebraic space as well. The answer is a resounding yes, provided that one has to go beyond the confines of the familiar Clifford algebra Cl(1,3)Cl(1,3).

Learning from the above experience that we arrived at Cl(1,3)Cl(1,3) via splitting the “imaginary number” II into four γa\gamma_{a} operators in (3), we may go one step further by decomposing Dirac’s gamma zero operator γ0\gamma_{0} into its underlying components [27]

γ0\displaystyle\gamma_{0}\ =Γ1Γ2Γ3,\displaystyle=\Gamma_{1}\Gamma_{2}\Gamma_{3}, (7)

where the additional trio of gamma operators {Γ1\Gamma_{1}, Γ2\Gamma_{2}, Γ3\Gamma_{3}} satisfy the anticommutation relations

{Γi,Γj}=ΓiΓj+ΓjΓi=2δij,\displaystyle\{\Gamma_{i},\Gamma_{j}\}=\Gamma_{i}\Gamma_{j}+\Gamma_{j}\Gamma_{i}=-2\delta_{ij}, (8)

and anticommute with Dirac’s original trio {γ1\gamma_{1}, γ2\gamma_{2}, γ3\gamma_{3}}

{γi,Γj}=γiΓj+Γjγi=0.\displaystyle\{\gamma_{i},\Gamma_{j}\}=\gamma_{i}\Gamma_{j}+\Gamma_{j}\gamma_{i}=0. (9)

Collectively, these six elements

Γ1,Γ2,Γ3,γ1,γ2,γ3,\displaystyle\Gamma_{1},\Gamma_{2},\Gamma_{3},\gamma_{1},\gamma_{2},\gamma_{3}, (10)

constitute the orthonormal vector basis of the real Clifford algebra Cl(0,6)Cl(0,6), which is sometimes labeled as Cl0,6Cl_{0,6} or Cl0,6(R)Cl_{0,6}(R) in the literature. Note that while the Clifford algebra has been extended, in our model we assume that the underlying space-time manifold remains 4-dimensional.

Thanks to the recognition of γ0\gamma_{0} as a composite tri-vector, we are able to extend Dirac’s Clifford algebra from Cl(1,3)Cl(1,3) to Cl(0,6)Cl(0,6), with Cl(1,3)Cl(1,3) being a sub-algebra of Cl(0,6)Cl(0,6). With it, we can define an algebraic spinor as a linear combination of all 26=642^{6}=64 basis elements of Cl(0,6)Cl(0,6). Considering that there are 16 Weyl fermions with 16×2=3216\times 2=32 complex components (i.e. 6464 real components) within each of the three fermion families including the right-handed neutrino, an algebraic spinor of the real Cl(0,6)Cl(0,6) with 64 real degrees of freedom is a perfect match for representing one generation of fermions.

The geometrical wealth of Clifford algebra Cl(0,6)Cl(0,6) can be exploited to establish a unified theory of gravity and the standard model [27, 29, 30] based on two central tenets: gauge symmetry and quantum condensation. The tenet of gauge symmetry stipulates that both Lorentz and internal symmetries should be treated on an equal footing as gauge symmetries, while the tenet of quantum condensation dictates that the fundamental energy scales of the universe such as the Planck scale are emergent and resulted from multi-spinor quantum condensation which is an ordered quantum phase induced by the dynamical symmetry breaking mechanism.

According to the central tenet of gauge symmetry, the spin connection Lorentz gauge field governing gravity and the Yang-Mills gauge fields governing the standard model interactions are associated with beyond the standard model (BSM) symmetries

Spin(1,3)L×Spin(1,3)R×Spin(1,3)WL×Spin(1,1)WR×U(1)WR\displaystyle Spin(1,3)_{L}\times Spin(1,3)_{R}\times Spin(1,3)_{WL}\times Spin(1,1)_{WR}\times U(1)_{WR}
×SU(3)C×U(1)BL,\displaystyle\times SU(3)_{C}\times U(1)_{B-L}, (11)

where Spin(1,3)LSpin(1,3)_{L} and Spin(1,3)RSpin(1,3)_{R} are the left- and right-handed local Lorentz gauge groups, and the extended left-handed weak gauge group Spin(1,3)WLSpin(1,3)_{WL} encompasses the standard model left-handed weak gauge group SU(2)WLSU(2)_{WL}.

The BSM symmetries (11) are accompanied by an extended vierbein valued in a 16-dimensional multivector subspace of Cl(0,6)Cl(0,6) as opposed to the traditional vierbein (5) valued in the 4-dimensional vector space of Cl(1,3)Cl(1,3). The extended vierbein transforms as a vector under both Lorentz and the extended weak Spin(1,3)WLSpin(1,3)_{WL} gauge transformations. Therefore, a new kind of gravi-weak interplay is permitted between the extended vierbein and the extended weak gauge field. This gravi-weak interplay is otherwise impossible since the traditional vierbein is invariant under the weak SU(2)WLSU(2)_{WL} gauge transformation. Note that the gravi-weak interplay is not in conflict with the Coleman-Mandula theorem [40], since there is no nontrivial mixing between the Lorentz groups (Spin(1,3)LSpin(1,3)_{L} and Spin(1,3)RSpin(1,3)_{R}) and the internal gauge groups including the extended weak group Spin(1,3)WLSpin(1,3)_{WL}.

According to the second central tenet of quantum condensation, we investigate the vierbein field e^μ\hat{e}_{\mu} as a composite entity emerging from a Cooper-pair-like fermion-antifermion quantum condensation via the dynamical symmetry breaking mechanism. Hence the standard model fermion fields are the origin of space-time metric. Given that vierbein can be viewed as the “square root” of metric, the standard model fermions can be considered as the “quarter root” of metric, which speaks to the fact that fermions have spin 1/21/2 while gravitons have spin 22. Consequently, quantum gravity is realized indirectly via the quantized standard model spinor fields which underlie the composite space-time metric. Note that due to the chirality of the vierbein-related condensations and the chirality of spin connection fields associated with left- and right-handed local Lorentz gauge groups Spin(1,3)LSpin(1,3)_{L} and Spin(1,3)RSpin(1,3)_{R}, there are left- and right-handed gravitational interactions.

We propose that all the regular Lagrangian terms, be it the fermion kinetic term or gravity and cosmological constant terms, are of quantum condensation origin. Therefore, both the Planck scale and the cosmological constant scale are emergent and resulted from quantum condensations. We advocate a multi-scale renormalization procedure for quantum condensation, which is a paradigm shift from the conventional QFT renormalization approach (or the Wilsonian renormalization group approach) characterized by a single renormalization scale. The cosmological constant problem can thus be evaded if we exercise extreme caution in the renormalization procedure that entails multiplications of divergent Feynman integrals.

It’s worth mentioning that Clifford algebra Cl(0,6)Cl(0,6) is capable of accommodating enveloping groups larger than the BSM groups (11). For example, the spin group Spin(4,4)Spin(4,4) and the real symplectic group Sp(8,R)Sp(8,R) are embedded in the Cl(0,6)Cl(0,6) geometric structure. The Lorentz gauge group Spin(1,3)Spin(1,3) and the extended weak group Spin(1,3)WLSpin(1,3)_{WL} are two commuting subgroups of Spin(4,4)Spin(4,4). The Pati-Salam’s SU(4)SU(4) [41], which is a subgroup of the real symplectic group Sp(8,R)Sp(8,R), is isomorphic to the six-dimensional rotation group Spin(6)Spin(6). We settle for a parsimonious set of subgroups (11) due to chirality considerations and lack of experimental evidence (such as proton decay) supporting any larger unification groups such as SU(4)SU(4), whereas there are various clues suggestive of the BSM symmetries (11).

According to the conventional wisdom, the usual candidates for gauge transformations are bi-vector-related rotations. Thus the symmetry group of Cl(0,6)Cl(0,6) seems to be restricted to Spin(6)Spin(6)/SO(6)SO(6) generated by all the 15 bi-vectors of Cl(0,6)Cl(0,6). Then how can Cl(0,6)Cl(0,6) accommodate the BSM symmetries discussed above? This is because of two advantages of the Clifford algebra approach that are not enjoyed by the conventional approach. First of all, the permissible group generators of the Clifford algebra approach could involve both bi-vector and non-bi-vector Clifford elements, generalizing the traditional notion of bi-vector rotations. For example, the Lorentz boosts and the left-handed weak-boosts are generated by Cl(0,6)Cl(0,6) 4-vectors rather than bi-vectors.

Secondly, a Clifford algebraic spinor ψ\psi allows double-sided gauge transformations

ψVψU,\psi\quad\rightarrow\quad V\psi U, (12)

where transformations VV and UU are independent of each other. And by definition, VV and UU commute with each other. Specifically, the gravi-weak symmetries in (11) (the Lorentz gravity Spin(1,3)L×Spin(1,3)RSpin(1,3)_{L}\times Spin(1,3)_{R} and the extended weak symmetries Spin(1,3)WL×Spin(1,1)WR×U(1)WRSpin(1,3)_{WL}\times Spin(1,1)_{WR}\times U(1)_{WR}) belong to the left-sided gauge transformation VV, while the color and B-L symmetries in (11) (SU(3)C×U(1)BLSU(3)_{C}\times U(1)_{B-L}) belong to the right-sided gauge transformation UU. These double-sided gauge transformations are otherwise impossible in the conventional column fermion formalism. Note that the left-handed and right-handed fermions transform independently under the chiral left-sided gauge transformations Spin(1,3)L×Spin(1,3)WLSpin(1,3)_{L}\times Spin(1,3)_{WL} and Spin(1,3)R×Spin(1,1)WR×U(1)WRSpin(1,3)_{R}\times Spin(1,1)_{WR}\times U(1)_{WR} respectively, whereas the left-handed and right-handed fermions transform in unison under the right-sided gauge transformations SU(3)C×U(1)BLSU(3)_{C}\times U(1)_{B-L}.

All in all, the above two features of the Clifford algebra approach are the underlying mechanism which enables us to explore symmetries that go beyond the conventional approach.

In this paper, we present a detailed account of how BSM symmetries (11) are broken by a cascade of symmetry breaking processes, triggered by the nonzero vacuum expectation values (VEV) acquired by the Clifford-valued vierbeins and Higgs fields. The first stage of symmetry breaking starts with the vierbeins acquiring nonzero flat space-time VEVs, or equivalently with the metric gμνg_{\mu\nu} acquiring the Minkowski VEV ημν\eta_{\mu\nu}. As a result, the pseudo-weak gauge symmetry (the coset Spin(1,3)WL/SU(2)WLSpin(1,3)_{WL}/SU(2)_{WL} and Spin(1,1)WRSpin(1,1)_{WR}) , local Lorentz gauge symmetry and diffeomorphism symmetry are lost. The residual gauge symmetries are SU(2)WL×U(1)WR×SU(3)C×U(1)BLSU(2)_{WL}\times U(1)_{WR}\times SU(3)_{C}\times U(1)_{B-L}, plus a remnant global Lorentz symmetry which is the synchronization of the global portion of Lorentz gauge and diffeomorphism symmetries.

The next step of symmetry breaking is triggered by the Majorana-Higgs field, which is a Higgs-like field in addition to the standard model Higgs field. At this stage, the Majorana-Higgs field assumes a nonzero VEV and breaks the local gauge symmetries down to the standard model symmetries SU(3)C×SU(2)WL×U(1)YSU(3)_{C}\times SU(2)_{WL}\times U(1)_{Y}. Consequently, the neutrino is endowed with a lepton number-conserving Majorana mass which is much heavier than the Dirac mass. A very small effective mass can thus be derived for the neutrino via the seesaw mechanism [42].

At the last stage of symmetry breaking, the standard model electroweak Higgs field acquires nonzero VEV and breaks the standard model symmetries down to SU(3)C×U(1)EMSU(3)_{C}\times U(1)_{EM}, where U(1)EMU(1)_{EM} is the electromagnetic gauge symmetry. In the context of spontaneous breaking of Peccei-Quinn-like symmetries, the fermion Dirac mass hierarchies can be explained by a three-Higgs-doublet model with the help from reorganizing the lepton-quark configurations of the three generations of standard model fermions. For instance, the first generation electron and neutrino are paired up with the third generation top and bottom quarks (rather than the first generation up and down quarks) to form one unique fermion generation in our model, which is very different from the traditional fermion family assignments.

One point we want to highlight is that all the ingredients of our model, such as fermions, gauge fields, vierbeins, and Higgs fields, share the same Clifford algebraic space of Cl(0,6)Cl(0,6). For instance, the electromagnetic gauge field A^μ\hat{A}_{\mu} is pseudoscalar-valued

A^μ\displaystyle\hat{A}_{\mu} =qAμI,\displaystyle=qA_{\mu}I, (13)

where AμA_{\mu} is real-valued, and we include charge qq (such as q=1q=-1 for electron) in the definition of A^μ\hat{A}_{\mu}. The pseudoscalar II is the 6-vector of Cl(0,6)Cl(0,6) which is the same Cl(1,3)Cl(1,3) pseudoscalar II in Eq. (3) after expanding the tri-vector γ0\gamma_{0} into its constituents

I\displaystyle I =γ0γ1γ2γ3=Γ1Γ2Γ3γ1γ2γ3.\displaystyle=\gamma_{0}\gamma_{1}\gamma_{2}\gamma_{3}=\Gamma_{1}\Gamma_{2}\Gamma_{3}\gamma_{1}\gamma_{2}\gamma_{3}. (14)

The electromagnetic gauge field A^μ\hat{A}_{\mu} as shown above and the gravity-related fields ω^μ\hat{\omega}_{\mu}/e^μ\hat{e}_{\mu} in Eq. (5) take values in various Clifford algebraic subspaces with the same six gamma operators {Γ1,Γ2,Γ3,γ1,γ2,γ3}\{\Gamma_{1},\Gamma_{2},\Gamma_{3},\gamma_{1},\gamma_{2},\gamma_{3}\} as the unifying building blocks. The Clifford algebraic gauge field of gravity and Yang-Mills fields are connected with each other through their interactions with the common fermion fields, vierbein fields and Higgs fields, all valued in Clifford algebraic space.

Therefore, the model outlined in this paper is indeed a cohesive unified theory of the standard model and gravity. Note that the Clifford algebra approach differs from the conventional grand unified theories (GUTs) [43, 44, 45, 46, 47] and gravi-GUTs [48, 49, 50, 51, 52, 53, 54, 55, 56] which demand that the gauge coupling constants should be unified. In the Clifford algebra approach, the allowable symmetries are the ones that preserve the invariance properties of spinor bilinears. Hence the symmetries of the model are in a sense derived rather than postulated. The permitted symmetries usually involve a direct product of different groups, suggesting that the individual gauge coupling constants are not necessarily related to each other. To a certain extent, the Clifford algebra approach as advocated here predicts the unpredictability of Weinberg angle θW\theta_{W}. As such, the fusion delineated in this paper is more of a unification via spinors and less of a unification via symmetry groups.

This paper is structured as follows: In Section 2, we introduce the algebraic spinors of Cl(0,6)Cl(0,6) and explore beyond the standard model gauge symmetries. In Section 3, we investigate spontaneous symmetry breaking due to the non-degenerate vacuum expectation values of various bosonic fields, and study the fermion mass hierarchies and the lepton number-conserving Majorana mass. In Section 4, we contemplate naturalness problems through the lens of quantum condensations and examine the extended gauge symmetries which enable gravi-weak interaction. In the last section we draw our conclusions. Throughout this paper, we adopt the natural units c==1c=\hbar=1.

2 Clifford Algebra Cl(0,6) and Gauge Symmetries

In this section, we introduce algebraic spinors of the real Clifford algebra Cl(0,6)Cl(0,6) and explore beyond the standard model gauge symmetries. We proceed with expressing the gauge fields and curvatures as multivectors of Cl(0,6)Cl(0,6). We round out the section with a detailed formulation of the Lagrangian of the algebraic spinors, as well as the Lagrangian of the Yang-Mills and gravitational interactions in terms of Clifford algebra.

Note that the complexified Clifford algebra Cl(6,C)Cl(6,C) [57, 58, 59, 60, 61, 62, 63, 64, 65, 66, 67, 68, 69, 70, 71] and its isomorphic equivalences such as Cl(7,0)Cl(7,0) [16] and the complex 8×88\times 8 matrix M(8,C)M(8,C) algebra [72], either as standalone algebra or in association with octonions or sedenions, have been investigated in connection with the color SU(3)cSU(3)_{c} symmetry and the other standard model symmetries. Nevertheless, in our approach [27, 29, 30] we choose to stick with the real Cl(0,6)Cl(0,6) which is based on two reasons: The first reason is that an algebraic spinor of the real Cl(0,6)Cl(0,6) with 64 real basis elements is a perfect match with one generation of 16 Weyl fermions (including the right-handed neutrino) in the standard model with 32 complex degrees of freedom (i.e. 6464 real degrees of freedom).

The second reason for choosing the real Cl(0,6)Cl(0,6) is that we regard the spinor and gauge fields as classical fields prior to field quantization. As explained in the introduction section, we consign the imaginary number ii to the realm of quantum theory. Therefore, the imaginary number ii should play no role in the definition of the classical spinor fields, gauge fields and their symmetry transformations, as demonstrated by the replacement of imaginary number ii with the pseudoscalar II in the electromagnetic U(1)U(1) gauge transformation (2). In our model, we rigorously enforce the rule of avoiding the quantum ii in the definition of classical spinors, gauge fields, and the corresponding gauge-covariant derivatives. Note that we can nonetheless maintain a “pseudo-complex representation” with the pseudoscalar II acting as the surrogate imaginary number. As a side note, in our earlier papers [27, 29, 30] we have used notations for imaginary number (denoted as i^\hat{i}) and pseudoscalar (denoted as ii) which are different from notations in the current paper.

Pioneered by Hestenes [1], one original objective of the Clifford algebra approach to physics is to abandon the imaginary number altogether and replace it with certain element of Clifford algebra. The endeavor of using an effective operator to proxy the imaginary number has been fairly successful in a wide variety of physics domains [11, 15, 73, 20]. However, it has been realized [30, 31] that the initiative championed by Hestenes has its limitations: When it comes to field quantization and quantum loop integral calculations, the imaginary number is indispensable and can not be replaced by a Clifford element. For example, a self-energy loop diagram would yield an imaginary-valued quantum correction due to proper contour integral on the complex plane of Feynman propagators. Therefore, in Section 4 on field quantization, we will formally introduce the imaginary number ii in the Clifford functional integral formalism [31] when we study quantum phenomena. In the same Section 4, we will try to demystify the unexpected appearance of the imaginary number ii in the classical fermion Lagrangian as the quantum fingerprint left on the classical world.

It is worth noting that the real 6-D Clifford algebra has 7 different signatures: Clifford algebras Cl(0,6)Cl(0,6), Cl(3,3)Cl(3,3) and Cl(4,2)Cl(4,2) are isomorphic to the real 8×88\times 8 matrix M(8,R)M(8,R) algebra. On the other hand, Clifford algebras Cl(6,0)Cl(6,0), Cl(5,1)Cl(5,1), Cl(2,4)Cl(2,4) and Cl(1,5)Cl(1,5) are isomorphic to the quaternion 4×44\times 4 matrix M(4,H)M(4,H) algebra. In the literature [74], the merits of various signatures of Clifford algebras have been discussed in connection with the standard model symmetries.

Given the isomorphisms noted above, the Cl(0,6)Cl(0,6)-based model can be faithfully translated to the Cl(3,3)Cl(3,3), Cl(4,2)Cl(4,2) or M(8,R)M(8,R) format, which would be basically the equivalent model. For example, in terms of the Cl(0,6)Cl(0,6) orthonormal vector basis {Γ1,Γ2,Γ3,γ1,γ2,γ3}\{\Gamma_{1},\Gamma_{2},\Gamma_{3},\gamma_{1},\gamma_{2},\gamma_{3}\}, the orthonormal vector bases of Cl(3,3)Cl(3,3) and Cl(4,2)Cl(4,2) are {Γ0Γ1,Γ0Γ2,Γ0Γ3,γ1,γ2,γ3}\{\Gamma_{0}\Gamma_{1},\Gamma_{0}\Gamma_{2},\Gamma_{0}\Gamma_{3},\gamma_{1},\gamma_{2},\gamma_{3}\} and {γ1γ0,γ2γ0,γ3γ0,Γ0,Γ1,Γ2}\{\gamma_{1}\gamma_{0},\gamma_{2}\gamma_{0},\gamma_{3}\gamma_{0},\Gamma_{0},\Gamma_{1},\Gamma_{2}\} respectively, where γ0=Γ1Γ2Γ3\gamma_{0}=\Gamma_{1}\Gamma_{2}\Gamma_{3} and Γ0=γ1γ2γ3\Gamma_{0}=\gamma_{1}\gamma_{2}\gamma_{3}. As such, the time-like γ0\gamma_{0} can be defined as the 6-vector (pseudoscalar) of Cl(3,3)Cl(3,3), whereas γ0\gamma_{0} can be defined as the 4-vector (product of the first 4 vectors) of Cl(4,2)Cl(4,2). The mapping between Cl(0,6)Cl(0,6) and M(8,R)M(8,R) can also be worked out, which will not be explored here in this paper since the physics essence of our model has already been elegantly captured by the purely Clifford algebraic formalism.

2.1 The algebraic spinor representation of fermions

As mentioned in the introduction section, one generation of the standard model fermions can be represented by the algebraic spinor of Clifford algebra Cl(0,6)Cl(0,6) [27, 29, 30]. The goal of this subsection is to demonstrate how individual fermions, such as electrons, neutrinos, and quarks, are linked to the algebraic spinor without resorting to the traditional column representation of fermions. Note that this subsection concerns the classical spinor field, while quantization of spinor field will be introduced in Section 4. Following our principle stated earlier, in this subsection we strictly enforce the regime of not allowing the imaginary number ii in the definition of the classical algebraic spinor and the projections thereof. Therefore, we are ensured to stay within the real Cl(0,6)Cl(0,6) algebraic space.

For Cl(0,6)Cl(0,6), there are (6k){\binom{6}{k}} independent kk-vectors. To wit, there are one single scalar 11 which is a 0-vector, 6 vectors (e.g. γ1\gamma_{1}), 15 bi-vectors (e.g. γ1γ2\gamma_{1}\gamma_{2}), 20 tri-vectors (e.g. γ0=Γ1Γ2Γ3\gamma_{0}=\Gamma_{1}\Gamma_{2}\Gamma_{3}), 15 4-vectors (e.g. γ1γ2I=Γ1Γ2Γ3γ3\gamma_{1}\gamma_{2}I=-\Gamma_{1}\Gamma_{2}\Gamma_{3}\gamma_{3}), 6 5-vectors (e.g. γ1I=Γ1Γ2Γ3γ2γ3\gamma_{1}I=\Gamma_{1}\Gamma_{2}\Gamma_{3}\gamma_{2}\gamma_{3}), and finally one single pseudoscalar I=Γ1Γ2Γ3γ1γ2γ3I=\Gamma_{1}\Gamma_{2}\Gamma_{3}\gamma_{1}\gamma_{2}\gamma_{3} which is a 6-vector. In total, there are 26=642^{6}=64 independent basis elements given by the set of all kk-vectors. The algebraic spinor ψ\psi is a multivector which can be expressed as a linear combination of all the 6464 basis elements

ψ=\displaystyle\psi= ψ1+ψ2Γ1+ψ3Γ2++ψ62Γ2I+ψ63Γ1I+ψ64I,\displaystyle\psi_{1}+\psi_{2}\Gamma_{1}+\psi_{3}\Gamma_{2}+\cdots+\psi_{62}\Gamma_{2}I+\psi_{63}\Gamma_{1}I+\psi_{64}I, (15)

where the 64 linear combination coefficients {ψn;n=1,2,,64}\{\psi_{n};n=1,2,\cdots,64\} are real Grassmann numbers (with ψnψm+ψmψn=0\psi_{n}\psi_{m}+\psi_{m}\psi_{n}=0 and ψn\psi_{n} commuting with all 64 Clifford algebra Cl(0,6) basis elements) satisfying the complex conjugation relation

ψn=\displaystyle\psi_{n}^{*}= ψn.\displaystyle\psi_{n}. (16)

As we noted in the introduction section, while the Clifford algebra has been extended to Cl(0,6)Cl(0,6), the underlying space-time manifold remains 4-dimensional. Therefore, if we write out the coordinate xx explicitly for the algebraic spinor ψ(x)\psi(x), xx still represents the 4-dimensional space-time. Also note that the fermionic algebraic spinor as expressed in (15) should not be confused with a bispinor, which is effectively bosonic (Grassmann-even) and can be also expanded in terms of the 64 elements of Cl(0,6)Cl(0,6). While the bosonic bispinor components may transform as Lorentz scalar/pseudoscalar/vector/tensor, it should be emphasized that the fermionic Grassmann-odd algebraic spinor ψ\psi transforms as a spinor only, albeit ψ\psi comprises all the Cl(0,6)Cl(0,6) basis elements. We will revisit the important subject of bosonic bispinors in later sections when we investigate scalar/tensor Higgs fields and (extended) vector vierbein fields as effective descriptions of bispinors.

A few comments are in order at this point regarding the real Grassmann numbers ψn\psi_{n}. First of all, due to the fermion nature of the algebraic spinor ψ\psi, it’s mandatory that ψn\psi_{n} should be Grassmann-odd. This requirement is not obvious when we write down the Dirac equation for ψ\psi, where there is no multiplication between spinors. In other words, defining ψn\psi_{n} as real number or as real Grassmann number does not make any difference as long as there is no multiplication between spinors. However, the Grassmann-odd characteristic of ψ\psi becomes essential when it comes to the Lagrangian involving multiplication between spinors. Since we are going to use the Lagrangian format to investigate multi-fermion condensations extensively in our model, we are compelled to employ the real Grassmann ψn\psi_{n}. As we will learn later in this paper, the Majorana mass Lagrangian term is allowed only if the algebraic spinor is Grassmann-odd, or otherwise the Majorana mass Lagrangian term is identically zero.

Secondly, it’s customary to adopt complex Grassmann numbers in the conventional QFT where the reality condition (16) does not hold. The way to make contact with the conventional complex Grassmann numbers is to reorganize ψn\psi_{n} in pairs, such as

ψ1+ψ64I,\displaystyle\psi_{1}+\psi_{64}I, (17)

where pseudoscalar II is acting as a proxy for the imaginary number ii. Therefore, the combination ψ1+ψ64I\psi_{1}+\psi_{64}I is tantamount to the conventional complex Grassmann number. Another example is the ψ2Γ1+ψ63Γ1I\psi_{2}\Gamma_{1}+\psi_{63}\Gamma_{1}I pair, which can be rewritten as Γ1(ψ2+ψ63I)\Gamma_{1}(\psi_{2}+\psi_{63}I). Hence ψ2+ψ63I\psi_{2}+\psi_{63}I is the proxy “complex” Grassmann number. Note that pseudoscalar II has to appear on the right side of Γ1\Gamma_{1}. We will come back to this point a bit later.

The algebraic spinor ψ\psi of the real Cl(0,6)Cl(0,6) with 26=642^{6}=64 real components corresponds to the union of all 16 Weyl fermions in one fermion generation of the standard model (plus right-handed neutrino) endowed with 16×2=3216\times 2=32 complex components (i.e. 6464 real components). For most part of this paper, our discussion is restricted to one generation/family of fermions. The Clifford algebraic structure of the fermions as well as the gauge symmetries are the same for the three generations. In other words, the three families are three replicas. That said, in Section 3.4 on the fermion mass hierarchy, we will propose three electroweak symmetry-breaking Higgs fields that couple to the three generations of fermions in different patterns.

How do we connect one generation of fermions, such as electrons, neutrinos, and quarks with ψ\psi? First of all, let’s distinguish between the left-handed and right-handed fermions in the setting of Clifford algebra. We propose that fermions with left (right) chirality correspond to Clifford-odd (even) portion of the algebraic spinor [27]

ψL\displaystyle\psi_{L} =12(ψ+IψI),\displaystyle=\frac{1}{2}(\psi+I\psi I), (18)
ψR\displaystyle\psi_{R} =12(ψIψI).\displaystyle=\frac{1}{2}(\psi-I\psi I). (19)

That is to say, the left-handed ψL\psi_{L} is composed of 6 vectors, 20 tri-vectors, and 6 5-vectors (32 degrees of freedom in total)

ψL\displaystyle\psi_{L} =ψ2Γ1++ψ63Γ1I\displaystyle=\psi_{2}\Gamma_{1}+\cdots+\psi_{63}\Gamma_{1}I (20)

whilst the right-handed ψR\psi_{R} is composed of one scalar, 15 bi-vectors, 15 4-vectors, and one pseudoscalar (32 degrees of freedom in total)

ψR\displaystyle\psi_{R} =ψ1++ψ64I,\displaystyle=\psi_{1}+\cdots+\psi_{64}I, (21)

The projection of Clifford-odd (even) portion of ψ\psi leverages the property that the pseudoscalar II anticommutes with Clifford-odd elements, and commutes with Clifford-even elements

IψL\displaystyle I\psi_{L} =ψLI,\displaystyle=-\psi_{L}I,
IψR\displaystyle I\psi_{R} =ψRI.\displaystyle=\psi_{R}I.

The operation of IψI-I\psi I as in Eq. (19) can be mapped to the traditional γ5ψ\gamma^{5}\psi operation, where I-I as in Iψ-I\psi plays the role of the conventional pseudoscalar (more discussion will be provided on the minus sign of I-I in Section 3.1), while II as in ψI\psi I plays the role of the conventional imaginary number ii. Note that the positioning of II relative to the algebraic spinor ψ\psi does matter. This speaks to the fact that the electromagnetic field, as a pseudoscalar in Eq. (13), should always be applied to the right side of a spinor so that II is equivalent to the imaginary number ii in the traditional setting. And for that matter, when we attempt to connect the real Grassmann numbers in our model with the traditional complex Grassmann numbers, we ought to make sure that the surrogate “imaginary number” II should always appear on the right side of any Clifford element.

We would like to emphasize that being Grassmann-odd/even and being Clifford-odd/even are two separate notions. Fermionic spinor fields are Grassmann-valued, while bosonic fields including gauge and Higgs fields are real-valued. On the other hand, being fermion or boson has no bearing on being Clifford-odd/even. For instance, according to the above spinor chirality definition, the left-handed spinor ψL\psi_{L} is Clifford-odd, while the right-handed spinor ψR\psi_{R} is Clifford-even. And we will learn later that the bosonic fields can also be either Clifford-odd or Clifford-even. For example, the bosonic Majorana-Higgs field and the bosonic vierbein field are both Clifford-odd, while the other bosonic fields such as the standard model Higgs field and all the gauge fields are Clifford-even.

Now we are ready to identify ψ\psi with electrons, neutrinos, and quarks. Specifically, the projection operators for the three colors of red, green, and blue quarks are given by
Pr\displaystyle P_{r} =14(1+Iγ1Γ1Iγ2Γ2Iγ3Γ3),\displaystyle=\frac{1}{4}(1+I\gamma_{1}\Gamma_{1}-I\gamma_{2}\Gamma_{2}-I\gamma_{3}\Gamma_{3}), (22a)
Pg\displaystyle P_{g} =14(1Iγ1Γ1+Iγ2Γ2Iγ3Γ3),\displaystyle=\frac{1}{4}(1-I\gamma_{1}\Gamma_{1}+I\gamma_{2}\Gamma_{2}-I\gamma_{3}\Gamma_{3}), (22b)
Pb\displaystyle P_{b} =14(1Iγ1Γ1Iγ2Γ2+Iγ3Γ3),\displaystyle=\frac{1}{4}(1-I\gamma_{1}\Gamma_{1}-I\gamma_{2}\Gamma_{2}+I\gamma_{3}\Gamma_{3}), (22c)
while the lepton projection operator is defined as
Pl\displaystyle P_{l} =14(1+Iγ1Γ1+Iγ2Γ2+Iγ3Γ3).\displaystyle=\frac{1}{4}(1+I\gamma_{1}\Gamma_{1}+I\gamma_{2}\Gamma_{2}+I\gamma_{3}\Gamma_{3}). (22d)

In the context of SU(4)SU(4), the lepton projection operator PlP_{l} can be regarded as the projection to the fourth color [41]. Leveraging the fact that II can be factorized into the 6 Cl(0,6)Cl(0,6) vectors (14), it can be readily verified that the four color projections PlP_{l}, PrP_{r}, PgP_{g}, PbP_{b} are orthogonal to each other and satisfy

Pl+Pr+Pg+Pb=Pl+Pq=1,\displaystyle P_{l}+P_{r}+P_{g}+P_{b}=P_{l}+P_{q}=1, (23)

where Pq=Pr+Pg+PbP_{q}=P_{r}+P_{g}+P_{b} is the quark projection operator. Note that the bi-vectors γiΓi\gamma_{i}\Gamma_{i} appearing in the color projectors suggest an interesting interplay between the trialities of {γ1\gamma_{1}, γ2\gamma_{2}, γ3\gamma_{3}}/{Γ1\Gamma_{1}, Γ2\Gamma_{2}, Γ3\Gamma_{3}} and three colors of quarks. Figuratively speaking, the three colors of quarks go hand in hand with the three space dimensions. In Section 2.2, we will further explore the significance of these color projectors in terms of carving out the color group SU(3)CSU(3)_{C} from Pati-Salam’s SU(4)SU(4). It’s worth mentioning that the color projectors can be equivalently expressed via products of idempotents 12(1±γ0γiΓi)\frac{1}{2}(1\pm\gamma_{0}\gamma_{i}\Gamma_{i}) [27], which will not be detailed here.

For the purpose of differentiating between weak isospin up-type and down-type fermions, we introduce another set of orthogonal projection operators

P±=12(1±IΓ1Γ2),\displaystyle P_{\pm}=\frac{1}{2}(1\pm I{\Gamma_{1}}{\Gamma_{2}}), (24)

which sum up to

P++P=1.\displaystyle P_{+}+P_{-}=1. (25)

We identify projections of the algebraic spinor ψ\psi

ψ=ψL+ψR=(P++P)(ψL+ψR)(Pl+Pr+Pg+Pb),\psi=\psi_{L}+\psi_{R}=(P_{+}+P_{-})(\psi_{L}+\psi_{R})(P_{l}+P_{r}+P_{g}+P_{b}), (26)

with left-handed neutrino, electron, and quarks

{νL=P+ψLPl,uL,r=P+ψLPr,uL,g=P+ψLPg,uL,b=P+ψLPb,eL=PψLPl,dL,r=PψLPr,dL,g=PψLPg,dL,b=PψLPb,\left\{\begin{array}[]{rl}\nu_{L}&=P_{+}\psi_{L}P_{l},\\ u_{L,r}&=P_{+}\psi_{L}P_{r},\quad u_{L,g}=P_{+}\psi_{L}P_{g},\quad u_{L,b}=P_{+}\psi_{L}P_{b},\\ e_{L}&=P_{-}\psi_{L}P_{l},\\ d_{L,r}&=P_{-}\psi_{L}P_{r},\quad d_{L,g}=P_{-}\psi_{L}P_{g},\quad d_{L,b}=P_{-}\psi_{L}P_{b},\end{array}\right. (27)

and right-handed neutrino, electron, and quarks

{νR=PψRPl,uR,r=PψRPr,uR,g=PψRPg,uR,b=PψRPb,eR=P+ψRPl,dR,r=P+ψRPr,dR,g=P+ψRPg,dR,b=P+ψRPb.\left\{\begin{array}[]{rl}\nu_{R}&=P_{-}\psi_{R}P_{l},\\ u_{R,r}&=P_{-}\psi_{R}P_{r},\;\;\;u_{R,g}=P_{-}\psi_{R}P_{g},\;\;\;u_{R,b}=P_{-}\psi_{R}P_{b},\\ e_{R}&=P_{+}\psi_{R}P_{l},\\ d_{R,r}&=P_{+}\psi_{R}P_{r},\;\;\;d_{R,g}=P_{+}\psi_{R}P_{g},\;\;\;d_{R,b}=P_{+}\psi_{R}P_{b}.\end{array}\right. (28)

Since the algebraic spinor ψ\psi of Cl(0,6)Cl(0,6) has 26=642^{6}=64 real components, each of the above 16 distinctive projections possesses 4 real degrees of freedom, matching with the 16 standard model Weyl fermions with each having 22 complex components (i.e. 44 real degrees of freedom).

Note that the definition of isospin I3I_{3} for a given standard model fermion ψf\psi_{f} is given by

ψf(I3I)=12Γ1Γ2ψf.\displaystyle\psi_{f}(I_{3}I)=\frac{1}{2}\Gamma_{1}\Gamma_{2}\psi_{f}. (29)

With the help from the property that

Γ1Γ2P±ψf=IP±ψf,\displaystyle\Gamma_{1}\Gamma_{2}P_{\pm}\psi_{f}={\mp}IP_{\pm}\psi_{f}, (30)

it can thus be verified that the isospin values of the fermions in Eq. (27) and Eq. (28) are consistent with those of the standard model. When the II in Eq. (30) appearing on the left side of ψf\psi_{f} is moved to the right side of ψf\psi_{f} as in Eq. (29), its sign is changed for the Clifford-odd left-handed fermions. This is the underlying reason why there is a flip of sign in P±P_{\pm} between the left- and right-handed fermions when P±P_{\pm} is assigned to the isospin up-type and down-type fermions respectively in Eq. (27) and Eq. (28).

It’s also worth mentioning that attempts have been made to associate species of fermions with minimal left ideals of the Clifford algebraic spinor where projection operators are restricted to acting on the right side of an algebraic spinor. Obviously, our fermion assignment scheme above departs from the minimal left ideal approach, given that the projection operators used to identify the standard model fermions are applied on both the right side and the left side of the algebraic spinor in Eq. (27) and Eq. (28).

In summary, we have identified individual fermions with the projections of the Cl(0,6)Cl(0,6) algebraic spinor without any reference to the column representation. And for that matter, there will not be a single expression of matrix or column in our model. In other words, every expression discussed in our model is purely algebra-based. Nevertheless, the mappings between the Cl(0,6)Cl(0,6) formalism and the conventional matrix/column representation can be worked out [27], which will not be detailed in this paper.

2.2 Beyond the standard model symmetries

As explained in the introduction section, we strive to walk a careful line between being too ambitious and being too conservative when it comes to choosing the suitable gauge symmetries for our model. The aim of this subsection is to give an account of our thought process in selecting the BSM symmetry groups employed in this paper. The in-depth investigation of the Clifford-valued gauge fields corresponding to these symmetries will be presented in Section 2.4, while the details of the spontaneous symmetry breaking process will be examined in Section 3.

The conventional way of model building is to postulate the symmetry group upfront, and then proceed to find the fermion representation. In the case of Clifford algebra approach, it’s the other way around. We choose the Clifford algebra Cl(0,6)Cl(0,6) as the first step which is tantamount to staking out the fermion space. The allowable symmetry groups are thus tightly constrained by the spinor space. This is a desirable feature of the Clifford algebra approach, since the symmetry groups are in a sense derived, rather than postulated.

So how do we determine the allowable symmetries? It hinges on the invariance property of spinor bilinear

ψ¯ψ1,I,\displaystyle\left\langle\bar{\psi}\psi\right\rangle_{1,I}, (31)

where 1,I\left\langle\ldots\right\rangle_{1,I} stands for the Clifford-scalar and -pseudoscalar parts of the enclosed expression. It is the Clifford algebraic counterpart of the conventional Dirac inner product ψ¯ψ\bar{\psi}\psi between the column spinors. For the rest of the paper, we will exclusively use \left\langle\ldots\right\rangle which stands for the Clifford-scalar part of the enclosed expression, since we can get the pseudoscalar part via I\left\langle I\ldots\right\rangle if needed. The Dirac conjugate ψ¯\bar{\psi} in Eq. (31) is defined as

ψ¯=ψγ0,\bar{\psi}=\psi^{\dagger}\gamma_{0}, (32)

and the Hermitian conjugate satisfies

(AB)\displaystyle(AB)^{\dagger} =BA,\displaystyle=B^{\dagger}A^{\dagger}, (33)

for any AA and BB valued in the Clifford algebraic space, regardless of AA and BB being Grassmann-even or Grassmann-odd. With the six Cl(0,6)Cl(0,6) basis vectors (10) defined as anti-Hermitian (Γi=Γi\Gamma_{i}^{\dagger}=-\Gamma_{i} and γi=γi\gamma_{i}^{\dagger}=-\gamma_{i}), the Hermitian conjugate of any Clifford element can thus be determined by recursively applying (33). For example,

γ0=(Γ1Γ2Γ3)=Γ3Γ2Γ1=Γ3Γ2Γ1=γ0.{\gamma}^{\dagger}_{0}=(\Gamma_{1}\Gamma_{2}\Gamma_{3})^{\dagger}=\Gamma_{3}^{\dagger}\Gamma_{2}^{\dagger}\Gamma_{1}^{\dagger}=-\Gamma_{3}\Gamma_{2}\Gamma_{1}=\gamma_{0}. (34)

Since the fermion Lagrangian comprises the Dirac inner product ψ¯ψ\left\langle\bar{\psi}\psi\right\rangle or some variants thereof, the allowable symmetry transformations are the ones under which these sorts of Dirac inner products are invariant. Let’s start with investigating the general gauge transformation

ψVψU,\psi\quad\rightarrow\quad V\psi U, (35)

where the Clifford-valued VV and UU are two independent gauge transformations. As an example, the following Dirac inner product transforms as

ψ¯IψI(UψV)γ0I(VψU)I=ψ(Vγ0IV)ψ(UIU),\left\langle\bar{\psi}I\psi I\right\rangle\quad\rightarrow\quad\left\langle(U^{\dagger}\psi^{\dagger}V^{\dagger})\gamma_{0}I(V\psi U)I\right\rangle=\left\langle\psi^{\dagger}(V^{\dagger}\gamma_{0}IV)\psi(UIU^{\dagger})\right\rangle, (36)

which is invariant if

Vγ0IV=γ0I,\displaystyle V^{\dagger}\gamma_{0}IV=\gamma_{0}I, (37)
UIU=I,\displaystyle UIU^{\dagger}=I, (38)

where we have used the property AB=BA\left\langle AB\right\rangle=\left\langle BA\right\rangle provided that A and B are Grassmann-even. If we restrict our discussion to gauge transformations continuously connected to identity, the general solutions of the above equations are

V=eθn(x)Tn,\displaystyle V=e^{\theta^{n}(x)T_{n}}, (39)
U=eϵn(x)Kn,\displaystyle U=e^{\epsilon^{n}(x)K_{n}}, (40)

where {Tn;n=1,,28}\{T_{n};n=1,\cdots,28\} are the generators of the spin group Spin(4,4)Spin(4,4) (double cover of the rotation group SO(4,4)SO(4,4))

γa,γaγb,ΓaΓb,IΓi,γiγjΓk,\gamma_{a},\gamma_{a}\gamma_{b},\Gamma_{a}\Gamma_{b},I\Gamma_{i},\gamma_{i}\gamma_{j}\Gamma_{k}, (41)

and {Kn;n=1,,36}\{K_{n};n=1,\cdots,36\} are the generators of the real symplectic group Sp(8,R)Sp(8,R) (i.e. all 15 bi-vectors, all 20 tri-vectors, and the pseudoscalar)

γiγj,ΓiΓj,γiΓk,γ0,Γ0,γiγjΓk,ΓiΓjγk,I,\gamma_{i}\gamma_{j},\Gamma_{i}\Gamma_{j},\gamma_{i}\Gamma_{k},\gamma_{0},\Gamma_{0},\gamma_{i}\gamma_{j}\Gamma_{k},\Gamma_{i}\Gamma_{j}\gamma_{k},I, (42)

where i,j,k=1,2,3,a,b=0,1,2,3,i>j,a>bi,j,k=1,2,3,a,b=0,1,2,3,i>j,a>b. The tri-vector Γ0\Gamma_{0} is defined as Γ0=γ1γ2γ3\Gamma_{0}=\gamma_{1}\gamma_{2}\gamma_{3}, thus the basis {Γa;a=0,,3}\{\Gamma_{a};a=0,\cdots,3\} parallels {γa;a=0,,3}\{\gamma_{a};a=0,\cdots,3\}. The real-valued transformation parameters θn(x)\theta^{n}(x) and ϵn(x)\epsilon^{n}(x) are space-time dependent, since we are dealing with local gauge transformations. For the sake of brevity, we will omit the xx label hereafter with the understanding that the space-time dependency is implied.

Note that the eθnTne^{\theta^{n}T_{n}} (eϵnKne^{\epsilon^{n}K_{n}}) format of gauge transformation is known as the mathematicians’ convention, whereas in the physicists’ convention the gauge transformations take the form eiθnTne^{i\theta^{n}T_{n}} (eiϵnKne^{i\epsilon^{n}K_{n}}) with an extra ii in front of θnTn\theta^{n}T_{n} (ϵnKn\epsilon^{n}K_{n}). As such, the physicists’ Hermitian Lie group generators are translated into the mathematicians’ anti-Hermitian generators, and vice versa. Following the overarching principle stated earlier, we should stay clear of introducing the quantum imaginary number ii in the definition of classical fields and their corresponding gauge transformations. Therefore, we choose the mathematicians’ convention where there is no extra ii in the definition of gauge transformations. And for that matter, the identified gauge generators TnT_{n} and KnK_{n} in Eqs. (41) and (42) are also independent of imaginary number ii as demonstrated above.

A few comments are in order. First of all, in the literature the usual candidates for gauge transformations are bi-vector-related rotations. The above TnT_{n} and KnK_{n} involve non-bi-vector Clifford elements such as γ0\gamma_{0} (tri-vector), γi\gamma_{i} (i=1,2,3, vector) and the Lorentz boosts γ0γi\gamma_{0}\gamma_{i} (4-vector) in TnT_{n}, which go beyond the confines of bi-vectors. While the traditional rotation transforms a vector into another vector, the generalized “rotation” via the non-bi-vector-valued Clifford elements could potentially transform vectors into multivectors.

Secondly, the two gauge transformations VV and UU are independent of each other. They are applied to the left side and right side of the algebraic spinor ψ\psi, respectively. Since by definition VV and UU commute with each other, the corresponding symmetry groups are the direct product Spin(4,4)×Sp(8,R)Spin(4,4)\times Sp(8,R) (Spin(4,4)Spin(4,4) commutes with Sp(8,R)Sp(8,R)). The availability of the double-sided gauge transformations is one of the advantages of the Clifford algebra approach compared with the conventional column fermion formalism. This advantage has historically been leveraged in various Clifford algebraic models [16, 12, 19].

One interesting observation is that the 10 generators of de Sitter group SO(1,4)SO(1,4) (or the double cover Spin(1,4)Spin(1,4) when spinors are involved) are contained in TnT_{n} (41), namely

γa,γaγb.\gamma_{a},\gamma_{a}\gamma_{b}. (43)

We know that there is another flavor of gauge gravity theory which is based on (anti-) de Sitter group [75, 76, 77]. It enjoys the desirable property that vierbein e^μ\hat{e}_{\mu} and spin connection ω^μ\hat{\omega}_{\mu} in Eq. (5) jointly constitute the gauge fields of de Sitter group. As a comparison, in Lorentz gauge gravity theory, vierbein e^μ\hat{e}_{\mu} is not a gauge field, albeit spin connection ω^μ\hat{\omega}_{\mu} is indeed the gauge field of Lorentz group. Vierbein is instead regarded as an add-on to Lorentz gauge gravity theory. This incentivized us to adopt de Sitter gauge theory of gravity in our first paper [27] on Clifford algebra Cl(0,6)Cl(0,6). However, there is a downside in this approach: Given that 4 γa\gamma_{a} out of 10 de Sitter group generators in Eq. (43) are Clifford-odd, the associated gauge transformations mix left- and right-handed spinors which are Clifford-odd and -even, respectively. Consequently, the left- and right-handed spinors have to transform in sync, which disagrees with chirality of weak interaction. This is a major shortcoming of our first paper [27] on Clifford algebra Cl(0,6)Cl(0,6).

In our subsequent papers [29, 30], we improved our model and circumvented the above limitation by demanding that only the Clifford-even sub-algebras of TnT_{n} and KnK_{n} are permitted, which enables us to accommodate the chirality of weak interaction by virtue of decoupling the gauge transformations of the left- and right-handed spinors. The trade-off is that we have to settle for the Lorentz gauge gravity theory where vierbein e^μ\hat{e}_{\mu} is an add-on transforming as a vector of the Lorentz symmetry. It is seemingly a disadvantage compared with the de Sitter gauge gravity theory. However, in Sections 4.3 and 4.4 we will learn that it is a blessing in disguise, since the vierbein is never meant to be a fundamental gauge field. It’s actually an emergent quantity arising from quantum condensation.

With the restriction to the Clifford-even sub-algebras of TnT_{n} and KnK_{n}, we are left with the following symmetries [29]

ψLVLψLUL,\displaystyle\psi_{L}\quad\rightarrow\quad V_{L}\psi_{L}U_{L}, (44)
ψRVRψRUR,\displaystyle\psi_{R}\quad\rightarrow\quad V_{R}\psi_{R}U_{R}, (45)

where

VL=eθLnTn,UL=eϵLnKn,\displaystyle V_{L}=e^{\theta_{L}^{n}T_{n}},\quad U_{L}=e^{\epsilon_{L}^{n}K_{n}}, (46)
VR=eθRnTn,UR=eϵRnKn.\displaystyle V_{R}=e^{\theta_{R}^{n}T_{n}},\quad U_{R}=e^{\epsilon_{R}^{n}K_{n}}. (47)

The 6+6=12 Clifford-even {Tn;n=1,,12}\{T_{n};n=1,\cdots,12\} comprise the generators of Spin(1,3)×Spin(1,3)WeakSpin(1,3)\times Spin(1,3)_{Weak}

γaγb;ΓaΓb,\displaystyle\gamma_{a}\gamma_{b};\quad\Gamma_{a}\Gamma_{b}, (48)

where a,b=0,1,2,3,a>ba,b=0,1,2,3,a>b, and the 15+1=16 Clifford-even {Kn;n=1,,16}\{K_{n};n=1,\cdots,16\} comprise the generators of Spin(6)PatiSalam×UI(1)Spin(6)_{Pati-Salam}\times U_{I}(1)

γiγj,\displaystyle\gamma_{i}\gamma_{j}, ΓiΓj,γiΓk;I,\displaystyle\Gamma_{i}\Gamma_{j},\gamma_{i}\Gamma_{k};\quad I, (49)

where i,j,k=1,2,3,i>ji,j,k=1,2,3,i>j. Note that the real-valued gauge transformation parameters such as θLn\theta_{L}^{n} (ϵLn\epsilon_{L}^{n}) and θRn\theta_{R}^{n} (ϵRn\epsilon_{R}^{n}) are independent of each other. Therefore the left- and right-handed spinors ψL\psi_{L} and ψR\psi_{R} transform independently. Considering that the same copies of the symmetry group generators TnT_{n} and KnK_{n} are employed for the left- and right-handed spinors, the model is left-right symmetric.

Since the vierbein e^μ\hat{e}_{\mu} transforms as a vector under the Lorentz gauge transformation

e^μ\displaystyle\hat{e}_{\mu} e14θabγaγbe^μe14θabγaγb,\displaystyle\quad\rightarrow\quad e^{\frac{1}{4}\theta^{ab}\gamma_{a}\gamma_{b}}\;\hat{e}_{\mu}\;e^{-\frac{1}{4}\theta^{ab}\gamma_{a}\gamma_{b}}, (50)

a spinor bilinear term such as

ψ¯e^μψ,\displaystyle\left\langle\bar{\psi}\hat{e}_{\mu}\psi\right\rangle, (51)

can be verified to be gauge invariant under the above gauge transformations restricted to the Clifford-even sub-space (with the exception of the weak-boosts generated by {Γ0Γi\Gamma_{0}\Gamma_{i}} which will be revisited in Section 4). This invariance is of paramount importance, given that the fermion-related Lagrangian is of similar form and should respect these symmetries. Note that e^μ\hat{e}_{\mu} should always appear on the left side of spinor ψ\psi (or on the right side of ψ¯\bar{\psi}), since Lorentz gauge transformation is applied on the left side of ψ\psi.

The above gauge symmetry groups are the largest ones permissible by a chiral algebraic spinor of Cl(0,6)Cl(0,6). The spin group Spin(6)PatiSalamSpin(6)_{Pati-Salam} is generated by all the 15 bi-vectors of Cl(0,6)Cl(0,6). It is isomorphic to Pati-Salem’s SU(4)SU(4) [41], which encompasses SU(3)C×U(1)BLSU(3)_{C}\times U(1)_{B-L}. The Spin(1,3)WeakSpin(1,3)_{Weak} group comprises the regular weak SU(2)SU(2) group generated by {ΓiΓj\Gamma_{i}\Gamma_{j}} as well as the weak-boosts generated by {Γ0Γi\Gamma_{0}\Gamma_{i}}. These are the counterparts of the spacial rotations generated by {γiγj\gamma_{i}\gamma_{j}} and the Lorentz boosts generated by {γ0γi\gamma_{0}\gamma_{i}}. It can be readily verified that the two sets of generators {γaγb}\{\gamma_{a}\gamma_{b}\} and {ΓaΓb}\{\Gamma_{a}\Gamma_{b}\} (with a,b=0,1,2,3,a>ba,b=0,1,2,3,a>b) commute with each other. Therefore, the left-sided gauge symmetries are the direct product between these two symmetries Spin(1,3)×Spin(1,3)WeakSpin(1,3)\times Spin(1,3)_{Weak}, which is the subgroup of the encompassing spin group Spin(4,4)Spin(4,4) in (41).

The BSM symmetry bonanza noted above is tantalizing. From a practical point of view, do we have any inkling of symmetries beyond the local Lorentz and standard model gauge symmetries? The observation of neutrino oscillations[78, 79, 80] provided an interesting clue. It implies that neutrinos have nonzero masses beyond the plain vanilla standard model. Curiously, the neutrino masses are much smaller than that of the other standard model fermions. The seesaw mechanism is hence proposed as an explanation [42], which invokes the right-handed neutrinos endowed with large Majorana masses. In light of these suggestive evidences, we whittle down to a minimum subset of groups which could accommodate a Higgs-like mechanism to generate the Majorana masses.

Therefore, our choice of symmetry groups are [29]

Spin(1,3)×SU(3)C×SU(2)WL×U(1)WR×U(1)BL.\displaystyle Spin(1,3)\times SU(3)_{C}\times SU(2)_{WL}\times U(1)_{WR}\times U(1)_{B-L}. (52)

Note that in Section 4.4 on emergent chiral vierbeins, we will expand the above groups to accommodate the extended vierbeins and the extended weak interactions. But for now, we will stay with the above unextended symmetry groups.

The symmetry groups in Eq. (52) are the direct product of the spin connection’s Lorentz Spin(1,3)Spin(1,3) with six distinct generators (as in ψeθnTnψ\psi\rightarrow e^{\theta^{n}T_{n}}\psi)

12γaγb,\displaystyle\frac{1}{2}\gamma_{a}\gamma_{b}, (53)

where a,b=0,1,2,3,a>ba,b=0,1,2,3,a>b, and the left-handed weak interaction’s SU(2)WLSU(2)_{WL} with three generators (as in ψLeθLnTnψL\psi_{L}\rightarrow e^{\theta_{L}^{n}T_{n}}\psi_{L})

12Γ2Γ3,12Γ3Γ1,12Γ1Γ2,\displaystyle\frac{1}{2}\Gamma_{2}\Gamma_{3},\quad\frac{1}{2}\Gamma_{3}\Gamma_{1},\quad\frac{1}{2}\Gamma_{1}\Gamma_{2}, (54)

and the right-handed weak interaction’s U(1)WRU(1)_{WR} with one generator (as in ψReθRnTnψR\psi_{R}\rightarrow e^{\theta_{R}^{n}T_{n}}\psi_{R})

12Γ1Γ2,\displaystyle\frac{1}{2}\Gamma_{1}\Gamma_{2}, (55)

and the strong interaction’s SU(3)CSU(3)_{C} with eight generators (as in ψψeϵnKn\psi\rightarrow\psi e^{\epsilon^{n}K_{n}})

14(γ1Γ2+γ2Γ1),14(Γ1Γ2+γ1γ2),14(Γ1γ1Γ2γ2),14(γ1Γ3+γ3Γ1),14(Γ1Γ3+γ1γ3),14(γ2Γ3+γ3Γ2),14(Γ2Γ3+γ2γ3),143(Γ1γ1+Γ2γ22Γ3γ3),\begin{array}[]{rl}&\frac{1}{4}(\gamma_{1}\Gamma_{2}+\gamma_{2}\Gamma_{1}),\quad\frac{1}{4}(\Gamma_{1}\Gamma_{2}+\gamma_{1}\gamma_{2}),\quad\frac{1}{4}(\Gamma_{1}\gamma_{1}-\Gamma_{2}\gamma_{2}),\\ &\frac{1}{4}(\gamma_{1}\Gamma_{3}+\gamma_{3}\Gamma_{1}),\quad\frac{1}{4}(\Gamma_{1}\Gamma_{3}+\gamma_{1}\gamma_{3}),\\ &\frac{1}{4}(\gamma_{2}\Gamma_{3}+\gamma_{3}\Gamma_{2}),\quad\frac{1}{4}(\Gamma_{2}\Gamma_{3}+\gamma_{2}\gamma_{3}),\\ &\frac{1}{4\sqrt{3}}(\Gamma_{1}\gamma_{1}+\Gamma_{2}\gamma_{2}-2\Gamma_{3}\gamma_{3}),\end{array} (56)

and the BL interaction’s U(1)BLU(1)_{B-L} with one generator (as in ψψeϵnKn\psi\rightarrow\psi e^{\epsilon^{n}K_{n}})

12J=16(γ1Γ1+γ2Γ2+γ3Γ3).\displaystyle\frac{1}{2}J=\frac{1}{6}(\gamma_{1}\Gamma_{1}+\gamma_{2}\Gamma_{2}+\gamma_{3}\Gamma_{3}). (57)

Note that some multipliers are applied to the generators to facilitate the gauge field definitions in Section 2.4. Due to the chirality of the weak interaction, the gauge transformation parameters for the left- and right-handed spinors (θLn\theta_{L}^{n} and θRn\theta_{R}^{n}) are kept independent for SU(2)WLSU(2)_{WL} and U(1)WRU(1)_{WR}, whereas the other gauge transformation parameters of Spin(1,3)Spin(1,3), SU(3)CSU(3)_{C}, and U(1)BLU(1)_{B-L} are synchronized between the left- and right-handed spinors.

The left-sided and right-sided gauge transformations are applied to the left side and right side of the Clifford algebraic spinor, respectively. The Spin(1,3)×SU(2)WL×U(1)WRSpin(1,3)\times SU(2)_{WL}\times U(1)_{WR} symmetries in (52) belong to the left-sided gauge transformations, while the SU(3)C×U(1)BLSU(3)_{C}\times U(1)_{B-L} symmetries in (52) belong to the right-sided gauge transformations. By definition, the left-sided and right-sided gauge transformations commute with each other. Therefore, the total gauge symmetry in (52) is a direct product of Spin(1,3)×SU(2)WL×U(1)WRSpin(1,3)\times SU(2)_{WL}\times U(1)_{WR} and SU(3)C×U(1)BLSU(3)_{C}\times U(1)_{B-L}.

Let’s look at some instances: The right-sided color SU(3)CSU(3)_{C} gauge transformations (56) commute with the left-sided local Lorentz gauge transformations Spin(1,3)Spin(1,3) (53) and left-sided weak gauge transformations SU(2)WLSU(2)_{WL} (54) since they are applied to the different sides of the algebraic spinor, despite the fact that the generators in Eq. (56) and generators in Eq. (53)/(54) seemingly do not commute with each other. In the same vein, since the color projection operators (22) are applied to the right side of the algebraic spinor, they do not break the Lorentz symmetries which are applied to the left side of the algebraic spinor.

There are three Clifford elements which play a pivotal role in the symmetry determination. The first element γ0\gamma_{0} is hard-wired into the definition of Dirac inner product ψ¯ψ=ψγ0ψ\left\langle\bar{\psi}\psi\right\rangle=\left\langle{\psi}^{\dagger}\gamma_{0}\psi\right\rangle. It facilitates pinning down the Lorentz group Spin(1,3)Spin(1,3). The second element Γ1Γ2\Gamma_{1}\Gamma_{2} is embedded in the definition of isospin (29), thus it picks out the isospin direction (we would like to highlight the fact that Γ1Γ2\Gamma_{1}\Gamma_{2} commutes with the Lorentz generators γaγb\gamma_{a}\gamma_{b}, hence isospin projection does not break Lorentz symmetry). The third critical Clifford element is the BL interaction’s JJ (57). It is instrumental in separating out U(3)=SU(3)C×U(1)BLU(3)=SU(3)_{C}\times U(1)_{B-L} from the encompassing Spin(6)PatiSalamSpin(6)_{Pati-Salam} which is isomorphic to SU(4)SU(4). Mathematically speaking, this is a specific case of a general procedure [81, 5] of separating out U(n)U(n) from Spin(2n)Spin(2n).

When JJ is applied to the four color projection operators (22), it has the nice property that

PlJ=PlI,\displaystyle P_{l}J=-P_{l}I, (58a)
PrJ=13PrI,PgJ=13PgI,PbJ=13PbI,\displaystyle P_{r}J=\frac{1}{3}P_{r}I,\quad P_{g}J=\frac{1}{3}P_{g}I,\quad P_{b}J=\frac{1}{3}P_{b}I, (58b)

which means that JJ is tantamount to

J=(BL)I,\displaystyle J=(B-L)I, (59)

where BB and LL are baryon and lepton numbers, respectively. Therefore, JJ indeed corresponds to the BL interaction. The definition of the four color projection operators (22) as well as the definition of the color algebra (56) are both predicated on how JJ is structured. The ansatz ensures that applying any generator in the color algebra to the lepton projector PlP_{l} is identical to zero, hence leptons are invariant (singlets) under the color gauge transformations.

If we start from our choice of symmetries (52) as a given, the symmetry breaking mechanism from symmetries (52) all the way down to SU(3)C×U(1)EMSU(3)_{C}\times U(1)_{EM} can be readily worked out. The follow is a high-level preview of the major symmetry breaking patterns. The details of these symmetry breaking processes in the Clifford algebraic setting will be elaborated in Section 3.

The cascade of symmetry breaking processes begins with the vierbein acquiring a nonzero flat space-time VEV, which breaks the gauge symmetries down to

SU(3)C×SU(2)WL×U(1)WR×U(1)BL.\displaystyle SU(3)_{C}\times SU(2)_{WL}\times U(1)_{WR}\times U(1)_{B-L}. (60)

As a result, the local Lorentz gauge symmetry is lost. The next step of symmetry breaking is triggered by the Majorana-Higgs field, which is a Higgs-like field in addition to the standard model Higgs field. At this stage, the Majorana-Higgs field assumes a nonzero VEV and breaks the local gauge symmetries down to the standard model symmetries

SU(3)C×SU(2)WL×U(1)Y,\displaystyle SU(3)_{C}\times SU(2)_{WL}\times U(1)_{Y}, (61)

where U(1)YU(1)_{Y} is the hypercharge gauge symmetry specified by the synchronized double-sided gauge transformation

ψLψLe12ϵYJ,\displaystyle\psi_{L}\rightarrow\psi_{L}e^{\frac{1}{2}\epsilon_{Y}J}, (62)
ψRe12ϵYΓ1Γ2ψRe12ϵYJ,\displaystyle\psi_{R}\rightarrow e^{\frac{1}{2}\epsilon_{Y}\Gamma_{1}\Gamma_{2}}\psi_{R}e^{\frac{1}{2}\epsilon_{Y}J}, (63)

where a shared rotation angle ϵY\epsilon_{Y} synchronizes the double-sided hypercharge gauge transformation. At the third stage of symmetry breaking, the electroweak Higgs fields acquire nonzero VEVs and break the standard model symmetries down to

SU(3)C×U(1)EM,\displaystyle SU(3)_{C}\times U(1)_{EM}, (64)

where U(1)EMU(1)_{EM} is the electromagnetic gauge symmetry characterized by the synchronized double-sided gauge transformation

ψe12ϵEMΓ1Γ2ψe12ϵEMJ,\displaystyle\psi\rightarrow e^{\frac{1}{2}\epsilon_{EM}\Gamma_{1}\Gamma_{2}}\psi e^{\frac{1}{2}\epsilon_{EM}J}, (65)

where a shared rotation angle ϵEM\epsilon_{EM} synchronizes the double-sided electromagnetic gauge transformation. Based on the definition of the pseudoscalar-valued electromagnetic gauge field A^μ\hat{A}_{\mu} in Eq. (13), the electric charge qq of a given standard model fermion ψf\psi_{f} can thus be obtained via

e12ϵEMΓ1Γ2ψfe12ϵEMJ=ψfeqϵEMI.\displaystyle e^{\frac{1}{2}\epsilon_{EM}\Gamma_{1}\Gamma_{2}}\psi_{f}e^{\frac{1}{2}\epsilon_{EM}J}=\psi_{f}e^{q\epsilon_{EM}I}. (66)

Thanks to the properties of Γ1Γ2\Gamma_{1}\Gamma_{2} in Eq. (30) and JJ in Eq. (58), the electric charges can be readily calculated as q=0,1,23q=0,-1,\frac{2}{3}, and 13-\frac{1}{3} for neutrino, electron, up quarks, and down quarks according to the definitions in Eq. (27) and Eq. (28), which are perfectly aligned with the standard model electric charge assignments.

We shall underscore the fact that the algebraic spinors and all the gauge group generators are valued in the real Clifford space. Any reference of the imagine number ii in the conventional formalism with regard to gauge transformations (and gauge fields) and spinors can be replaced by the pseudoscalar II acting on the right side of the spinor, as illustrated in the definition of electric charge above.

2.3 Charge conjugation without particle-antiparticle interchange

The charge conjugation CC changes the sign of charges. In the conventional matrix formalism, the CC conjugation of a fermion ψ\psi in the Weyl basis is expressed as

C:ψψc=iγ2ψ,\displaystyle C:\quad\psi\rightarrow\psi_{c}=-i\gamma_{2}\psi^{\star}, (67)

where ψ\psi^{\star} is the complex conjugate of ψ\psi. Because of the complex conjugate operation, CC converts a particle into its corresponding antiparticle.

Can we decouple charge conjugation from complex conjugate and thus evade particle-antiparticle interchange? Such a decoupling is indeed possible in the Clifford algebra approach, thanks to the identification of the imaginary number ii with the pseudoscalar II acting on the right side of a spinor. Considering the definition of electric charge qq in Eq. (66), we can define a weaker form of charge conjugation

C:ψψc=(IΓ2Γ3)ψγ0.\displaystyle C^{\prime}:\quad\psi\rightarrow\psi_{c^{\prime}}=(I\Gamma_{2}\Gamma_{3})\psi\gamma_{0}. (68)

Note that IΓ2Γ3I\Gamma_{2}\Gamma_{3} and γ0\gamma_{0} in the above definition could be replaced with the general IΓ2Γ3eθΓ1Γ2I\Gamma_{2}\Gamma_{3}e^{\theta\Gamma_{1}\Gamma_{2}} and γ0eϵI\gamma_{0}e^{\epsilon I}, where θ\theta and ϵ\epsilon are two arbitrary phase factors. The weaker form of charge conjugation satisfies the property (ψc)c=ψ(\psi_{c^{\prime}})_{c^{\prime}}=\psi. It does not involve complex conjugate, hence there is no particle-antiparticle switching. In Section 3.2, this property of CC^{\prime} will be leveraged to construct a Majorana mass term that conserves lepton number.

According to Eq. (66), it can be easily checked that ψc\psi_{c^{\prime}} transforms as

ψcψceqϵEMI.\displaystyle\psi_{c^{\prime}}\rightarrow\psi_{c^{\prime}}e^{-q\epsilon_{EM}I}. (69)

under the electromagnetic gauge transformation. Therefore, the sign of electric charge is indeed changed. It’s driven by the fact that γ0\gamma_{0} in the definition of CC^{\prime} anticommutes with the unit pseudoscalar II

eqϵEMIγ0=γ0eqϵEMI.\displaystyle e^{q\epsilon_{EM}I}\gamma_{0}=\gamma_{0}e^{-q\epsilon_{EM}I}. (70)

This sort of mathematical maneuvering is otherwise impossible in the conventional formalism where the electromagnetic gauge transformation is associated with the imaginary number ii as in Eq. (2). Since ii commutes with any operator, the only way to change sign of ii is to invoke complex conjugate. Consequently, charge conjugation in the conventional formalism is inextricably linked to particle-antiparticle interchange.

It can be verified that CC^{\prime} does not change isospin (29) or color (22) of any standard model fermion. Since IΓ2Γ3I\Gamma_{2}\Gamma_{3} commutes with the Lorentz transformation generators γaγb\gamma_{a}\gamma_{b}, the Lorentz transformation properties of ψc\psi_{c^{\prime}} remain the same as ψ\psi. Note that CC^{\prime} changes the chirality of ψ\psi, since CC^{\prime} involves the multiplication of the Clifford-odd tri-vector γ0\gamma_{0} and it turns a left-handed fermion into a right-handed one, and vice versa.

The charge conjugation CC^{\prime} of the gauge transformation parameters (and thus gauge fields) can be defined as

C:θnTnθcnTn=θn(IΓ2Γ3)Tn(IΓ2Γ3),\displaystyle C^{\prime}:\quad\theta^{n}T_{n}\rightarrow\theta^{n}_{c^{\prime}}T_{n}=\theta^{n}(I\Gamma_{2}\Gamma_{3})T_{n}(I\Gamma_{2}\Gamma_{3}), (71)
C:ϵnKnϵcnKn=ϵnγ0Knγ0,\displaystyle C^{\prime}:\quad\epsilon^{n}K_{n}\rightarrow\epsilon^{n}_{c^{\prime}}K_{n}=\epsilon^{n}\gamma_{0}K_{n}\gamma_{0}, (72)

with the understanding that the left side-type TnT_{n} should include the generators of Spin(1,3)×SU(2)WL×U(1)WRSpin(1,3)\times SU(2)_{WL}\times U(1)_{WR} and the right side-type KnK_{n} should include the generators of SU(3)C×U(1)BLSU(3)_{C}\times U(1)_{B-L}. Some notable examples are that the electromagnetic gauge field A^μ\hat{A}_{\mu} is CC^{\prime}-odd, while the gravity-related spin connection Lorentz gauge field ω^μ\hat{\omega}_{\mu} is CC^{\prime}-even.

2.4 Clifford-valued gauge fields and Lagrangian of the world

Having established the fermion representation and the symmetry structure, we are now well-positioned to investigate the Clifford-valued gauge fields corresponding to these symmetries, as well as Lagrangians and actions on the 4-dimensional space-time manifold. As we noted in the introduction section, while the Clifford algebra has been extended to Cl(0,6)Cl(0,6), the underlying space-time manifold remains 4-dimensional. With a view toward writing down the diffeomorphism-invariant actions for general covariance, we are going to make extensive use of differential forms. We define gauge field as 1-forms and gauge forces as curvature 2-forms. Diffeomorphism invariance/general covariance can be ensured if the action for the curved space-time is expressed as an integration of 4-forms on the 4-dimensional space-time manifold.

The vierbein 1-form e^\hat{e} and spin connection 1-form ω^\hat{\omega} of the Lorentz gauge theory of gravity are

e^=e^μdxμ,\displaystyle\hat{e}=\hat{e}_{\mu}dx^{\mu}, (73)
ω^=ω^μdxμ,\displaystyle\hat{\omega}=\hat{\omega}_{\mu}dx^{\mu}, (74)

where μ=0,1,2,3\mu=0,1,2,3, and the Clifford-valued e^μ\hat{e}_{\mu} and ω^μ\hat{\omega}_{\mu} are given in Eq. (5). The Clifford-valued forms are also called Clifforms in the literature [37, 38].

In an similar fashion, the other gauge field 1-forms related to the gauge symmetries SU(3)C×SU(2)WL×U(1)WR×U(1)BLSU(3)_{C}\times SU(2)_{WL}\times U(1)_{WR}\times U(1)_{B-L} can be defined as

G^=G^μdxμ,\displaystyle\hat{G}=\hat{G}_{\mu}dx^{\mu}, (75)
W^L=W^Lμdxμ,\displaystyle\hat{W}_{L}=\hat{W}_{L\mu}dx^{\mu}, (76)
W^R=W^Rμdxμ,\displaystyle\hat{W}_{R}=\hat{W}_{R\mu}dx^{\mu}, (77)
A^BL=A^BLμdxμ,\displaystyle\hat{A}_{BL}=\hat{A}_{BL\mu}dx^{\mu}, (78)

where the strong interaction gauge field G^μ\hat{G}_{\mu}, the left-handed weak interaction gauge field W^Lμ\hat{W}_{L\mu}, the right-handed weak interaction gauge field W^Rμ\hat{W}_{R\mu}, and the BL interaction gauge field A^BLμ\hat{A}_{BL\mu} are valued in the gauge generator space of SU(3)CSU(3)_{C}, SU(2)WLSU(2)_{WL}, U(1)WRU(1)_{WR}, and U(1)BLU(1)_{B-L} (Eqs. (54), (55), (56) and (57)), respectively. As an example, according to the gauge group generators specified in Eqs. (54), the left-handed weak interaction gauge field W^Lμ\hat{W}_{L\mu} can be defined as

W^Lμ=12(WLμ1Γ2Γ3+WLμ2Γ3Γ1+WLμ3Γ1Γ2),\displaystyle\hat{W}_{L\mu}=\frac{1}{2}(W^{1}_{L\mu}\Gamma_{2}\Gamma_{3}+W^{2}_{L\mu}\Gamma_{3}\Gamma_{1}+W^{3}_{L\mu}\Gamma_{1}\Gamma_{2}), (79)

where WLμ1W^{1}_{L\mu}, WLμ2W^{2}_{L\mu}, and WLμ3W^{3}_{L\mu} are real-valued. The other gauge fields G^μ\hat{G}_{\mu}, W^R\hat{W}_{R}, and A^BLμ\hat{A}_{BL\mu} can be defined in a similar manner using the corresponding gauge group generators specified in Eqs.  (55), (56) and (57), respectively. We adopt the notation convention (e.g. G^\hat{G} rather than GG) to highlight the fact that these gauge fields are Clifford-valued 1-forms, i.e. Clifforms.

The chiral gauge-covariant derivatives of the chiral spinor fields are defined as

DLψL=(d+ω^+W^L)ψL+ψL(G^+A^BL),\displaystyle D_{L}\psi_{L}=(d+\hat{\omega}+\hat{W}_{L})\psi_{L}+\psi_{L}(\hat{G}+\hat{A}_{BL}), (80)
DRψR=(d+ω^+W^R)ψR+ψR(G^+A^BL),\displaystyle D_{R}\psi_{R}=(d+\hat{\omega}+\hat{W}_{R})\psi_{R}+\psi_{R}(\hat{G}+\hat{A}_{BL}), (81)

where dd is the exterior derivative d=dxμμd=dx^{\mu}\partial_{\mu}. We follow the convention of putting the gauge coupling constant in the coefficient of the Yang-Mills Lagrangian (see e.g. Eq. (109)), rather than in the gauge-covariant derivatives above (via re-scaling the gauge fields). The gauge-covariance property of the covariant derivatives is ensured by the gauge transformation rules of the gauge fields involved [27, 29]. It is essential that the gauge fields should appear on the proper side of the spinor, which is dictated by how the gauge symmetries are defined in Section 2.2. Specifically, ω^\hat{\omega} and W^L/R\hat{W}_{L/R} correspond to left-sided gauge symmetries, thus they should act on the left side of the spinor. On the other hand, G^\hat{G} and A^BL\hat{A}_{BL} correspond to right-sided gauge symmetries, hence they should be applied to the right side.

Note that there is no extra imaginary number ii in front of the gauge fields (such as iWLi{W}_{L} in the conventional QFT formalism) in the definition of the gauge-covariant derivatives. This conforms with the way the gauge transformations are defined in Subsection 2.2 where we choose the mathematicians’ convention without the extra ii in the definition of gauge transformations. It is also consistent with the general rule stated earlier that we should eschew the quantum imaginary number ii in the definition of classical fields and their corresponding gauge-covariant derivatives.

The spin connection ω^\hat{\omega}, as the gauge field of the Lorentz gauge group, is crucial in maintaining the local Lorentz gauge covariance of DLψLD_{L}\psi_{L} and DRψRD_{R}\psi_{R}. On the other hand, given that the vierbein e^\hat{e} is not a gauge field, e^\hat{e} is conspicuously absent in the gauge-covariant derivatives of the spinor fields ψL/R(x)\psi_{L/R}(x). Nonetheless, as we will learn below, e^\hat{e} shows up in other parts of the Lagrangian and it plays a pivotal role in the model building.

The gauge interactions are formulated as curvature 22-forms, namely R^\hat{R}, F^G\hat{F}_{G}, F^WL\hat{F}_{WL}, F^WR\hat{F}_{WR}, and F^BL\hat{F}_{BL}. For instance, the spin connection curvature 22-form R^\hat{R} and the left-handed weak interaction curvature 2-form F^WL\hat{F}_{WL} are expressed as

R^=dω^+ω^ω^,\displaystyle\hat{R}=d\hat{\omega}+\hat{\omega}\wedge\hat{\omega}, (82)
F^WL=dW^L+W^LW^L=12F^WLμνdxμdxν\displaystyle\hat{F}_{WL}=d\hat{W}_{L}+\hat{W}_{L}\wedge\hat{W}_{L}=\frac{1}{2}\hat{F}_{WL\mu\nu}dx^{\mu}\wedge dx^{\nu} (83)
=14(FWLμν1Γ2Γ3+FWLμν2Γ3Γ1+FWLμν3Γ1Γ2)dxμdxν,\displaystyle=\frac{1}{4}(F_{WL\mu\nu}^{1}\Gamma_{2}\Gamma_{3}+F_{WL\mu\nu}^{2}\Gamma_{3}\Gamma_{1}+F_{WL\mu\nu}^{3}\Gamma_{1}\Gamma_{2})dx^{\mu}\wedge dx^{\nu}, (84)

where \wedge stands for outer product between differential forms. For later usage we have expanded F^WL\hat{F}_{WL} in more details. The other curvature 22-forms F^WR\hat{F}_{WR}, F^G\hat{F}_{G}, and F^BL\hat{F}_{BL} can be defined in a similar way. Note that the outer product term vanishes for abelian interactions such as F^WR\hat{F}_{WR} and F^BL\hat{F}_{BL}.

Now we are ready to write down the local gauge- and diffeomorphism-invariant Lagrangian of the world

World=\displaystyle\mathcal{L}_{World}= Fermion\displaystyle\mathcal{L}_{Fermion} (85)
+\displaystyle+ Gravity+CC\displaystyle\mathcal{L}_{Gravity}+\mathcal{L}_{CC} (86)
+\displaystyle+ YMColor+YMWeakLeft+YMWeakRight+YMBL\displaystyle\mathcal{L}_{YM-Color}+\mathcal{L}_{YM-Weak-Left}+\mathcal{L}_{YM-Weak-Right}+\mathcal{L}_{YM-BL} (87)
+\displaystyle+ HiggsMajorana+HiggsElectroweak.\displaystyle\mathcal{L}_{Higgs-Majorana}+\mathcal{L}_{Higgs-Electroweak}. (88)

The fermion Lagrangian in curved space-time is of the form

FermioniIe^e^e^(ψLDLψL¯)+iIe^e^e^(ψRDRψR¯),\displaystyle\mathcal{L}_{Fermion}\sim i\left\langle I\hat{e}\wedge\hat{e}\wedge\hat{e}\wedge(\psi_{L}\overline{D_{L}\psi_{L}})\right\rangle+i\left\langle I\hat{e}\wedge\hat{e}\wedge\hat{e}\wedge(\psi_{R}\overline{D_{R}\psi_{R}})\right\rangle, (89)

where DL/RψL/R¯\overline{D_{L/R}\psi_{L/R}} is the Dirac conjugate of DL/RψL/RD_{L/R}\psi_{L/R} defined as DL/RψL/R¯=(DL/RψL/R)γ0\overline{D_{L/R}\psi_{L/R}}=(D_{L/R}\psi_{L/R})^{\dagger}\gamma_{0}. The gravity plus cosmological constant Lagrangian terms are of the form

Gravity+CC\displaystyle\mathcal{L}_{Gravity}+\mathcal{L}_{CC} =18πGI(e^e^R^Λ4!e^e^e^e^),\displaystyle=\frac{1}{8\pi G}\left\langle I(\hat{e}\wedge\hat{e}\wedge\hat{R}-\frac{\Lambda}{4!}\hat{e}\wedge\hat{e}\wedge\hat{e}\wedge\hat{e})\right\rangle, (90)

where R^\hat{R} is the spin connection curvature 22-form (82), GG is gravitational constant, and Λ\Lambda is the cosmological constant. The left-handed weak interaction Yang-Mills Lagrangian term in curved space-time is of the form

YMWeakLeft(Ie^e^F^WL)(Ie^e^F^WL)Ie^e^e^e^.\displaystyle\mathcal{L}_{YM-Weak-Left}\sim\frac{\left\langle(I\hat{e}\wedge\hat{e}\wedge\hat{F}_{WL})(I\hat{e}\wedge\hat{e}\wedge\hat{F}_{WL})\right\rangle}{\left\langle I\hat{e}\wedge\hat{e}\wedge\hat{e}\wedge\hat{e}\right\rangle}. (91)

The Yang-Mills-type Lagrangian terms for the other gauge interactions such as F^G\hat{F}_{G}, F^WR\hat{F}_{WR}, and F^BL\hat{F}_{BL} take a similar form, which for brevity sake we will not write out explicitly. Here we adopted the generic “Yang-Mills-type” label, albeit historically the term Yang-Mills is reserved for non-abelian gauge fields only. Note that \left\langle\ldots\right\rangle denotes the Clifford-scalar part of the enclosed expression, as defined earlier.

The Higgs field-related Lagrangian terms HiggsMajorana\mathcal{L}_{Higgs-Majorana} and HiggsElectroweak\mathcal{L}_{Higgs-Electroweak} will be outlined in Sections 3.2 and 3.3 when we discuss the Higgs mechanism. Upon symmetry breaking, the Majorana and Dirac mass terms will emerge from HiggsMajorana\mathcal{L}_{Higgs-Majorana} and HiggsElectroweak\mathcal{L}_{Higgs-Electroweak} via the Higgs mechanism. For later reference, we write down the Dirac mass term for a given standard model fermion ψf\psi_{f} in curved space-time as

DiracMassimfIe^e^e^e^(ψfIψ¯f),\displaystyle\mathcal{L}_{Dirac-Mass}\sim im_{f}\left\langle I\hat{e}\wedge\hat{e}\wedge\hat{e}\wedge\hat{e}(\psi_{f}I\bar{\psi}_{f})\right\rangle, (92)

where mfm_{f} is the Dirac mass of fermion ψf\psi_{f}.

It shall be reminded that in the Yang-Mills Lagrangian term, the 4-form factor d4x=dx0dx1dx2dx3d^{4}x=dx^{0}\wedge dx^{1}\wedge dx^{2}\wedge dx^{3} from one of the Ie^e^F^WLI\hat{e}\wedge\hat{e}\wedge\hat{F}_{WL} should be canceled out by the similar 4-form factor from the denominator Ie^e^e^e^I\hat{e}\wedge\hat{e}\wedge\hat{e}\wedge\hat{e} before multiplication with the other Ie^e^F^WLI\hat{e}\wedge\hat{e}\wedge\hat{F}_{WL}. As such, the Yang-Mills Lagrangian terms, along with the other Lagrangian terms of the world, are diffeomorphism-invariant 4-forms on the 4-dimensional space-time manifold.

Also note that the Clifford algebra elements of the vierbein e^\hat{e} and the curvature 22-forms such as F^G\hat{F}_{G} formally commute with each other in the Yang-Mills Lagrangian, since they transform under commuting gauge groups. Since the vierbein e^\hat{e} transforms as a vector under Lorentz gauge transformation (50) and is invariant under the other gauge transformations, all the terms of the Lagrangian of the world can be proved to be invariant under the local gauge symmetry transformations (52).

If we look at the fermion Lagrangian term Fermion\mathcal{L}_{Fermion} in isolation, it can potentially accommodate Pati-Salam’s left-right symmetrical SU(2)L×SU(2)R×SU(4)SU(2)_{L}\times SU(2)_{R}\times SU(4), since no quark/lepton projections or P±P_{\pm} projections (which would otherwise spoil the Pati-Salam symmetries) are applied to the fermions ψL\psi_{L} and ψR\psi_{R} in Fermion\mathcal{L}_{Fermion}. However, as we will learn later in section 3, the Higgs Lagrangian terms HiggsMajorana\mathcal{L}_{Higgs-Majorana} and HiggsElectroweak\mathcal{L}_{Higgs-Electroweak} do involve the Pati-Salam-violating quark/lepton projections (on the Majorana-Higgs field and fermion fields) and P±P_{\pm} projections (on the standard model Higgs field and right-handed fermion fields). Therefore, the Lagrangian of the world as a whole does not enjoy the Pati-Salam symmetries.

The action of the world is

Sworld=World,\displaystyle S_{world}=\int\mathcal{L}_{World}, (93)

where the integration over d4x=dx0dx1dx2dx3d^{4}x=dx^{0}\wedge dx^{1}\wedge dx^{2}\wedge dx^{3} is already embedded in the definition of the Lagrangian as 4-form. We know that the space-time metric gμνg_{\mu\nu} can be derived from the vierbein (see Eq. (6)). Thus the metric tensor gμνg_{\mu\nu}-related quantities in the conventional metric gravity can be constructed using various combinations/transformations of the vierbein. For instance, the 4-form 14!Ie^e^e^e^\frac{1}{4!}I\hat{e}\wedge\hat{e}\wedge\hat{e}\wedge\hat{e} plays the role of the metric volume form |g|d4x\sqrt{|g|}d^{4}x. Another example is that the conventional Hodge star \star is replaced by the specific configuration of vierbeins in the Yang-Mills Lagrangian (91).

We subscribe to the general notion of effective field theory [82, 83], which states that all the terms allowed by the symmetry requirements should be included in the Lagrangian of the world. Since one goal of this paper is to treat gravity and Yang-Mills interactions on an equal footing, we should consider Lagrangian terms that is linear in Yang-Mills curvature 2-forms as well, such as

Ie^e^F^WL.\displaystyle\left\langle I\hat{e}\wedge\hat{e}\wedge\hat{F}_{WL}\right\rangle. (94)

The above term is analogs to the gravity Lagrangian (90) which is linear in the spin connection curvature 22-form R^\hat{R}. However, it can be verified that such linear Lagrangian terms for the Yang-Mills curvature 2-forms are identically zero. The only allowable linear term other than the gravity Lagrangian is the Holst term [84]

e^e^R^,\displaystyle\left\langle\hat{e}\wedge\hat{e}\wedge\hat{R}\right\rangle, (95)

which differs from the gravity Lagrangian (90) by removing the pseudoscalar II.

When it comes to the Lagrangian terms with two or more gauge curvature 2-forms, there is a plethora of allowable forms besides the Yang-Mills-type Lagrangian. Some examples are the topological CP-violating terms for the Yang-Mills interactions, the topological Gauss-Bonnet term and Nieh-Yan term [85], and the higher-derivative gravity terms [83]. While all these higher-order terms should in principle be included in the Lagrangian, the key for model building is to recognize that the practical predictions of any model must be made within the context of separation of energy scales. The gravity and Yang-Mills Lagrangian terms happen to be amongst the first few order terms that are relevant at the energy scale accessible to experiments.

The attentive readers may have noticed the presence of the imaginary number ii in the fermion kinetic Lagrangian (89) and Dirac mass Lagrangian (92). As explained in the introduction section, there are two kinds of imaginary numbers. One is the genuine ii, and the other can be replaced by the pseudoscalar II. We have demonstrated that the algebraic spinors and the gauge group generators are valued in the real Clifford space. Hence we have managed to stay away from the imaginary number ii. So why do we need ii in the fermion Lagrangian terms? It has to do with the requirement that the classical action of the world should be real

Sworld=Sworld.\displaystyle S^{*}_{world}=S_{world}. (96)

We know that \left\langle\ldots\right\rangle is employed in each Lagrangian term. By definition, it is the Clifford-scalar part of the expression, which means \left\langle\ldots\right\rangle is real as long as the related fields in the expression are valued in the real Clifford space. Since the bosonic fields (gauge fields, vierbein, and Higgs fields) are valued in the real Clifford space, the reality condition is automatically satisfied for all the bosonic field-related Lagrangian terms, such as the gravity and Yang-mills Lagrangian terms.

On the other hand, since spinors are valued in the real Clifford space with Grassmann-odd coefficients, the fermion action can essentially be reduced to a sum/integral of terms like iψnψmi\psi_{n}\psi_{m}, where ψn\psi_{n} and ψm\psi_{m} are Grassmann-odd coefficients of the spinors. Given that ψn\psi_{n} and ψm\psi_{m} are defined as real ψn=ψn\psi^{*}_{n}=\psi_{n} and ψm=ψm\psi^{*}_{m}=\psi_{m}, the complex conjugate of iψnψmi\psi_{n}\psi_{m} can be calculated as

(iψnψm)=iψmψn=iψmψn=iψnψm.\displaystyle(i\psi_{n}\psi_{m})^{*}=i^{*}\psi^{*}_{m}\psi^{*}_{n}=-i\psi_{m}\psi_{n}=i\psi_{n}\psi_{m}. (97)

Hence the reality condition is satisfied, which is otherwise violated if ii in the expression is removed. Note that the complex conjugate of the multiplication of Grassmann numbers is defined as

(ψnψm)=ψmψn,\displaystyle(\psi_{n}\psi_{m})^{*}=\psi^{*}_{m}\psi^{*}_{n}, (98)

with no extra minus sign, even though both ψn\psi_{n} and ψm\psi_{m} are Grassmann-odd.

In summary, we are compelled to include the imaginary number ii in the definition of the fermion Lagrangian to enforce the reality condition. That said, as mentioned earlier, the imaginary number ii is intimately related to the quantum theory. It will be shown in Section 4 that the appearance of ii in the fermion Lagrangian is the tip of the iceberg of quantum essence of almost everything.

3 Spontaneous Symmetry Breaking

In this section, we investigate spontaneous symmetry breaking (SSB) driven by the non-degenerate vacuum expectation values (VEVs) of various bosonic fields, such as vierbein e^\hat{e}, Majorana-Higgs field ϕM\phi_{M}, the standard model Higgs field ϕ\phi, antisymmetric-tensor Higgs field ϕAT\phi_{AT}, and Φ\Phi fields. Among these bosonic fields, the vierbein e^\hat{e} field and the antisymmetric-tensor Higgs field ϕAT\phi_{AT} are Lorentz vector and Lorentz sextet respectively, while the rest are Lorentz scalars. Along the way, we also study the fermion mass hierarchies and the lepton number-conserving Majorana mass.

Consistent with Section 2, we regard these bosonic fields as classical fields prior to field quantization. Therefore, the quantum imaginary number ii should not be allowed in the definition of these classical fields such as the classical vierbein and Higgs fields. In the current section, all these symmetry-breaking bosonic fields are expressed as real Clifford algebra Cl(0,6)Cl(0,6) multivectors. The important topic of field quantization via the Clifford functional integral formalism and the formal introduction of imaginary number ii will be discussed in detail in Section 4.

There are two common threads running through these bosonic fields. The first common thread is that all these bosonic fields develop non-zero VEVs and consequently lead to SSB. Note that while the Majorana-Higgs field ϕM\phi_{M}, the standard model Higgs field ϕ\phi, and the antisymmetric-tensor Higgs field ϕAT\phi_{AT} break gauge symmetries only, the vierbein e^\hat{e} field breaks both Lorentz gauge symmetry and diffeomorphism symmetry given that vierbein e^\hat{e} is a differential 1-form unlike the 0-form Higgs fields. The Φ\Phi fields are unique in that they are gauge invariant and hence they break global symmetries and generate (pseudo) Nambu-Goldstone bosons.

The second common thread is that all these symmetry-breaking fields are composite fields of quantum condensation origin, albeit in the current section we treat these symmetry-breaking fields as fundamental fields only. The compositeness of these bosonic fields will be investigated in Section 4. Note that all the standard model fermion fields and all the gauge fields examined in Section 2 are still fundamental non-composite fields.

3.1 Vierbein-induced SSB and the residual global Lorentz symmetry

The SSB saga of the universe starts with the vierbein field e^\hat{e} acquiring a nonzero VEV. As a consequence, the local Lorentz gauge symmetry Spin(1,3)Spin(1,3) and the diffeomorphism symmetry are violated. The remaining local gauge symmetries are SU(3)C×SU(2)WL×U(1)WR×U(1)BLSU(3)_{C}\times SU(2)_{WL}\times U(1)_{WR}\times U(1)_{B-L} plus a residual global Lorentz symmetry.

The “ground state” of the vierbein e^\hat{e} and spin connection ω^\hat{\omega} should satisfy the field equations, which are obtained by varying the world action SworldS_{world} with the fields e^\hat{e} and ω^\hat{\omega} independently. The resultant Einstein-Cartan equations read

18πG(R^e^+e^R^Λ3!e^e^e^)I=𝕋,\displaystyle\frac{1}{8\pi G}(\hat{R}\wedge\hat{e}+\hat{e}\wedge\hat{R}-\frac{\Lambda}{3!}\hat{e}\wedge\hat{e}\wedge\hat{e})I=\mathbb{T}, (99)
18πG(T^e^e^T^)I=𝕊,\displaystyle\frac{1}{8\pi G}(\hat{T}\wedge\hat{e}-\hat{e}\wedge\hat{T})I=\mathbb{S}, (100)

where the energy-momentum current 33-form 𝕋\mathbb{T} and the spin current 33-form 𝕊\mathbb{S} arise from the matter sector, such as the fermion, Yang-Mills, and Higgs action terms. Note that R^\hat{R} is the spin connection curvature 22-form (82), and T^\hat{T} is the torsion 22-form

T^\displaystyle\hat{T} =de^+ω^e^+e^ω^.\displaystyle=d\hat{e}+\hat{\omega}\wedge\hat{e}+\hat{e}\wedge\hat{\omega}. (101)

When the spin-current 𝕊\mathbb{S} is zero, the second Einstein-Cartan equation (100) amounts to enforcing the zero-torsion condition

T^\displaystyle\hat{T} =0,\displaystyle=0, (102)

which can be used to express the spin connection ω^\hat{\omega} in terms of the vierbein e^\hat{e}. In this case, the remaining (first) Einstein-Cartan equation (99) can be shown to be equivalent to the regular Einstein field equations of gravity plus a cosmological constant term.

Upon SSB, the vierbein field develops a nonzero VEV

e^=δμaγadxμ=γμdxμ,\displaystyle\hat{e}=\delta_{\mu}^{a}\gamma_{a}dx^{\mu}=\gamma_{\mu}dx^{\mu}, (103)

while the spin connection remains zero

ω^=0.\displaystyle\hat{\omega}=0. (104)

It can be verified that the above e^\hat{e} and ω^\hat{\omega} satisfy the Einstein-Cartan equations, provided that Λ=0\Lambda=0, 𝕋=0\mathbb{T}=0, and 𝕊=0\mathbb{S}=0. Subsequently, the space-time metric gμν=e^μe^νg_{\mu\nu}=\left\langle\hat{e}_{\mu}\hat{e}_{\nu}\right\rangle reduces to

gμν=γμγν=ημν,g_{\mu\nu}=\left\langle\gamma_{\mu}\gamma_{\nu}\right\rangle=\eta_{\mu\nu}, (105)

which is the Minkowski flat space-time metric.

With the substitution of e^\hat{e} and ω^\hat{\omega} by the VEVs, the fermion action in the flat Minkowski space-time reduces to

Sfermion=iψ¯LγμDLμψL+ψ¯RγμDRμψRd4x,\displaystyle S_{fermion}=\int i{\left\langle\bar{\psi}_{L}\gamma^{\mu}D_{L\mu}\psi_{L}+\bar{\psi}_{R}\gamma^{\mu}D_{R\mu}\psi_{R}\right\rangle d^{4}x}, (106)

where

DLμψL=(μ+W^Lμ)ψL+ψL(G^μ+A^BLμ),\displaystyle D_{L\mu}\psi_{L}=(\partial_{\mu}+\hat{W}_{L\mu})\psi_{L}+\psi_{L}(\hat{G}_{\mu}+\hat{A}_{BL\mu}), (107)
DRμψR=(μ+W^Rμ)ψR+ψR(G^μ+A^BLμ).\displaystyle D_{R\mu}\psi_{R}=(\partial_{\mu}+\hat{W}_{R\mu})\psi_{R}+\psi_{R}(\hat{G}_{\mu}+\hat{A}_{BL\mu}). (108)

Similarly, the Yang-Mills action(91) of the left-handed weak interaction F^WL\hat{F}_{WL} can be rewritten as

SYMWeakLeft=14gWLFWLμνiFWLi,μνd4x,\displaystyle S_{YM-Weak-Left}=-\frac{1}{4g_{WL}}\int{F_{WL\mu\nu}^{i}F_{WL}^{i,\mu\nu}d^{4}x}, (109)

where gWLg_{WL} is the dimensionless coupling constant of the left-handed weak interaction. The Yang-Mills-type action terms of the right-handed weak, strong, and BL interactions take a similar form, with coupling constants gWRg_{WR}, gGg_{G}, and gBLg_{BL}, respectively. Note that

γμημν=γν,\displaystyle\gamma^{\mu}\eta_{\mu\nu}=\gamma_{\nu}, (110)
FWLi,μνημαηνβ=FWLαβi,\displaystyle F_{WL}^{i,\mu\nu}\eta_{\mu\alpha}\eta_{\nu\beta}=F_{WL\alpha\beta}^{i}, (111)

where {γμ}\{\gamma^{\mu}\} is the reciprocal frame of {γa}\{\gamma_{a}\}. The reciprocal frame {γμ}\{\gamma^{\mu}\} is the avatar of the vierbein 3-form Ie^e^e^I\hat{e}\wedge\hat{e}\wedge\hat{e} from the original fermion Lagrangian (89) when the vierbein field e^\hat{e} acquires the nonzero VEV in Eq. (103). Therefore, when the fermion action in the flat Minkowski space-time (106) is employed to derive the massless Dirac equation (the Dirac equation with nonzero mass will be discussed in Section 3.3)

γμDL,μψL=0,\displaystyle\gamma^{\mu}D_{L,\mu}\psi_{L}=0, (112)
γμDR,μψR=0,\displaystyle\gamma^{\mu}D_{R,\mu}\psi_{R}=0, (113)

what shows up in the Dirac equation is the reciprocal frame. As such, it’s the reciprocal frame {γμ}\{\gamma^{\mu}\} that corresponds to the gamma matrices used in the conventional formalism. This fact also explains the minus sign we mentioned earlier: I-I plays the role of the conventional pseudoscalar when it is applied to the left side of a spinor such as Iψ-I\psi. The conventional pseudoscalar is defined using the reciprocal frame {γμ}\{\gamma^{\mu}\}, whereas we define the pseudoscalar using the original Clifford algebra basis {γa}\{\gamma_{a}\}. Hence there is a minus sign.

It’s worth mentioning that when we derive the flat space-time fermion action from the curved space-time counterpart, we have leveraged (γμ)=γ0γμγ0(\gamma^{\mu})^{\dagger}=\gamma_{0}\gamma^{\mu}\gamma_{0} and the following properties

FG=GF,\displaystyle\left\langle FG\right\rangle=-\left\langle GF\right\rangle, (114a)
(FG)=FG,\displaystyle\left\langle(FG)^{\dagger}\right\rangle=-\left\langle FG\right\rangle, (114b)

where the Grassmann-odd FF and GG are functionals of odd multiples of ψ(x)\psi(x) and ψ¯(x)\bar{\psi}(x). The minus sign arises from the Grassmann-odd nature of ψ(x)\psi(x) and ψ¯(x)\bar{\psi}(x).

Upon SSB induced by the nonzero VEV of the vierbein e^\hat{e}, both the local Lorentz gauge symmetry Spin(1,3)Spin(1,3) and the diffeomorphism symmetry are violated. That said, it can be verified that the fermion (106) and the Yang-Mills (109) actions in flat Minkowski space-time is invariant under the residual global Lorentz transformations

xμ\displaystyle x^{\mu} (Λ1)νμxν,\displaystyle\quad\rightarrow\quad(\Lambda^{-1})^{\mu}_{\nu}x^{\nu}, (115)
WLμi(x)\displaystyle W^{i}_{L\mu}(x) (Λ1)μνWLνi(Λ1x),\displaystyle\quad\rightarrow\quad(\Lambda^{-1})_{\mu}^{\nu}W^{i}_{L\nu}(\Lambda^{-1}x), (116)
ψ(x)\displaystyle\psi(x) e14θabγaγbψ(Λ1x),\displaystyle\quad\rightarrow\quad e^{\frac{1}{4}\theta^{ab}\gamma_{a}\gamma_{b}}\psi(\Lambda^{-1}x), (117)

where the Lorentz transformation parameters θab=θba\theta^{ab}=-\theta^{ba} and Λνμ\Lambda^{\mu}_{\nu} are related via the equation

e14θabγaγbγμe14θabγaγb=Λνμγν.\displaystyle e^{\frac{1}{4}\theta^{ab}\gamma_{a}\gamma_{b}}\gamma^{\mu}e^{-\frac{1}{4}\theta^{ab}\gamma_{a}\gamma_{b}}=\Lambda^{\mu}_{\nu}\gamma^{\nu}. (118)

Note that the global Lorentz transformation parameters θab\theta^{ab} above are independent of position, as opposed to the position-dependent θab(x)\theta^{ab}(x) for the local Lorentz gauge transformations.

The situation here parallels the Higgs mechanism where there remains a global SU(2)SU(2) custodial symmetry [86] after the electroweak symmetry breaking. In the literature [87, 88, 89], comparisons have been made between the vierbein-induced gravitational symmetry breaking and the Higgs-induced electroweak symmetry breaking.

In the case of the vierbein-induced SSB, the vestigial global Lorentz symmetry is a synchronization (enforced by Eq. (118)) between the global portion of the local Lorentz gauge transformation (e14θabγaγbe^{\frac{1}{4}\theta^{ab}\gamma_{a}\gamma_{b}}) for spinors and the global volume-preserving portion of the diffeomorphism transformation (Λμν\Lambda_{\mu}^{\nu}) for space-time coordinates. The local Lorentz gauge transformation involves Clifford algebraic elements such as γaγb\gamma_{a}\gamma_{b} labeled by Roman indices, while the diffeomorphism transformation involves coordinates xμx^{\mu} and gauge fields (e.g. the electromagnetic field AμA_{\mu} in Eq. (13)) labeled by Greek indices. At the nexus is the VEV of the vierbein eμa=δμae_{\mu}^{a}=\delta_{\mu}^{a} which acts as a soldering form gluing together the Roman and Greek propers.

3.2 Majorana mass and absence of neutrinoless double beta decay

The second stage of SSB is triggered by the Majorana-Higgs field ϕM\phi_{M} that couples to the right-handed neutrinos only. It is a Higgs-like bosonic field in addition to the well-known electroweak symmetry-breaking Higgs field ϕ\phi of the standard model. The VEV of ϕM\phi_{M} generates Majorana mass for the right-handed neutrino. This is why we call it the Majorana-Higgs field. It breaks the gauge symmetries from SU(3)C×SU(2)WL×U(1)WR×U(1)BLSU(3)_{C}\times SU(2)_{WL}\times U(1)_{WR}\times U(1)_{B-L} down to the standard model symmetries. This subsection also presents one major thesis of our paper: The neutrino Majorana mass preserves lepton number and therefore it does not lead to the neutrinoless double beta decay.

The Majorana-Higgs field ϕM\phi_{M} is valued in the real Clifford algebraic subspace spanned by two multivectors

ϕM=(ϕM1+ϕM2I)γ0Pl,\displaystyle\phi_{M}=(\phi_{M1}+\phi_{M2}I)\gamma_{0}P_{l}, (119)

where ϕM1\phi_{M1} and ϕM2\phi_{M2} are two real numbers, and PlP_{l} is the lepton projection operator (22). The Majorana-Higgs field obeys gauge transformation rules

ϕMe12θWRI12ϵBLJϕMe12θWRI+12ϵBLJ,\displaystyle\phi_{M}\quad\rightarrow\quad e^{-\frac{1}{2}\theta_{WR}I-\frac{1}{2}\epsilon_{BL}J}\;\phi_{M}\;e^{\frac{1}{2}\theta_{WR}I+\frac{1}{2}\epsilon_{BL}J}, (120)

where θWR\theta_{WR} and ϵBL\epsilon_{BL} are the right-handed weak U(1)WRU(1)_{WR} and BL U(1)BLU(1)_{B-L} gauge transformation parameters. As such, ϕM\phi_{M} is invariant under the Lorentz Spin(1,3)Spin(1,3) (Lorentz scalar), left-handed weak SU(2)WLSU(2)_{WL} (weak singlet), and color SU(3)CSU(3)_{C} (color singlet) gauge transformations. Given that JPl=IPlJP_{l}=-IP_{l}, one can replace JJ with I-I in the above transformation. We keep JJ to highlight its relevance to the BL symmetry. Note that ϕM\phi_{M} is Clifford-odd, different from the Clifford-even electroweak Higgs field which will be investigated in Section 3.3.

The Majorana-Higgs Lagrangian reads

HiggsMajorana=(DμϕM)(DμϕM)VM+(yMiI)ν¯R(IΓ2Γ3)νRϕM,\displaystyle\mathcal{L}_{Higgs-Majorana}=\left\langle(D^{\mu}\phi_{M})^{\dagger}(D_{\mu}\phi_{M})-V_{M}+(y_{M}iI)\bar{\nu}_{R}(I\Gamma_{2}\Gamma_{3}){\nu}_{R}\phi_{M}\right\rangle, (121)

where νR{\nu}_{R} is the right-handed neutrino, yMy_{M} is the Majorana-Yukawa coupling constant, and the Majorana-Higgs potential VMV_{M} is

VM=μM2ϕMϕM+λM(ϕMϕM)2.\displaystyle V_{M}=-\mu_{M}^{2}\phi_{M}^{\dagger}\phi_{M}+\lambda_{M}(\phi_{M}^{\dagger}\phi_{M})^{2}. (122)

The gauge-covariant derivative of ϕM\phi_{M} is defined as

DμϕM=(μ12WRμI12ABLμJ)ϕM+ϕM(12WRμI+12ABLμJ),\displaystyle D_{\mu}\phi_{M}=(\partial_{\mu}-\frac{1}{2}W_{R\mu}I-\frac{1}{2}A_{BL\mu}J)\phi_{M}+\phi_{M}(\frac{1}{2}W_{R\mu}I+\frac{1}{2}A_{BL\mu}J), (123)

which involves the right-handed weak gauge field W^Rμ\hat{W}_{R\mu} and the BL gauge field A^BLμ\hat{A}_{BL\mu}. Note that the bi-vector Γ2Γ3\Gamma_{2}\Gamma_{3} in the Yukawa term can be replaced by an arbitrary combination of Γ2Γ3\Gamma_{2}\Gamma_{3} and Γ1Γ3\Gamma_{1}\Gamma_{3}. But it does not change the overall picture. The imaginary number ii shows up in the Yukawa term. This is in compliance with the reality condition for the Majorana-Higgs Lagrangian. It’s worth mentioning that for flat space-time we follow the convention of not including d4xd^{4}x in the definition of the Lagrangian, as opposed to the curved space-time case where d4xd^{4}x is embedded in the definition of the Lagrangian as 4-form.

Given that ϕM\phi_{M} is a weak singlet, the Majorana-Yukawa term couples with the right-handed neutrinos only, as opposed to the electroweak Higgs Yukawa term which couples with both the left- and right-handed fermions. The Majorana-Higgs Lagrangian HiggsMajorana\mathcal{L}_{Higgs-Majorana} can be verified to be SU(3)C×SU(2)WL×U(1)WR×U(1)BLSU(3)_{C}\times SU(2)_{WL}\times U(1)_{WR}\times U(1)_{B-L} gauge invariant. Due to the gauge transformation properties of ϕM\phi_{M} (120), it can be shown that a similar Majorana-Yukawa term coupling to the right-handed electrons is prohibited since such a term violates the gauge symmetries. Therefore, the Majorana-Yukawa term couples to the right-handed neutrinos exclusively.

By virtue of the Mexican hat-shaped potential VMV_{M}, the Majorana-Higgs field ϕM\phi_{M} acquires a nonzero VEV

ϕM=12υMγ0Pl,\displaystyle\phi_{M}=\frac{1}{\sqrt{2}}\upsilon_{M}\gamma_{0}P_{l}, (124)

where υM=μMλM\upsilon_{M}=\frac{\mu_{M}}{\sqrt{\lambda_{M}}} is called the Majorana scale (or the seesaw scale).

As a result, the gauge symmetry related to the gauge field Z^μ\hat{Z}^{\prime}_{\mu}

Z^μ=WRμI+ABLμJ,\displaystyle\hat{Z}^{\prime}_{\mu}=W_{R\mu}I+A_{BL\mu}J, (125)

is spontaneously broken. The would-be Nambu-Goldstone boson is "eaten” by the gauge field Z^μ\hat{Z}^{\prime}_{\mu} which gains a mass as a consequence. The local gauge symmetries are broken down to the standard model symmetries SU(3)C×SU(2)WL×U(1)YSU(3)_{C}\times SU(2)_{WL}\times U(1)_{Y}, with the hypercharge gauge symmetry U(1)YU(1)_{Y} specified by the synchronized double-sided gauge transformation (62). The U(1)YU(1)_{Y} gauge field A^Y\hat{A}_{Y} remains massless and has an effective coupling constant of [29]

gY=gWRgBLgWR2+gBL2,\displaystyle g_{Y}=\frac{g_{WR}g_{BL}}{\sqrt{g_{WR}^{2}+g_{BL}^{2}}}, (126)

where gWRg_{WR} and gBLg_{BL} are the right-handed weak and BL coupling constants, respectively.

After replacement of ϕM\phi_{M} with its VEV, the Majorana-Yukawa term reduces to the Majorana mass term of the right-handed neutrino

MiIν¯R(IΓ2Γ3)νRγ0=MiIν¯R(νR)C,\displaystyle Mi\left\langle I\bar{\nu}_{R}(I\Gamma_{2}\Gamma_{3})\nu_{R}\gamma_{0}\right\rangle=Mi\left\langle I\bar{\nu}_{R}(\nu_{R})_{C^{\prime}}\right\rangle, (127)

where (νR)C(\nu_{R})_{C^{\prime}} is the weaker form charge conjugation CC^{\prime} (68) of νR\nu_{R} and the Majorana mass MM is

M=12yMυM.\displaystyle M=\frac{1}{\sqrt{2}}y_{M}\upsilon_{M}. (128)

It can be verified that the Majorana mass term respects all the standard model symmetries. This kind of mass is allowed for a standard model singlet such as νR\nu_{R}. It can also be shown that the Majorana mass term is permitted only if νR\nu_{R} is valued in the Clifford algebraic space with real Grassmann coefficients. The Majorana mass term would be identically zero if νR\nu_{R} were valued in the Clifford algebraic space with real coefficients.

If we juxtapose the Majorana mass term with a typical Dirac mass term between neutrinos

mνiIν¯ν=mνiIν¯LνR+Iν¯RνL,\displaystyle m_{\nu}i\left\langle I\bar{\nu}\nu\right\rangle=m_{\nu}i\left\langle I\bar{\nu}_{L}\nu_{R}+I\bar{\nu}_{R}\nu_{L}\right\rangle, (129)

we can see that the former couples ν¯R\bar{\nu}_{R} with (νR)C(\nu_{R})_{C^{\prime}}, while the later couples ν¯R\bar{\nu}_{R} with νL\nu_{L}. We know that the weaker form of charge conjugation CC^{\prime} (68) is a Clifford-odd operation. It converts the Clifford-even νR\nu_{R} to Clifford-odd (νR)C(\nu_{R})_{C^{\prime}}. Consequently, (νR)C(\nu_{R})_{C^{\prime}} is effectively left-handed and could be coupled to the right-handed ν¯R\bar{\nu}_{R} in a similar fashion as the Dirac mass term.

The observation of neutrino oscillations[78, 79, 80] indicates that neutrinos have nonzero masses which are much smaller than that of the other standard model fermions. If we assume that the neutrino Majorana mass MM is much heavier than the neutrino Dirac mass mνm_{\nu}, a very small effective mass of the order of mν2/Mm_{\nu}^{2}/M can thus be generated for the neutrino. This appealing explanation for the tiny neutrino mass is called the seesaw mechanism [42]. If we could experimentally detect the Majorana nature of the neutrino mass, it would lend support to the seesaw mechanism.

Given that the traditional definition of the Majorana mass involves the charge conjugation CC (67) that converts a particle into its corresponding antiparticle, the traditional Majorana mass term violates the conservation of lepton number and could be confirmed by the lepton number-violating process of the neutrinoless double beta decay. Therefore, it’s widely believed that the observation of the neutrinoless double beta decay could be a confirmation of the Majorana mass. The lepton number-violating process can also be used to explain the origin of matter in the universe via the leptogenesis mechanism [90]. A slew of experiments have been commissioned to search for the neutrinoless double beta decay. As of yet, no evidence of such decay has ever been found [91, 92].

On the other hand, the weaker form of charge conjugation CC^{\prime} (68) does not invoke complex conjugate, and thus there is no particle-antiparticle interchange. Consequently, the Majorana mass term as shown in Eq. (127) conserves lepton number, which is dissimilar to the traditional Majorana mass term that invokes the stronger form of charge conjugation CC. This suggests that the absence of the neutrinoless double beta decay does not disapprove the Majorana mass as defined in Eq. (127). We shall seek other means of the Majorana mass detection.

3.3 Scalar and antisymmetric-tensor Higgs fields

The third step of SSB concerns the well-known electroweak symmetry-breaking Higgs field ϕ\phi of the standard model which couples to both the left-handed and the right-handed fermions. The VEV of the scalar ϕ\phi breaks the standard model symmetries down to SU(3)C×U(1)EMSU(3)_{C}\times U(1)_{EM}. The SSB pattern outlined in this subsection is in many ways similar to the conventional Higgs mechanism, only that it’s transposed onto the Clifford algebraic landscape. That said, toward the end of this subsection we will touch upon a non-scalar Higgs field which could have cosmological implications.

The Higgs field ϕ\phi is valued in the real Clifford algebraic subspace spanned by four Clifford-even multivectors

ϕ\displaystyle\phi =(ϕ0+ϕ1Γ2Γ3+ϕ2Γ3Γ1+ϕ3Γ1Γ2)P+,\displaystyle=(\phi_{0}+\phi_{1}\Gamma_{2}\Gamma_{3}+\phi_{2}\Gamma_{3}\Gamma_{1}+\phi_{3}\Gamma_{1}\Gamma_{2})P_{+}, (130)

where P+P_{+} is the projection operator (24) with the property Γ1Γ2P+=IP+\Gamma_{1}\Gamma_{2}P_{+}=-IP_{+}. The 4 real coefficients {ϕa;a=0,1,2,3}\{\phi_{a};a=0,1,2,3\} correspond to the 2 complex components (i.e. 4 real degrees of freedom) of the traditional Higgs doublet. The Higgs field obeys gauge transformation rules

ϕe12θWL1Γ2Γ3+12θWL2Γ3Γ1+12θWL3Γ1Γ2ϕe12ϵYΓ1Γ2,\displaystyle\phi\quad\rightarrow\quad e^{\frac{1}{2}\theta_{WL}^{1}\Gamma_{2}\Gamma_{3}+\frac{1}{2}\theta_{WL}^{2}\Gamma_{3}\Gamma_{1}+\frac{1}{2}\theta_{WL}^{3}\Gamma_{1}\Gamma_{2}}\;\phi\;e^{-\frac{1}{2}\epsilon_{Y}\Gamma_{1}\Gamma_{2}}, (131)

where {θWL1,θWL2,θWL3}\{\theta_{WL}^{1},\theta_{WL}^{2},\theta_{WL}^{3}\} and ϵY\epsilon_{Y} are the left-handed weak SU(2)WLSU(2)_{WL} and the hypercharge U(1)YU(1)_{Y} gauge transformation parameters. As such, ϕ\phi is a weak doublet and is invariant under the Lorentz Spin(1,3)Spin(1,3) (Lorentz scalar) and the color SU(3)CSU(3)_{C} (color singlet) gauge transformations. Given that P+Γ1Γ2=P+IP_{+}\Gamma_{1}\Gamma_{2}=-P_{+}I, one can replace 12ϵYΓ1Γ2-\frac{1}{2}\epsilon_{Y}\Gamma_{1}\Gamma_{2} with 12ϵYI\frac{1}{2}\epsilon_{Y}I in the above transformations and therefore the Higgs field has Hypercharge 11 (or 12\frac{1}{2} depending on the Hypercharge definition convention). We keep 12ϵYΓ1Γ2-\frac{1}{2}\epsilon_{Y}\Gamma_{1}\Gamma_{2} to highlight its relevance to the Hypercharge symmetry (62).

Note that the Higgs field could take values in a complimentary Clifford-even subspace

ϕ\displaystyle\phi^{\prime} =(ϕ0+ϕ1Γ2Γ3+ϕ2Γ3Γ1+ϕ3Γ1Γ2)P,\displaystyle=(\phi^{\prime}_{0}+\phi^{\prime}_{1}\Gamma_{2}\Gamma_{3}+\phi^{\prime}_{2}\Gamma_{3}\Gamma_{1}+\phi^{\prime}_{3}\Gamma_{1}\Gamma_{2})P_{-}, (132)

where the projection operator is changed from P+P_{+} to PP_{-}. We call the original ϕ\phi (130) and the complimentary ϕ\phi^{\prime} (132) the ϕ+\phi_{+}-type and ϕ\phi_{-}-type Higgs fields, respectively. They have opposite Hypercharges P±Γ1Γ2=P±IP_{\pm}\Gamma_{1}\Gamma_{2}=\mp P_{\pm}I and thus their coupling patterns with the isospin up-type and down-type fermions differ from each other.

It can be verified that the 4 degrees of freedom of ϕ+\phi_{+}-type Higgs field plus the 4 degrees of freedom of ϕ\phi_{-}-type Higgs field amount to the 8 degrees of freedom of the Clifford subspace {1,ΓiΓj,I,IΓiΓj}\{1,\Gamma_{i}\Gamma_{j},I,I\Gamma_{i}\Gamma_{j}\}. The additional ϕ\phi_{-}-type Higgs field can be exploited in various extensions of the standard model such as the two-Higgs-doublet model (2HDM) [93, 94] or the three-Higgs-doublet model (3HDM) [95]. We will circle back to this point in Section 3.4. But for now, let’s focus on the ϕ+\phi_{+}-type Higgs field only.

The standard model gauge-invariant Higgs Lagrangian reads

HiggsElectroweak=(Dμϕ)(Dμϕ)V+(yeiIl¯LϕeR+h.c.),\displaystyle\mathcal{L}_{Higgs-Electroweak}=\left\langle(D^{\mu}\phi)^{\dagger}(D_{\mu}\phi)-V+(y_{e}iI\bar{l}_{L}\phi e_{R}+h.c.)\right\rangle, (133)

where lL=νL+eLl_{L}=\nu_{L}+e_{L} is the left-handed lepton doublet, eRe_{R} is the right-handed electron, yey_{e} is the Yukawa coupling constant, and Higgs potential VV is

V=μ2ϕϕ+λ(ϕϕ)2.\displaystyle V=-\mu^{2}\phi^{\dagger}\phi+\lambda(\phi^{\dagger}\phi)^{2}. (134)

The gauge-covariant derivative is defined as

Dμϕ=(μ+12WLμ1Γ2Γ3+12WLμ2Γ3Γ1+12WLμ3Γ1Γ2)ϕϕ(12AYμΓ1Γ2),\displaystyle D_{\mu}\phi=(\partial_{\mu}+\frac{1}{2}W^{1}_{L\mu}\Gamma_{2}\Gamma_{3}+\frac{1}{2}W^{2}_{L\mu}\Gamma_{3}\Gamma_{1}+\frac{1}{2}W^{3}_{L\mu}\Gamma_{1}\Gamma_{2})\phi-\phi(\frac{1}{2}A_{Y\mu}\Gamma_{1}\Gamma_{2}), (135)

which involves the left-handed weak gauge field W^Lμ\hat{W}_{L\mu} and the Hypercharge gauge field A^Yμ\hat{A}_{Y\mu}. We omit Yukawa terms for non-electron fermions which will be investigated in more detail in Section 3.4 when we tackle the issue of the fermion mass hierarchies. Note that the imaginary number ii shows up in the Yukawa term. This is in compliance with the reality condition.

By virtue of the Mexican hat-shaped potential VV, the Higgs field acquires a nonzero VEV

ϕ=12υEWP+,\displaystyle\phi=\frac{1}{\sqrt{2}}\upsilon_{EW}P_{+}, (136)

where υEW=μλ\upsilon_{EW}=\frac{\mu}{\sqrt{\lambda}} is usually called the electroweak scale. As a result, the gauge fields W^Lμ±\hat{W}^{\pm}_{L\mu} and Z^μ\hat{Z}_{\mu} gain masses. The standard model symmetries are broken down to SU(3)C×U(1)EMSU(3)_{C}\times U(1)_{EM}. The electromagnetic U(1)EMU(1)_{EM} gauge field A^\hat{A} remains massless and has an effective coupling constant of [29]

gEM=gWLgWRgBLgWL2gWR2+gWL2gBL2+gWR2gBL2,\displaystyle g_{EM}=\frac{g_{WL}g_{WR}g_{BL}}{\sqrt{g_{WL}^{2}g_{WR}^{2}+g_{WL}^{2}g_{BL}^{2}+g_{WR}^{2}g_{BL}^{2}}}, (137)

where gWLg_{WL}, gWRg_{WR} and gBLg_{BL} are the left-handed weak, the right-handed weak and the BL coupling constants, respectively. The electromagnetic field A^\hat{A}-related gauge-covariant derivative of the algebraic spinor ψ\psi can be cast into the form

Dμψ=(μ+12AμΓ1Γ2)ψ+ψ(12AμJ)=μψ+qAμψI,\displaystyle D_{\mu}\psi=(\partial_{\mu}+\frac{1}{2}A_{\mu}\Gamma_{1}\Gamma_{2})\psi+\psi(\frac{1}{2}A_{\mu}J)=\partial_{\mu}\psi+qA_{\mu}\psi I, (138)

where qq is the electric charge.

With replacement of ϕ\phi with its VEV, the Yukawa term reduces to the Dirac mass term of electron

meiIe¯e=meiIe¯LeR+Ie¯ReL,\displaystyle m_{e}i\left\langle I\bar{e}e\right\rangle=m_{e}i\left\langle I\bar{e}_{L}e_{R}+I\bar{e}_{R}e_{L}\right\rangle, (139)

where the electron mass mem_{e} is

me=12yeυEW.\displaystyle m_{e}=\frac{1}{\sqrt{2}}y_{e}\upsilon_{EW}. (140)

At this final stage of SSB, we are ready to write down the action of the electron

Selectron=d4x=iψ¯γμ(μψ+qAμψI)+mψ¯ψId4x,\displaystyle S_{electron}=\int\mathcal{L}\;d^{4}x=i\int{\left\langle\bar{\psi}\gamma^{\mu}(\partial_{\mu}\psi+qA_{\mu}\psi I)+m\bar{\psi}\psi I\right\rangle d^{4}x}, (141)

where q=1q=-1 and we relabel ee as ψ\psi and mem_{e} as mm. The Clifford algebraic Dirac equation can be readily derived

γμ(μψIqAμψ)mψ=0.\displaystyle\gamma^{\mu}(\partial_{\mu}\psi I-qA_{\mu}\psi)-m\psi=0. (142)

It’s similar to the conventional Dirac equation, provided that ii is replaced with II positioned on the right side of ψ\psi. It can be used to derive the equation for the CC^{\prime} charge conjugation (68) counterpart ψc\psi_{c^{\prime}}

γμ(μψcI+qAμψc)mψc=0.\displaystyle\gamma^{\mu}(\partial_{\mu}\psi_{c^{\prime}}I+qA_{\mu}\psi_{c^{\prime}})-m\psi_{c^{\prime}}=0. (143)

The above equation demonstrates that the weaker form of charge conjugation CC^{\prime} indeed changes the sign of the electric charge.

We ought to emphasize that the Clifford algebraic Dirac equation (142) without the quantum imaginary number ii is a classical field equation for the classical spinor field ψ\psi, whereas the Clifford functional-differential Schwinger-Dyson equation (178) (which will be derived in Section 4 on field quantization) is the true QFT equation for the quantized spinor field. This is different from the view of regarding Dirac equation as a relativistic version of quantum mechanical equation. As defined in Section 2, the classical spinor field ψ\psi (15) is a Grassmann-valued Clifford algebraic multivector, which is obviously not a complex-valued quantum wave function. Hence the Clifford algebraic Dirac equation (142) could not be regarded as a quantum mechanical equation for quantum wave function. In Section 4 on field quantization, we will formally introduce the quantum imaginary number ii via the Clifford functional integral formalism and further dispel the notion of “first quantization” usually ascribed to Dirac equation.

The electroweak symmetry breaking process delineated in this section bears close resemblance to the traditional Higgs mechanism. Curiously, the Clifford algebra framework allows for a non-scalar Higgs field ϕAT\phi_{AT} which could potentially break both the electroweak and Lorentz symmetries. The non-scalar Higgs field is valued in the real Clifford algebraic subspace spanned by 46=244*6=24 Clifford-even multivectors[29]

γaγb,γaγbΓiΓj,\displaystyle\gamma_{a}\gamma_{b},\quad\gamma_{a}\gamma_{b}\Gamma_{i}\Gamma_{j}, (144)

where i,j=1,2,3,i>j,a,b=0,1,2,3,a>bi,j=1,2,3,i>j,a,b=0,1,2,3,a>b. We have the flexibility of only considering the projected portion ϕAT±=ϕATP±\phi_{AT{\pm}}=\phi_{AT}P_{\pm} with each half having 12 independent Clifford algebraic components. The non-scalar Higgs field obeys the transformation rules

ϕATe14θabγaγb+12θWL1Γ2Γ3+12θWL2Γ3Γ1+12θWL3Γ1Γ2ϕATe12ϵYΓ1Γ214θabγaγb,\displaystyle\phi_{AT}\quad\rightarrow\quad e^{\frac{1}{4}\theta^{ab}\gamma_{a}\gamma_{b}+\frac{1}{2}\theta_{WL}^{1}\Gamma_{2}\Gamma_{3}+\frac{1}{2}\theta_{WL}^{2}\Gamma_{3}\Gamma_{1}+\frac{1}{2}\theta_{WL}^{3}\Gamma_{1}\Gamma_{2}}\;\phi_{AT}\;e^{-\frac{1}{2}\epsilon_{Y}\Gamma_{1}\Gamma_{2}-\frac{1}{4}\theta^{ab}\gamma_{a}\gamma_{b}}, (145)

where θabγaγb\theta^{ab}\gamma_{a}\gamma_{b} are Lorentz transformations. As such, ϕAT\phi_{AT} is a weak doublet as well as a Lorentz sextet (an antisymmetric tensor rather than a scalar). If ϕAT\phi_{AT} acquires a nonzero VEV

ϕAT=12υATγ0γ3,\displaystyle\phi_{AT}=\frac{1}{\sqrt{2}}\upsilon_{AT}\gamma_{0}\gamma_{3}, (146)

it would break the electroweak and Lorentz symmetries at the same time, since it singles out a specific space-time direction via γ0γ3\gamma_{0}\gamma_{3}. The magnitude of this VEV could be extremely small compared with the electroweak scale υATυEW\upsilon_{AT}\ll\upsilon_{EW}, rendering the υAT\upsilon_{AT}-related effects unobservable in laboratories. We hypothesize that the ethereal VEV of the antisymmetric-tensor Higgs field might manifest itself as the large-scale anisotropies of the universe [96, 97, 98, 99, 100, 101].

3.4 The 3HDM and the fermion mass hierarchy problem

Dimensionless ratios between physical constants appearing in a physical theory cannot be accidentally small. The technical naturalness principle is elegantly defined by ’t Hooft [102]: A quantity should be small only if the underlying theory becomes more symmetric as that quantity tends to zero. The weakly broken symmetry ensures that the smallness of a parameter is preserved against possible large quantum corrections.

For the application of the naturalness principle, let’s examine two global symmetries related to the vector UV(1)U_{V}(1) phase transformation
ψL\displaystyle\psi_{L} ψLeθVI,ψRψReθVI,\displaystyle\quad\rightarrow\quad\psi_{L}e^{\theta_{V}I},\quad\quad\psi_{R}\quad\rightarrow\quad\psi_{R}e^{\theta_{V}I}, (147a)
ϕM\displaystyle\phi_{M} ϕMe2θVI,\displaystyle\quad\rightarrow\quad\phi_{M}e^{2\theta_{V}I}, (147b)
ϕ\displaystyle\phi ϕ,\displaystyle\quad\rightarrow\quad\phi, (147c)

and the axial UA(1)U_{A}(1) phase transformation

ψL\displaystyle\psi_{L} ψLeθAI,ψRψReθAI,\displaystyle\quad\rightarrow\quad\psi_{L}e^{-\theta_{A}I},\quad\psi_{R}\quad\rightarrow\quad\psi_{R}e^{\theta_{A}I}, (148a)
ϕM\displaystyle\phi_{M} ϕMe2θAI,\displaystyle\quad\rightarrow\quad\phi_{M}e^{2\theta_{A}I}, (148b)
ϕ\displaystyle\phi ϕe2θAI,\displaystyle\quad\rightarrow\quad\phi e^{2\theta_{A}I}, (148c)

where ψL\psi_{L} is the left-handed spinor, ψR\psi_{R} is the right-handed spinor, ϕM\phi_{M} is the Majorana-Higgs field, and ϕ\phi is the regular Higgs field. The phase transformation rules for ϕM\phi_{M} and ϕ\phi may not seem intuitive. But when we consider ϕM\phi_{M} and ϕ\phi as multi-fermion condensations in Section 4.2, the reason for these transformation rules will become clear.

For later discussion, let’s also introduce a Uα(1)U_{\alpha}(1) phase transformation for the right-handed spinors

ψL\displaystyle\psi_{L} ψL,ψRψReαI,\displaystyle\quad\rightarrow\quad\psi_{L},\quad\quad\quad\psi_{R}\quad\rightarrow\quad\psi_{R}e^{\alpha I}, (149a)
ϕM\displaystyle\phi_{M} ϕMe2αI,\displaystyle\quad\rightarrow\quad\phi_{M}e^{2\alpha I}, (149b)
ϕ\displaystyle\phi ϕeαI,\displaystyle\quad\rightarrow\quad\phi e^{\alpha I}, (149c)

which is basically a combination of UV(1)U_{V}(1) and UA(1)U_{A}(1) .

It can be checked that, when ϕM\phi_{M} and ϕ\phi are replaced by their VEVs, the Majorana (127) and Dirac (139) mass terms violate the UV(1)U_{V}(1)/UA(1)U_{A}(1)/Uα(1)U_{\alpha}(1) and UA(1)U_{A}(1)/Uα(1)U_{\alpha}(1) symmetries, respectively. Hence the Majorana and Dirac masses are technically natural, given that these global symmetries can be restored if the Majorana and Dirac masses are set to zero. In other words, the smallness of the Majorana and Dirac masses are protected by the global symmetries against possible large quantum corrections.

Prior to the SSB induced by ϕM\phi_{M} and ϕ\phi, these two Higgs fields would transform according to the aforementioned global phase transformation rules. It can be shown that all the terms of the Lagrangian of the world (85) respect the UV(1)U_{V}(1), UA(1)U_{A}(1), and Uα(1)U_{\alpha}(1) global symmetries, with only one exception which is the UA(1)U_{A}(1)/Uα(1)U_{\alpha}(1)-violating electron Yukawa term in Eq. (133). It would be nice if we can tinker with the UA(1)U_{A}(1)/Uα(1)U_{\alpha}(1) transformation rule for ϕ\phi, so that the entire Lagrangian of the world is invariant. Contrary to our expectation, it’s not achievable. Within the confines of a single standard model Higgs field ϕ\phi, it is impossible to make both the isospin up-type and down-type fermion Yukawa terms UA(1)U_{A}(1)/Uα(1)U_{\alpha}(1)-invariant.

The seemingly worrisome symmetry-violating Yukawa terms can be turned into our advantage. In the spirit of the technical naturalness principle, we can exploit the global symmetry properties to explain the vast range of fermion masses which span five orders of magnitude between the heaviest top quark and the lightest electron. The key for solving the fermion mass hierarchy problem is to realize that some of the Yukawa coupling constants are actually not constants at all [30]. Embedded in the Yukawa couplings, there are six Clifford-valued bosonic scalar fields

Φαt\displaystyle\Phi_{\alpha t} =Φαt1+Φαt2I,Φβt=Φβt1+Φβt2I,\displaystyle=\Phi_{\alpha t1}+\Phi_{\alpha t2}I,\quad\quad\Phi_{\beta t}=\Phi_{\beta t1}+\Phi_{\beta t2}I, (150)
Φαντ\displaystyle\Phi_{\alpha{\nu_{\tau}}} =Φαντ1+Φαντ2I,Φβντ=Φβντ1+Φβντ2I,\displaystyle=\Phi_{\alpha{\nu_{\tau}}1}+\Phi_{\alpha{\nu_{\tau}}2}I,\quad\Phi_{\beta{\nu_{\tau}}}=\Phi_{\beta{\nu_{\tau}}1}+\Phi_{\beta{\nu_{\tau}}2}I, (151)
Φατ\displaystyle\Phi_{\alpha{\tau}} =Φατ1+Φατ2I,Φβτ=Φβτ1+Φβτ2I,\displaystyle=\Phi_{\alpha{\tau}1}+\Phi_{\alpha{\tau}2}I,\quad\quad\Phi_{\beta{\tau}}=\Phi_{\beta{\tau}1}+\Phi_{\beta{\tau}2}I, (152)

where all the coefficients, such as Φαt1\Phi_{\alpha t1} and Φαt2\Phi_{\alpha t2}, are real numbers.

The three α\alpha-type Φ\Phi fields are tied to the U(1)αU(1)_{\alpha} symmetry, while the three β\beta-type Φ\Phi fields are tied to a novel U(1)βU(1)_{\beta} symmetry (see table 1). The global symmetry-violating nature of the effective Yukawa terms originates from these six Φ\Phi fields acquiring nonzero VEVs via the SSB mechanism. Note that these Φ\Phi fields are gauge singlets, i.e. they are invariant under all the gauge transformations. This is in contrast to the regular electroweak Higgs field which is a weak SU(2)WLSU(2)_{WL} doublet.

To account for the masses of the three families of fermions, we adopt three Higgs fields in our model (a.k.a. 3HDM), namely, the top-quark Higgs field ϕt\phi_{t}, the tau-neutrino Higgs field ϕντ\phi_{\nu_{\tau}}, and the tau-lepton Higgs field ϕτ\phi_{\tau}. The naming convention of the three Higgs fields and the six Φ\Phi fields will become clear when we related them to their corresponding quantum condensations in Section 4.2. Among these Higgs fields, ϕt\phi_{t} and ϕντ\phi_{\nu_{\tau}} are ϕ+\phi_{+}-type Higgs field (130), while ϕτ\phi_{\tau} is ϕ\phi_{-}-type Higgs field (132). All the three Higgs doublets obey the usual gauge transformation rules for the electroweak Higgs field (131).

We introduce one more global symmetry U(1)βU(1)_{\beta} which, like U(1)αU(1)_{\alpha}, is related to the phases of the right-handed fermions. However, the U(1)βU(1)_{\beta} charge is not uniformly assigned to fermions. While Uα(1)U_{\alpha}(1) transforms all the right-handed fermions by the same phase eαIe^{\alpha I}, Uβ(1)U_{\beta}(1) transforms the isospin up-type quarks (uRu_{R}, cRc_{R}, tRt_{R}) and down-type leptons (eRe_{R}, μR\mu_{R}, τR\tau_{R}) by the phase eβIe^{\beta I} and it transforms the down-type quarks (dRd_{R}, sRs_{R}, bRb_{R}) and up-type leptons (νeR\nu_{eR}, νμR\nu_{{\mu}R}, ντR\nu_{{\tau}R}) by the opposite phase eβIe^{-\beta I}. The U(1)αU(1)_{\alpha}/U(1)βU(1)_{\beta} charge assignments are summarized in table 1.

Table 1: The U(1)αU(1)_{\alpha} and U(1)βU(1)_{\beta} charge
uR{u_{R}},cR{c_{R}},tR{t_{R}}, dR{d_{R}},sR{s_{R}},bR{b_{R}}, ϕt\phi_{t} ϕντ\phi_{\nu_{\tau}} ϕτ\phi_{\tau} Φαt\Phi_{\alpha t}, Φαντ\Phi_{\alpha{\nu_{\tau}}}, Φβt\Phi_{\beta t}, Φβντ\Phi_{\beta{\nu_{\tau}}},
eR{e_{R}},μR{\mu_{R}},τR{\tau_{R}} νeR{\nu_{eR}},νμR{\nu_{\mu R}},ντR{\nu_{\tau R}} Φατ\Phi_{\alpha{\tau}} Φβτ\Phi_{\beta{\tau}}
U(1)αU(1)_{\alpha} 1 1 1 1 1 -2 0
U(1)βU(1)_{\beta} 1 -1 1 -1 1 0 -2

It will be shown later in this subsection that the two global symmetries U(1)αU(1)_{\alpha} and U(1)βU(1)_{\beta} are instrumental in determining the relative magnitudes of the effective Yukawa coupling constants, and consequently establishing the fermion mass hierarchies. As the U(1)αU(1)_{\alpha} charge assignment is analogous to that of the Peccei-Quinn U(1)PQU(1)_{PQ} symmetry [103], we will use the term U(1)αU(1)_{\alpha} and U(1)PQU(1)_{PQ} interchangeably henceforth.

Now we are ready to write down the Yukawa coupling terms for all three generations of the standard model fermions (plus right-handed neutrinos)
igtIq¯L3ϕ~ttR+gνeΦβtIl¯L1ϕ~tνeR+gbΦαtIq¯L3ϕtbR+geΦαtΦβtIl¯L1ϕteR+h.c.\displaystyle i\left\langle g_{t}I\bar{q}^{3}_{L}\tilde{\phi}_{t}{t}_{R}+g_{\nu_{e}}{\Phi}^{\dagger}_{\beta t}I\bar{l}^{1}_{L}\tilde{\phi}_{t}{\nu}_{eR}+g_{b}\Phi_{\alpha t}I\bar{q}^{3}_{L}{\phi}_{t}{b}_{R}+g_{e}\Phi_{\alpha t}\Phi_{\beta t}I\bar{l}^{1}_{L}{\phi}_{t}{e}_{R}\right\rangle+h.c. (153a)
+\displaystyle+ igντIl¯L3ϕ~ντντR+gcΦβντIq¯L2ϕ~ντcR+gμΦαντIl¯L2ϕντμR+gdΦαντΦβντIq¯L1ϕντdR\displaystyle i\left\langle g_{{\nu}_{\tau}}I\bar{l}^{3}_{L}\tilde{\phi}_{\nu_{\tau}}{\nu}_{\tau R}+g_{c}\Phi_{\beta{\nu_{\tau}}}I\bar{q}^{2}_{L}\tilde{\phi}_{\nu_{\tau}}{c}_{R}+g_{\mu}\Phi_{\alpha{\nu_{\tau}}}I\bar{l}^{2}_{L}{\phi}_{\nu_{\tau}}{\mu}_{R}+g_{d}\Phi_{\alpha{\nu_{\tau}}}{\Phi}^{\dagger}_{\beta{\nu_{\tau}}}I\bar{q}^{1}_{L}{\phi}_{\nu_{\tau}}{d}_{R}\right\rangle
+h.c.\displaystyle+h.c. (153b)
+\displaystyle+ igτIl¯L3ϕ~ττR+gsΦβτIq¯L2ϕ~τsR+gνμΦατIl¯L2ϕτνμR+guΦατΦβτIq¯L1ϕτuR+h.c.,\displaystyle i\left\langle g_{\tau}I\bar{l}^{3}_{L}\tilde{\phi}_{\tau}{\tau}_{R}+g_{s}{\Phi}^{\dagger}_{\beta{\tau}}I\bar{q}^{2}_{L}\tilde{\phi}_{\tau}{s}_{R}+g_{\nu_{\mu}}\Phi_{\alpha{\tau}}I\bar{l}^{2}_{L}{\phi}_{\tau}\nu_{\mu R}+g_{u}\Phi_{\alpha{\tau}}\Phi_{\beta{\tau}}I\bar{q}^{1}_{L}{\phi}_{\tau}{u}_{R}\right\rangle+h.c., (153c)

where gt,gντ,g_{t},g_{{\nu}_{\tau}},\cdots are the bare Yukawa coupling constants which are dimensionless parameters of order O(1)O(1). The left-handed doublets are

lL1=νeL+eL,qL1=uL+dL,\displaystyle l^{1}_{L}=\nu_{eL}+e_{L},\quad q^{1}_{L}=u_{L}+d_{L}, (154)
lL2=νμL+μL,qL2=cL+sL,\displaystyle l^{2}_{L}=\nu_{\mu L}+\mu_{L},\quad q^{2}_{L}=c_{L}+s_{L}, (155)
lL3=ντL+τL,qL3=tL+bL,\displaystyle l^{3}_{L}=\nu_{\tau L}+\tau_{L},\quad q^{3}_{L}=t_{L}+b_{L}, (156)

where quarks stand for color triplets, such as uL=urL+ugL+ubLu_{L}=u_{rL}+u_{gL}+u_{bL}. From the Yukawa coupling pattern we can tell that the Φ\Phi singlets are of mass dimension zero, different from the traditional mass dimension-one scalar fields. Alternatively, we can rewrite these singlets as the conventional mass dimension-one scalar fields, as long as they show up in the Yukawa terms as Φ/M\Phi/M with MM being an unknown energy scale.

As we have mentioned before, ϕt{\phi_{t}} is a ϕ+\phi_{+}-type Higgs field, which means that it can only couple to the isospin down-type fermions such as bR{b}_{R} and eR{e}_{R}, whereas direct coupling to the up-type fermions is prohibited. Only a transformed form of ϕt{\phi_{t}}

ϕt~=14γμϕtγμ,\displaystyle\tilde{\phi_{t}}=\frac{1}{4}\gamma^{\mu}\phi_{t}\gamma_{\mu}, (157)

can couple to the up-type fermions such as tR{t}_{R} and νeR{\nu}_{eR}. Note that γμ\gamma_{\mu} flips the sign of P±P_{\pm}: P±γμ=γμPP_{\pm}\gamma_{\mu}=\gamma_{\mu}P_{\mp}. Therefore, ϕt~\tilde{\phi_{t}} effectively turns a ϕ+\phi_{+}-type Higgs field ϕt\phi_{t} into a ϕ\phi_{-}-type Higgs field. Similar logic applies to ϕντ{\phi}_{\nu_{\tau}} and ϕτ{\phi}_{\tau}, which are ϕ+\phi_{+}-type and ϕ\phi_{-}-type, respectively.

The conventional QFT formalism leverages a different transformation of the standard model Higgs field

ϕ~=iσ2ϕ,\displaystyle\tilde{\phi}=i\sigma_{2}\phi^{*}, (158)

so that ϕ~\tilde{\phi} can be coupled to up-type fermions. It involves the complex conjugate, whereas the Clifford algebra version (157) doesn’t.

The Yukawa coupling scheme (153) partitions fermions into three cohorts, namely

ϕtcohort\displaystyle{\phi}_{t}\quad cohort :t,νe,b,e,\displaystyle:t,{\nu}_{e},b,e, (159)
ϕντcohort\displaystyle{\phi}_{\nu_{\tau}}\quad cohort :ντ,c,μ,d,\displaystyle:\nu_{\tau},c,{\mu},d, (160)
ϕτcohort\displaystyle{\phi}_{\tau}\quad cohort :τ,s,νμ,u.\displaystyle:{\tau},s,\nu_{\mu},u. (161)

The right-handed fermions in each cohort only couple to the designated Higgs field, thus preventing the flavor-changing neutral currents (FCNCs). Within each of the Higgs field cohort, only one out of the four Yukawa terms is free from the Φ\Phi coupling. This is because that in each of the Higgs field cohort, three out of the four Yukawa terms violate the U(1)αU(1)_{\alpha}/U(1)βU(1)_{\beta} symmetries without including the additional Φ\Phi singlets. After inserting these Φ\Phi singlets in the Yukawa couplings, it can be verified that all the Yukawa terms respect the U(1)αU(1)_{\alpha} and U(1)βU(1)_{\beta} global symmetries.

The coupling patterns (153) of the three Higgs fields are predicated on an alternative generation/family assignment,

Generation0\displaystyle Generation\quad 0 :t,b,νe,e,\displaystyle:\quad t,b,\nu_{e},e, (162)
Generation+\displaystyle Generation\quad+ :c,s,ντ,τ,\displaystyle:\quad c,s,\nu_{\tau},\tau, (163)
Generation\displaystyle Generation\quad- :u,d,νμ,μ,\displaystyle:\quad u,d,\nu_{\mu},\mu, (164)

which are tied to the flavor projection operators {ζ0\zeta^{0}, ζ+\zeta^{+}, ζ\zeta^{-}[29, 30] associated with ternary Clifford algebra [104, 105]. These flavor projection operators dictate the ζ+\zeta^{+}/ζ\zeta^{-} mixing between the ϕντ{\phi}_{\nu_{\tau}} cohort and the ϕτ{\phi}_{\tau} cohort. The projection operators can also be applied to the Majorana-type Yukawa coupling and the resultant Majorana mass can directly mix the νμR\nu_{\mu R} and ντR\nu_{\tau R} neutrinos [29, 30] which is evidenced in the observation of neutrino oscillations[78, 79, 80]. Other flavor mixing phenomena might also be accommodated by the framework, which we defer to future research.

We assume that the Lagrangians of the three Higgs doublets and six Φ\Phi singlets are analogous to the one specified for the regular Higgs mechanism (133), albeit the potential VV could be more complicated, such as involving cross terms mixing different scalar fields [94, 95]. The study of the exact form of VV is beyond the scope of this paper. For our purpose here, we just postulate that these fields acquire the following nonzero VEVs

ϕt=12υtP+,ϕντ=12υντP+,ϕτ=12υτP,\displaystyle\phi_{t}=\frac{1}{\sqrt{2}}\upsilon_{t}P_{+},\quad{\phi}_{\nu_{\tau}}=\frac{1}{\sqrt{2}}\upsilon_{\nu_{\tau}}P_{+},\quad{\phi}_{\tau}=\frac{1}{\sqrt{2}}\upsilon_{\tau}P_{-}, (165)
Φαt=υαt,Φαντ=υαντ,Φατ=υατ,\displaystyle\Phi_{\alpha t}=\upsilon_{\alpha t},\quad\Phi_{\alpha{\nu_{\tau}}}=\upsilon_{\alpha{\nu_{\tau}}},\quad\Phi_{\alpha{\tau}}=\upsilon_{\alpha{\tau}}, (166)
Φβt=υβt,Φβντ=υβντ,Φβτ=υβτ.\displaystyle\Phi_{\beta t}=\upsilon_{\beta t},\quad\Phi_{\beta{\nu_{\tau}}}=\upsilon_{\beta{\nu_{\tau}}},\quad\Phi_{\beta{\tau}}=\upsilon_{\beta{\tau}}. (167)

The three Φα\Phi_{\alpha}-type fields break the global U(1)αU(1)_{\alpha}/U(1)PQU(1)_{PQ} symmetry, while the three Φβ\Phi_{\beta}-type fields break the global U(1)βU(1)_{\beta} symmetry. Note that the Φ\Phi fields do not break any local gauge symmetry since they are gauge singlets. Post the SSB, there will be six massive sigma modes and six Nambu-Goldstone modes. As opposed to the Higgs mechanism, the Nambu-Goldstone modes are not “eaten” by the gauge field. Due to the explicit symmetry breaking originated from the quantum anomaly and instanton effects, the otherwise massless Nambu-Goldstone bosons of the three Φα\Phi_{\alpha} fields acquire masses and turn into pseudo-Nambu-Goldstone bosons in a similar fashion as the axions [103, 106, 107]. Since the Φα\Phi_{\alpha} fields are local gauge (especially electroweak) singlets, they are more in line with the invisible axions [108, 109, 110, 111]. The axions have historically been proposed as dark matter candidates as well as a possible solution to the strong CP problem. We leave the investigation of the U(1)βU(1)_{\beta}-type (pseudo-)Nambu-Goldstone boson’s role as dark matter to future study.

After replacement of the three Higgs doublets and six Φ\Phi singlets with their VEVs, the Yukawa terms reduce to the Dirac mass terms

gtυtiIt¯t+gνeυβtυtiIν¯eνe+gbυαtυtiIb¯b+geυαtυβtυtiIe¯e\displaystyle g_{t}\upsilon_{t}i\left\langle I\bar{t}t\right\rangle+g_{\nu_{e}}\upsilon_{\beta t}\upsilon_{t}i\left\langle I\bar{\nu}_{e}\nu_{e}\right\rangle+g_{b}\upsilon_{\alpha t}\upsilon_{t}i\left\langle I\bar{b}b\right\rangle+g_{e}\upsilon_{\alpha t}\upsilon_{\beta t}\upsilon_{t}i\left\langle I\bar{e}e\right\rangle (168a)
+\displaystyle+ gντυντiIν¯τντ+gcυβντυντiIc¯c+gμυαντυντiIμ¯μ+gdυαντυβντυντiId¯d\displaystyle g_{\nu_{\tau}}\upsilon_{\nu_{\tau}}i\left\langle I\bar{\nu}_{\tau}\nu_{\tau}\right\rangle+g_{c}\upsilon_{\beta{\nu_{\tau}}}\upsilon_{\nu_{\tau}}i\left\langle I\bar{c}c\right\rangle+g_{\mu}\upsilon_{\alpha{\nu_{\tau}}}\upsilon_{\nu_{\tau}}i\left\langle I\bar{\mu}\mu\right\rangle+g_{d}\upsilon_{\alpha{\nu_{\tau}}}\upsilon_{\beta{\nu_{\tau}}}\upsilon_{\nu_{\tau}}i\left\langle I\bar{d}d\right\rangle (168b)
+\displaystyle+ gτυτiIτ¯τ+gsυβτυτiIs¯s+gνμυατυτiIν¯μνμ+guυατυβτυτiIu¯u,\displaystyle g_{{\tau}}\upsilon_{{\tau}}i\left\langle I\bar{{\tau}}{\tau}\right\rangle+g_{s}\upsilon_{\beta{\tau}}\upsilon_{{\tau}}i\left\langle I\bar{s}s\right\rangle+g_{\nu_{\mu}}\upsilon_{\alpha{\tau}}\upsilon_{{\tau}}i\left\langle I\bar{\nu}_{\mu}\nu_{\mu}\right\rangle+g_{u}\upsilon_{\alpha{\tau}}\upsilon_{\beta{\tau}}\upsilon_{{\tau}}i\left\langle I\bar{u}u\right\rangle, (168c)

where for the sake of brevity, all terms are re-scaled by 2\sqrt{2}.

Before making contact with the experimental results, we have to identify which mode of the three Higgs doublets corresponds to the 125 GeV boson observed at the Large Hadron Collider [112, 113]. Generally speaking, a Higgs boson can be defined as a linear combination of the Clifford-scalar sector (with VEVs subtracted) of the three Higgs fields. For an order-of-magnitude analysis, let’s assume that the 125GeV125\;GeV Higgs boson is aligned with the top-quark Higgs field ϕt\phi_{t}. Therefore the VEV of ϕt\phi_{t} is approximately

υt246GeV,\displaystyle\upsilon_{t}\approx 246GeV, (169)

and the bare Yukawa coupling constant gtg_{t} can be identified as the top quark Yukawa constant yt=gty_{t}=g_{t}. For the sake of estimation, we make the further assumption that the bare Yukawa coupling constants are almost uniform

yt=gtgνegu.\displaystyle y_{t}=g_{t}\approx g_{\nu_{e}}\approx\cdots\approx g_{u}. (170)

The standard model Yukawa constants, except yty_{t}, can be regarded as effective coupling constants. For example, the bottom quark’s effective Yukawa constant is yb=ytυαty_{b}=y_{t}\upsilon_{\alpha t}, and tau neutrino’s effective Yukawa constant is yντ=ytυντ/υty_{\nu_{\tau}}=y_{t}\upsilon_{\nu_{\tau}}/\upsilon_{t}.

Aided by the above assumptions and the mass formula (168), we arrive at an estimation of the Higgs/Φ\Phi VEVs and the neutrino Dirac masses as shown in table 2, where the known fermion masses are also included for comparison.

Table 2: Higgs VEVs (MeV), Φ\Phi VEVs, and Dirac masses (MeV)
ϕt\phi_{t} Cohort ϕντ{\phi}_{\nu_{\tau}} Cohort ϕτ{\phi}_{\tau} Cohort
Higgs VEVs υt\upsilon_{t} 246,000 υντ\upsilon_{\nu_{\tau}} 41,900 υτ\upsilon_{\tau} 2,530
Φα\Phi_{\alpha} VEVs υαt\upsilon_{\alpha t} 1/411/41 υαντ\upsilon_{\alpha{\nu_{\tau}}} 1/2781/278 υατ\upsilon_{\alpha{\tau}} 1/441/44
Φβ\Phi_{\beta} VEVs υβt\upsilon_{\beta t} 1/82001/8200 υβντ\upsilon_{\beta{\nu_{\tau}}} 1/231/23 υβτ\upsilon_{\beta{\tau}} 1/191/19
tt 173,000 ντ\nu_{\tau} 29,500 τ{\tau} 1,780
Dirac Masses νe{{\nu_{e}}} 21 c{{c}} 1,280 s{{s}} 96
b{b} 4,180 μ{\mu} 106 νμ{{\nu_{\mu}}} 40
e{e} 0.51 d{d} 4.6 u{u} 2.2

There are a couple of takeaways from the above estimations. First of all, the magnitudes of Φ\Phi VEVs (υαt,υβt,\upsilon_{\alpha t},\upsilon_{\beta t},\cdots) are all small, albeit to varying degrees. In accordance with the technical naturalness principle of ’t Hooft [102], the weakly broken symmetries of U(1)αU(1)_{\alpha}/U(1)βU(1)_{\beta} ensure that the smallness of the VEVs is preserved against possible quantum corrections. We have mentioned earlier that the Φ\Phi singlets can be considered as traditional mass dimension-one scalar fields characterized by an energy scale MM. We assume that the energy scale MM is higher than the Majorana scale υM\upsilon_{M} (124). This is to ensure that the Φ\Phi field-induced U(1)αU(1)_{\alpha}/U(1)βU(1)_{\beta} global symmetry breaking process is decoupled from the Higgs(-like) symmetry breaking mechanism triggered by either the Majorana-Higgs field ϕM\phi_{M} or the electroweak Higgs fields ϕt\phi_{t}, ϕντ{\phi}_{\nu_{\tau}}, and ϕτ{\phi}_{\tau}.

The Φ\Phi VEVs play a crucial role in determining the magnitudes of the effective Yukawa constants and thus establishing the fermion mass hierarchies within each of the ϕt\phi_{t}, ϕντ{\phi}_{\nu_{\tau}}, and ϕτ{\phi}_{\tau} cohorts. On the other hand, the relative fermion mass sizes between different ϕ\phi cohorts are controlled by the Higgs VEVs (υt,υντ,υτ\upsilon_{t},\upsilon_{\nu_{\tau}},\upsilon_{\tau}).

The fermion masses within a given ϕ{\phi} cohort are mostly in a descending order in each column of table  2. The only exception is the reversed order between the νe{\nu_{e}} and b{b} masses due to the abnormally small magnitude of the Φβt\Phi_{\beta t} VEV (υβt1/8200\upsilon_{\beta t}\sim 1/8200) compared with the other Φ\Phi VEVs. Note that the estimated neutrino masses are meant to be the Dirac masses, as opposed to the much smaller seesaw effective masses or the vastly larger Majorana masses discussed in Section 3.2. Interestingly, according to our estimation, the Dirac mass of the ντ\nu_{\tau} neutrino (mντ29,500MeVm_{\nu_{\tau}}\sim 29,500MeV) is considerably larger than those of the νμ{{\nu_{\mu}}} and νe{{\nu_{e}}} neutrinos (mνμ40MeVm_{{\nu_{\mu}}}\sim 40MeV and mνe21MeVm_{{\nu_{e}}}\sim 21MeV).

Secondly, assuming that there is no cross term between the kinetic part of the three Higgs Lagrangians, the masses of the W±W^{\pm} and Z0Z^{0} bosons can be calculated as

mW±\displaystyle m_{W^{\pm}} =12υtotalgWL,\displaystyle=\frac{1}{2}\upsilon_{total}g_{WL}, (171)
mZ0\displaystyle m_{Z^{0}} =12υtotalgWL2+gY2,\displaystyle=\frac{1}{2}\upsilon_{total}\sqrt{g_{WL}^{2}+g_{Y}^{2}}, (172)

where gWLg_{WL} and gYg_{Y} are the weak and Hypercharge gauge coupling constants. The total electroweak scale υtotal\upsilon_{total} is dependent on all three Higgs VEVs

υtotal=υt2+υντ2+υτ2.\displaystyle\upsilon_{total}=\sqrt{\upsilon_{t}^{2}+\upsilon_{\nu_{\tau}}^{2}+\upsilon_{{\tau}}^{2}}. (173)

According to table 2, the estimated three Higgs VEVs {υt\upsilon_{t}, υντ\upsilon_{\nu_{\tau}}, υτ\upsilon_{{\tau}} } have a hierarchical structure

246GeV42GeV2.5GeV,\displaystyle 246\;GeV\gg 42\;GeV\gg 2.5\;GeV, (174)

where the ϕt\phi_{t} Higgs VEV is significantly larger than the other two. The ϕντ\phi_{\nu_{\tau}} Higgs VEV plays a non-negligible role in the electroweak scale saturation.

The total electroweak scale υtotal\upsilon_{total} is dominated by the ϕt\phi_{t} Higgs VEV. The ratio between them is given by

υtotalυt=1.014.\displaystyle\frac{\upsilon_{total}}{\upsilon_{t}}=1.014. (175)

Given the assumption that the 125GeV125\;GeV Higgs boson is attributed to the top-quark Higgs field ϕt\phi_{t}, this 1.4%1.4\% discrepancy might be the underlying reason for the deviation of the measured W-boson mass from the standard model prediction [114]. If we tweak the uniform Yukawa coupling assumption by proposing that the bare Yukawa couplings of the ϕντ\phi_{\nu_{\tau}} cohort are 5 times larger than the other bare Yukawa couplings, then the υtotal/υt{\upsilon_{total}}/{\upsilon_{t}} difference is around 0.06%0.06\%, in the neighborhood of what is observed by the CDF Collaboration [114].

And lastly, according to the Yukawa coupling scheme (153), the muon belongs to the tau-neutrino Higgs field hντh_{\nu_{\tau}} cohort. Given the intrinsic connection between the muon and the hντh_{\nu_{\tau}} Higgs field, it is worthwhile to investigate the hντh_{\nu_{\tau}} Higgs field’s contribution to the muon anomalous magnetic moment, especially in light of the recent muon g2g-2 measurement with improved accuracy which confirms a deviation from the standard model prediction [115].

4 Quantum Condensation and Naturalness Problems

In this section, we investigate the extended gauge symmetries and contemplate naturalness problems through the lens of quantum condensations. While in the previous section the symmetry-breaking fields are regarded as fundamental fields, in the current section we propose that each and every symmetry-breaking bosonic field is an effective representation of a unique multi-fermion quantum condensation via the dynamical symmetry breaking mechanism. All the mass scales of the universe, including the Planck scale MplM_{\mathrm{pl}}, are quantum emergent. Each mass scale is associated with a particular symmetry and the corresponding symmetry breaking process via quantum condensation.

According to the QFT renormalization procedure, a divergent Feynman integral AA needs to be regularized at the intermediate stage. After renormalization, a finite and regularization scheme-independent result <A>R<A>_{R} can be obtained, so that it can be compared with measurable quantities. As detailed in this section, we advocate a paradigm shift from the conventional renormalization procedure: We stipulate that the relationship involving the renormalized values of the multiplications of divergent Feynman integrals such as <A4>R=(<A2>R)2<A^{4}>_{R}=(<A^{2}>_{R})^{2} shall be avoided. This means that even though we have seemingly only one divergent Feynman integral AA, there could be multiple unrelated scales, in stark contrast to the conventional QFT renormalization procedure (or the Wilsonian renormalization group approach) characterized by a single renormalization scale.

In the case of the cosmological constant Λ\Lambda , the implication is that Λ\Lambda (which is linked to <A4>R<A^{4}>_{R}) should be deemed as a parameter completely decoupled from the Planck scale MplM_{\mathrm{pl}} (which is linked to (<A2>R)2(<A^{2}>_{R})^{2}). The magnitudes of these two scales could differ vastly from each other. Hence the cosmological constant problem can be evaded.

4.1 Quantization via the Clifford functional integral formalism

As mentioned in the introduction section, there are two kinds of imaginary numbers. One is the genuine ii which is central to the quantum theory. The other one can be replaced by the pseudoscalar II which shows up in the definition of spinors and gauge fields. Intriguingly, the imaginary number ii is inextricably embedded in the classical fermion Lagrangians (89) and (141), which suggests that there might be quantum phenomenon lurking beneath the veneer of the classical Lagrangian terms. It eventually leads us to the epiphany that quantum condensations may hold the golden key to various sorts of naturalness problems.

But first, let’s examine how to quantize the classical spinor fields. Historically, field quantization is also referred to as “second quantization”. However, “second quantization” would be a misnomer in our case here, since there is no separate “first quantization” in the first place when we define the classical spinor, gauge, vierbein, and Higgs fields in Section 2 and Section 3.

Different Clifford algebraic field quantization methods have been proposed in the literature [18, 24]. With the goal of quantizing the classical Grassmann-odd spinor fields valued in the Clifford algebraic space, we have developed the Clifford functional integral formalism in our earlier paper [31], whereby the generating functional Z[η]Z[\eta] for the spinors can be represented by the Clifford functional integral

Z[η]\displaystyle Z[\eta] =𝒟ψe12d4x{i[ψ]+Iη¯(x)ψ(x)+Iψ¯(x)η(x)},\displaystyle=\int\mathcal{D}\psi e^{\frac{1}{2}\int d^{4}x\{i\mathcal{L}[\psi]+\left\langle I\bar{\eta}(x)\psi(x)+I\bar{\psi}(x)\eta(x)\right\rangle\}}, (176)

where we formally introduce the imaginary number ii in front of the Lagrangian i[ψ]i\mathcal{L[\psi]} which is essential for quantization. The real Grassmann-odd sources η(x)\eta(x) and η¯(x)\bar{\eta}(x) are valued in the same Clifford space as ψ(x)\psi(x) and ψ¯(x)\bar{\psi}(x). It is understood that Z[η]Z[\eta] satisfies the normalization condition Z[0]=1Z[0]=1.

Note that we have adopted the natural units c==1c=\hbar=1 in this paper. If we write out the Planck constant \hbar explicitly, the Lagrangian [ψ]\mathcal{L}[\psi] in the Clifford functional integral (176) shall be replace by /\mathcal{L}/\hbar. As a universal rule, we should always deem /\mathcal{L}/\hbar as an inseparable quantity whenever we use the Lagrangian with or without quantization. One implication is that the Planck constant \hbar from the Dirac derivative γμiμ\gamma^{\mu}i\hbar\partial_{\mu} in the spinor Lagrangian [ψ]\mathcal{L}[\psi] is canceled out by the denominator \hbar in /\mathcal{L}/\hbar. Therefore, there is no explicit \hbar in the spinor /\mathcal{L}/\hbar, which dovetails nicely with our earlier argument about no “first quantization”. The generalized rule of treating /{\mathcal{L}}/{\hbar} as de facto Lagrangian could lead to an alternative view on the choice of physics units [116, 117].

We regard ψ(x)\psi(x) and ψ¯(x)\bar{\psi}(x) as dependent variables, as opposed to the traditional way of treating them as independent variables (as such, the functional integration is over 𝒟ψ\mathcal{D}\psi rather than 𝒟ψ𝒟ψ¯\mathcal{D}\psi\mathcal{D}\bar{\psi}). The same logic applies to η(x)\eta(x) and η¯(x)\bar{\eta}(x). Therefore, an extra 1/2{1}/{2} factor in front of the action is required to keep the calculated quantities, such as the fermion propagators, consistent with those of the conventional formalism. Note that the single-source format Iη¯(x)ψ(x)+Iψ¯(x)η(x)\left\langle I\bar{\eta}(x)\psi(x)+I\bar{\psi}(x)\eta(x)\right\rangle is employed here. Alternatively, we can adopt the bilocal-source format η¯(x)ψ(x)η(y)ψ¯(y)\left\langle\bar{\eta}(x)\psi(x)\right\rangle\left\langle\eta(y)\bar{\psi}(y)\right\rangle [31] which is well-suited for the non-perturbative approximations analogous to the two-particle irreducible (2PI) effective action approach [118].

One feature of the Clifford functional integral formalism is that we don’t need to literally perform the functional integration for most cases. Rather, we resort to the property that the functional integration of a total functional derivative is zero

𝒟ψδδψ(x)e12d4x{i[ψ]+Iη¯(x)ψ(x)+Iψ¯(x)η(x)}\displaystyle\int\mathcal{D}\psi\frac{\delta}{\delta\psi(x)}e^{\frac{1}{2}\int d^{4}x\{i\mathcal{L}[\psi]+\left\langle I\bar{\eta}(x)\psi(x)+I\bar{\psi}(x)\eta(x)\right\rangle\}} =0.\displaystyle=0. (177)

Similar property holds for ψ¯(x)\bar{\psi}(x). It means that the functional integral is invariant under a shift of ψ(x)\psi(x).

In our earlier paper on the Clifford functional integral formalism [31], we have provided the specific definition of the Clifford functional derivatives δ/δψ(x){\delta}/{\delta\psi(x)} and δ/δψ¯(x){\delta}/{\delta\bar{\psi}(x)}. For our purpose here, we only need to know the basic Leibniz rule

δδψ(x)ψ(y)F[ψ]\displaystyle\frac{\delta}{\delta\psi(x)}\left\langle\psi(y)F[\psi]\right\rangle =δ(xy)F[ψ]+δδψ(x)ψ(y)F˙[ψ],\displaystyle=\delta(x-y)F[\psi]+\frac{\delta}{\delta\psi(x)}\left\langle\psi(y)\dot{F}[\psi]\right\rangle,

where the dot on F˙[ψ]\dot{F}[\psi] denotes functional derivative performed on F[ψ]F[\psi] only. Similar Leibniz rules can be applied to ψ¯(x)\bar{\psi}(x), η(x)\eta(x) and η¯(x)\bar{\eta}(x). The Leibniz rules, coupled with the other two Clifford algebra properties (114), enable us to perform the relevant Clifford functional derivatives in this paper.

As an exercise, let’s apply the property  (177) to the fermion Lagrangian (141) absent the electromagnetic coupling. We arrive at the Clifford functional-differential version of the Schwinger-Dyson (SD) equation

γμμ{δδη¯(x)Z[η]I}mδδη¯(x)Z[η]+η(x)IZ[η]=0.\displaystyle\gamma^{\mu}{\partial}_{\mu}\{\frac{\delta}{\delta\bar{\eta}(x)}Z[\eta]I\}-m\frac{\delta}{\delta\bar{\eta}(x)}Z[\eta]+\eta(x)IZ[\eta]=0. (178)

The solution to the SD equation can be readily obtained as

Z[η]=e12d4p(2π)4Iη¯(p)S(p)η(p),\displaystyle Z[\eta]=e^{-\frac{1}{2}\int\frac{d^{4}p}{(2\pi)^{4}}\left\langle I\bar{\eta}(p)S(p)\eta(p)\right\rangle}, (179)

where η(p)=d4xη(x)eIpx\eta(p)=\int d^{4}x\eta(x)e^{Ip\cdot x} and px=pμxμp\cdot x=p_{\mu}x^{\mu}. Note that the “Fourier transformation” of η(x)\eta(x) is in terms of eIpxe^{Ip\cdot x} rather than eipxe^{ip\cdot x}. Hence η(x)eIpxeIpxη(x)\eta(x)e^{Ip\cdot x}\neq e^{Ip\cdot x}\eta(x), since Clifford-odd part of η(x)\eta(x) anticommutes with pseudoscalar II. The Feynman propagator S(p)S(p) is given by

S(p)=1m+iϵ,\displaystyle S(p)=\frac{1}{\not{p}-m+{i}\epsilon}, (180)

where =pμγμ\not{p}=p_{\mu}\gamma^{\mu}.

A few comments are in order. First of all, the imaginary number ii does not explicitly show up in the DS equation (178). It is because the ii in the Clifford functional integral (176) and the ii in the fermion Lagrangian (141) cancel out. When gauge fields are included in the Lagrangian, there is no such cancellation due to the absence of ii in the Yang-Mills-type Lagrangian terms.

Secondly, the Feynman propagator S(p)S(p) has poles at p2=m2p^{2}=m^{2}. The propagator is not properly defined without a prescription on the p0p_{0}-related integral in the vicinity of the poles. A well-defined Lorentz-invariant Feynman propagator hinges on the contour integral on the p0p_{0} complex plane prescribed by iϵi\epsilon. As will be shown later in this paper, Feynman’s iϵi\epsilon trick has profound implications for quantum condensations and quantum loop integrals, ultimately contributing to the mysterious appearance of the quantum imaginary number ii in the classical fermion Lagrangians (89) and (141).

In the subsequent subsections, the Feynman propagator will be used extensively in various calculations of quantum loop effects. For the sake of brevity, going forward we will not explicitly write down iϵi\epsilon in the propagators.

4.2 Composite Higgs and the Higgs mass naturalness problem

The discovery of the 125 GeV Higgs boson [112, 113] has renewed the interest in the possible explanation for the Higgs mass naturalness problem [119, 120, 121], notwithstanding differing views [122, 123] on the merits of naturalness and fine-tuning arguments in particle physics and cosmology.

The 125 GeV Higgs mass is technically unnatural according to ’t Hooft [102], since even if one takes the massless Higgs boson limit, the symmetry of the standard model is not enhanced. The perturbative quantum corrections tend to draw the Higgs mass towards higher scale. This is in contrast to the case of the fermion mass, which is protected by the UA(1)U_{A}(1) global symmetry against possible large quantum corrections.

One way of addressing the Higgs mass naturalness problem is to replace the fundamental Higgs boson with a fermion-antifermion condensation, such as in the technicolor[124, 125, 126] and the (extended) top condensation models [127, 128, 129, 130, 131, 132, 133, 134, 135, 136, 30]. In these models, the Higgs sector is an effective description of the low energy physics represented by the composite Higgs field. The condensation is induced via the dynamical symmetry breaking (DSB) mechanism, which is a profound concept in physics. It is introduced into the relativistic QFT by Nambu and Jona-Lasinio (NJL)[137], inspired by the earlier Bardeen-Cooper-Schriefer (BCS) theory of superconductivity[138].

Motivated by the proximity of top quark mass scale and the electroweak symmetry breaking scale, the top condensation model has been extensively studied. The simplest version of the top condensation model assumes the top quark-antiquark condensation only. With a view toward explaining the fermion mass hierarchies in the context of composite electroweak Higgs bosons, we have proposed the extended top condensation model in our previous work [30]. In addition to the top quark condensation, the extended top condensation model involves the tau neutrino and tau lepton condensations as well. The 3HDM in Section 3.4 is essentially an effective representation of these three condensations.

The top condensation model in its original form is based on the NJL-like four-fermion interactions. For example, the top quark interaction term takes the form

Vtopquark\displaystyle V_{top-quark} gIq¯L3γμqL3It¯RγμtR,\displaystyle\sim g\left\langle I\bar{q}^{3}_{L}\gamma^{\mu}{q}^{3}_{L}I\bar{t}_{R}\gamma_{\mu}{t}_{R}\right\rangle, (181)

where g is the four-fermion coupling constant and qL3=tL+bLq^{3}_{L}=t_{L}+b_{L}. Comparing above with the ϕt\phi_{t} Higgs field Yukawa coupling term (153), one can see that ϕt\phi_{t} is an effective representation of the fermion-antifermion pair

iϕt\displaystyle i\phi_{t} gqL3It¯R,\displaystyle\sim g{q}^{3}_{L}I\bar{t}_{R}, (182)

where the ii multiplier will be explained later in this subsection. With the replacement of the effective Higgs field, the top quark interaction term (181) turns into the top quark Yukawa term

Vtopquark\displaystyle V_{top-quark} iIq¯L3γμϕtγμtRiIq¯L3ϕ~ttR,\displaystyle\sim i\left\langle I\bar{q}^{3}_{L}\gamma^{\mu}\phi_{t}\gamma_{\mu}{t}_{R}\right\rangle\sim i\left\langle I\bar{q}^{3}_{L}\tilde{\phi}_{t}{t}_{R}\right\rangle, (183)

Now let’s investigate what kind of Clifford algebraic value the effective Higgs field ϕt\phi_{t} can take. First of all, ϕt\phi_{t} is Clifford-even, given that qL3{q}^{3}_{L} is Clifford-odd and tR{t}_{R} is Clifford-even (meaning that t¯R=tRγ0\bar{t}_{R}={t}_{R}^{\dagger}\gamma_{0} is Clifford-odd). And since tR=PtR{t}_{R}=P_{-}{t}_{R} (meaning that t¯R=(Pt)Rγ0=t¯RP+\bar{t}_{R}={(P_{-}t)}^{\dagger}_{R}\gamma_{0}=\bar{t}_{R}P_{+}), ϕt=ϕtP+\phi_{t}=\phi_{t}P_{+} should be the ϕ+\phi_{+}-type Higgs field. Therefore, there are 32/2=1632/2=16 components which correspond to the combination of the 4-component ϕ+\phi_{+}-type scalar Higgs field (130) and the 12-component ϕAT+\phi_{AT+}-type antisymmetric-tensor Higgs field (144).

For a free fermion, it’s straightforward to obtain the solution (179) to the SD equation (178). In the presence of interactions such as (181), solving the corresponding SD equation is notoriously hard. The path well-trodden is to find a perturbative solution, under the assumption that a certain coupling constant is small. In our previous paper [31], we follow a non-perturbative scheme dubbed as the bilocal-source approximation [139, 140], which effectively treats the bilocal-source term as a series expansion parameter. The zeroth-order approximation of the Clifford functional SD equation [31] is equivalent to the self-consistent Hartree mean-field approximation (a.k.a. rainbow approximation). According to the DSB mechanism, when the four-fermion interaction (181) is strong enough, it will trigger a quantum condensation

iυt\displaystyle i\upsilon_{t} gd4p(2π)4mp2m2,\displaystyle\sim g\int\frac{d^{4}p}{(2\pi)^{4}}\frac{m}{p^{2}-m^{2}}, (184)

where υt\upsilon_{t} is the magnitude of the condensation and mm is the emergent top quark mass.

We can see that the above integral is quadratically divergent. The integral is seemingly a real number. However, as we mentioned in Section 4.1, the fermion propagator has poles at p2=m2p^{2}=m^{2}. Feynman’s iϵi\epsilon trick ensures that the integral on p0p_{0} is well-defined. The proper contour integral on the complex plane of p0p_{0} (or equivalently the Wick rotation of time axis) would pick up an imaginary number ii, thus making the quadratically divergent Feynman integral (184) imaginary valued. Therefore, even if there is no ii in the original four-fermion interaction (181), the imaginary number shows up explicitly in effective Higgs field definition (182) and in the Higgs Yukawa coupling term (183).

It is well know that the calculations of QFT are plagued by divergent Feynman integrals, which need to be regularized at the intermediate stage. After renormalization, a finite and regularization scheme-independent result can be obtained for the renormalizable theories. The top condensation model’s four-fermion interaction is nonrenormalizable in the conventional sense, since the four-fermion interaction is a dimension six operator. That said, as mentioned earlier, we subscribe to the general notion of effective field theory [82, 83], according to which the seemingly nonrenormalizable models, including a viable quantum theory of gravity [141, 142, 143], are nonetheless manageable renormalization-wise and predictive quantum effect-wise, insofar as there is a separation of low energy physics from the high energy quantum perturbations.

Historically the NJL model has been presented with the energy cutoff schemes [144], which usually break the Lorentz invariance. In the presence of a cutoff scale, the four-fermion interaction coupling constant has to be fine-tuned in order to establish the hierarchy between the putative large cutoff scale and the much smaller fermion mass scale. Thus the naturalness problem seems to haunt us again in the Lorentz symmetry-violating cutoff approach.

On the other hand, there is a Lorentz symmetry-preserving implicit regularization framework [145, 146, 147] (IR) wherein the divergent parts of Feynman integrals could be isolated in a few Lorentz-invariant primitive integrals that are independent of the external momentum, whereas the remaining external momentum-dependent integrals are convergent. Because the convergent integrals are separated from the divergent ones, the finite parts can be integrated free from the effects of regularization.

In our earlier paper [31], we applied the IR technique to the NJL-type model. Granted that the divergent primitive integrals are independent of the external momentum, they can be treated as finite quantities as a result of unspecified (implicit) regularization. The central tenet of the IR approach is that no attempt whatsoever shall be made to calculate these divergent primitive integrals via explicit regularization. The external momentum-independent divergent primitive integrals are regarded as free parameters of the model that shall be determined by comparing with measurable quantities, such as the emergent fermion mass, the composite boson mass, and the vacuum energy.

Given that explicit regularization is eschewed in the calculation, the traditional notion of a cutoff scale and a fine-tuned coupling constant are of no relevance in the IR approach. Instead, the smallness of the symmetry breaking scale of the fermion mass mm is an a priori assumption. Once a small scale of mm is assumed at the lower order of approximation, it’s ensured that the smallness of mm is preserved against possible higher order disturbances due to the protection from the weakly broken axial UA(1)U_{A}(1) symmetry, which is in accordance with the technical naturalness principle.

Before proceeding with examining the bosonic bound state properties of the composite Higgs model, we would like to mention some open questions. One question is how to properly calculate the vacuum energy shift due to the quantum condensation. And the other is the long-standing issue of the momentum routing ambiguity associated with the fermion bubble diagram [148]. With the goal of tackling these issues, we propose an improved version of the IR methodology by adding two supplementary rules below [31].

Supplementary rule No. 1: The original IR approach sets forth the rule that if an external momentum-independent primitive divergent Feynman integral AA such as Eq. (184) is isolated, at the final stage of calculation it should be replaced with a finite renormalized value <A>R<A>_{R} so that it can be compared with the measurable quantities. We denote this renormalization procedure (R procedure) as

A<A>R.\displaystyle A\quad\rightarrow\quad<A>_{R}. (185)

Rule No. 1 stipulates that if divergent Feynman integrals AA and BB are related to the same physical process, then

<AB>R<A>R<B>R.\displaystyle<AB>_{R}\neq<A>_{R}<B>_{R}. (186)

In other words, the relationship involving the multiplication of divergent Feynman integrals such as <AB>R=<A>R<B>R<AB>_{R}=<A>_{R}<B>_{R} shall be avoided if AA and BB are related to the same physical process. The value of <AB>R<AB>_{R} should be treated as independent of <A>R<A>_{R} or <B>R<B>_{R}. On the other hand, the R procedure is allowed to be applied recursively to the multiplication of two primitive divergent Feynman integrals if AA and BB are linked to independent physical processes, such as two independent condensations.

Supplementary rule No. 2: When a Feynman integral is convergent or logarithmically divergent, the integral is independent of the momentum routing parameter, because the parameter can be shifted away by a translation of the integration variable. When it comes to integrals that are more than logarithmically divergent, one should proceed with caution. For example, the quadratically divergent Feynman integral corresponding to the fermion bubble diagram [137, 148] in the scalar (Higgs boson) channel is

Πs(q)\displaystyle\Pi_{s}(q) =id4p(2π)4S(p+(1α)q)S(pαq),\displaystyle=i\int\frac{d^{4}p}{(2\pi)^{4}}\left\langle S(p+(1-\alpha)q)S(p-\alpha q)\right\rangle, (187)

where SS is the fermion propagator and α\alpha is an arbitrary parameter controlling the momentum shifting [148]. Unlike the case of convergent or logarithmically divergent Feynman integrals, the seemingly innocuous momentum shifting changes the integral values. Rule No. 2 stipulates that for the quadratically (or higher order) divergent Feynman integrals with momentum routing ambiguities, the momentum routing parameter α\alpha shall be set at the symmetrical value. For the above instance, the momentum routing parameter should be set at α=12\alpha=\frac{1}{2}, so that (1α)q=αq(1-\alpha)q=\alpha q is symmetrical. Note that a related ambiguity problem is the triangle diagrams of the Adler-Bell-Jackiw (ABJ) anomaly [149, 150], where the integrals are linearly divergent. This ambiguity is fixed by enforcing the vector Ward identity, at the expense of the axial Ward identity.

With these two supplementary rules specified, let’s investigate the bosonic bound state properties of the composite Higgs model. To this end, we go beyond the zeroth-order bilocal-source approximation and turn to the first-order approximation of the Clifford functional SD equation [31]. The collective mode of the composite Higgs boson can be determined via the pole of the composite boson propagator (a.k.a. the fermion-antifermion channel T-matrix) in the scalar channel

Ds(p)\displaystyle D_{s}(p) 1g1Πs(p),\displaystyle\sim\frac{1}{g^{-1}-\Pi_{s}(p)}, (188)

where Πs(p)\Pi_{s}(p) is the bubble function (187). The composite boson propagators Ds(p)D_{s}(p) is the re-summation of the infinite order chain of the fermion bubble diagrams. Similar leading order calculation in the context of contact interactions goes by various names, such as the random-phase approximation, ladder approximation, Bethe-Salpeter T-matrix equation, and 1/N expansion.

After setting the momentum routing parameter in Eq. (187) to α=12\alpha=\frac{1}{2}, the pole (i.e. the Higgs boson mass) of the composite boson propagator Ds(p)D_{s}(p) can be calculated as [31]

mh\displaystyle m_{h} =21+|Δ|m,\displaystyle=\frac{2}{\sqrt{1+|\Delta|}}m, (189)

where mm is the dynamically generated fermion mass and Δ\Delta is defined by the renormalized logarithmically divergent Feynman integral

Δ1=64π2<d4p(2π)41(p2m2)2>R.\displaystyle\Delta^{-1}=64\pi^{2}<\int\frac{d^{4}p}{(2\pi)^{4}}\frac{1}{(p^{2}-m^{2})^{2}}>_{R}. (190)

Because of the 1+|Δ|\sqrt{1+|\Delta|} factor, the composite Higgs boson mass mhm_{h} is less than 2m2m, which deviates from the typical first-order approximation prediction mh=2mm_{h}=2m [137]. In other words, 2m2m serves as an upper bound of the Higgs boson mass, which implies that the Higgs boson mass is also protected by the weakly broken axial symmetry, given that the Higgs boson mass and the fermion mass are simultaneously generated by the same DSB mechanism. And additionally, at the electroweak scale there is no elementary Higgs mass term to be modified by any higher order quantum perturbation from external sources. Therefore, the composite Higgs mass is naturally small.

Historically, when it comes to the top quark condensation model, one phenomenological problem is related to the prediction of the Higgs-top mass ratio. Since the 2012 discovery [112, 113], the Higgs boson is known to be lighter than the top quark. According to the traditional way of Higgs mass calculation, the top condensation model appears to fail since it gives too heavy Higgs mass compared with the top quark mass. However, in our calculation the Higgs mass and the top mass relation involves an extra primitive divergent Feynman integral (190). According to the central rule of the IR approach, the value of such integral should not be explicitly calculated. Rather, it is determined by the experimental measurements. Therefore, the observed Higgs-top mass ratio does not falsify the top condensation model. Instead, the ratio fixes the dimensionless parameter |Δ||\Delta| of the model. Based on the measured top quark mass (173173Gev) and Higgs mass (125125Gev), we arrive at an estimation of |Δ|=6.66|\Delta|=6.66 from Eq. (189).

In the same vein as the composite electroweak Higgs field, the Majorana-Higgs field ϕM\phi_{M} can be regarded as a composite field representing the condensation of a right-handed neutrino-antineutrino pair [30]

iϕMIν¯R(IΓ2Γ3)νR.\displaystyle i\phi_{M}\sim I\bar{\nu}_{R}(I\Gamma_{2}\Gamma_{3}){\nu}_{R}. (191)

Similarly, the Φ\Phi singlets can be linked to the condensation of fermion-antifermion double pairs [30] such as

Φαt\displaystyle\Phi_{\alpha t} b¯RtRq¯L3qL3,\displaystyle\sim\bar{b}_{R}{t}_{R}\bar{q}^{3}_{L}{q}^{3}_{L}, (192)
Φβt\displaystyle\Phi_{\beta t} l¯L1γμqL3t¯RγμνeR.\displaystyle\sim\bar{l}^{1}_{L}\gamma^{\mu}{q}^{3}_{L}\bar{{t}}_{R}\gamma_{\mu}\nu_{eR}. (193)

The quantum condensation details of the ϕM\phi_{M} and Φ\Phi composite fields can be worked out along the lines of the aforementioned composite electroweak Higgs field. Note that there is no imaginary number ii in the definition of the effective Φ\Phi field, since even numbers of ii (two fermion-antifermion pairs) cancel out.

In summary, the Higgs mass could be naturally small and we have demystified the imaginary number ii in the Yukawa/mass term as a vestige of the quantum condensation. Emboldened by these achievements, one might wonder whether we can also surmount the naturalness problem of vacuum energy and decipher the origin of the imaginary number ii in the fermion kinetic Lagrangian term. That is the subject of the next subsection.

4.3 Composite vierbein and the cosmological constant problem

Quantum fluctuations of the vacuum contribute to the cosmological constant Λ\Lambda. The calculated vacuum energy is extremely large compared with the commonly accepted estimation of Λ\Lambda [151, 152, 153, 154]. The vacuum energy is 1012010^{120} times too large according to the zero-point energy calculation, or 105510^{55} times too large according to the electroweak symmetry breaking calculation. The cosmological constant problem is perceived as the most severe naturalness problem in physics [155, 156, 157].

Inspired by the composite Higgs model investigated in Section 4.2, we turn to the composite vierbein field [158, 159, 160, 161, 162, 163, 164] as a possible solution to the cosmological constant problem. Paralleling the dynamical symmetry breaking (DSB) mechanism of the composite Higgs approach, the vierbein field e^{\hat{e}} can be considered as an effective representation of the the standard model fermion-antifermion condensation

ie^\displaystyle i{\hat{e}} E=ψdψ¯,\displaystyle\sim E=\psi d\bar{\psi}, (194)

where dd is the exterior derivative, hence Eμ=ψμψ¯E_{\mu}=\psi\partial_{\mu}\bar{\psi}. Consequently, quantum gravity is realized indirectly via the quantized the standard model spinor field which underlies the composite vierbein field.

Unlike the previous composite vierbein approaches, the Clifford-valued composite vierbein field above is not restricted to the vector space γa\gamma_{a}, albeit its VEV will congeal around γa\gamma_{a}. This is analogous to the Higgs mechanism where the Higgs VEV settles around the subspace ϕ0P+\phi_{0}P_{+} out of the full Higgs doublet space of (ϕ0+ϕ1Γ2Γ3+ϕ2Γ3Γ1+ϕ3Γ1Γ2)P+(\phi_{0}+\phi_{1}\Gamma_{2}\Gamma_{3}+\phi_{2}\Gamma_{3}\Gamma_{1}+\phi_{3}\Gamma_{1}\Gamma_{2})P_{+}. We will delve into more details about the extended vierbein space in Section 4.4, where a more accurate definition of the chiral composite vierbein fields will be provided when we examine the gauge-covariant chiral vierbeins.

The composite vierbein field is to be compared with a generalized version of the composite Higgs field

iϕ\displaystyle i\phi H=ψIψ¯.\displaystyle\sim H=\psi I\bar{\psi}. (195)

For simplicity reasons, we consider a generic spinor field ψ\psi with both chirality and ignore gauge field coupling.

There are a couple of similarities and dissimilarities between the spinor bilinears HH and EE. Given that there is no \left\langle\ldots\right\rangle operation in the definition of HH and EE, both HH and EE are allowed to take values in the general Clifford algebraic space. The Higgs spinor bilinear HH is a 0-form, whereas the vierbein spinor bilinear E=EμdxμE=E_{\mu}dx^{\mu} is a 1-form which conforms with fact that the vierbein field e^\hat{e} is a 1-form. The Higgs spinor bilinear HH acquires a Clifford-even VEV, which implies that the Higgs field ϕ\phi describes the condensation of an opposite-handed fermion-antifermion pair (ψLIψ¯R\psi_{L}I\bar{\psi}_{R} or ψRIψ¯L\psi_{R}I\bar{\psi}_{L}). On the other hand, the vierbein spinor bilinear EE acquires Clifford-odd VEVs valued in {γa\gamma_{a}}, which suggests that the vierbein field e^\hat{e} describes the condensation of a like-handed fermion-antifermion pair (ψLdψ¯L\psi_{L}d\bar{\psi}_{L} or ψRdψ¯R\psi_{R}d\bar{\psi}_{R}).

In the above HH and EE definitions, we follow the tradition [27, 165] of regarding the spinor field ψ\psi as dimensionless, a.k.a. bare spinor field. Consequently, the Higgs spinor bilinear HH is also dimensionless. The vierbein spinor bilinear Eμ=ψμψ¯E_{\mu}=\psi\partial_{\mu}\bar{\psi} is endowed with mass dimension one from the partial derivative. As such, a proper differential form would remain dimensionless. For the example of E=EμdxμE=E_{\mu}dx^{\mu}, the mass dimension one of EμE_{\mu} is canceled out by the mass dimension minus one of dxμdx^{\mu}. The same logic applies to any 1-form gauge field (such as A^=A^μdxμ\hat{A}=\hat{A}_{\mu}dx^{\mu}), provided that A^μ\hat{A}_{\mu} is assigned mass dimension one. If we construct a Lagrangian term using the proper differential forms, the mass dimension assignment convention implies that the coefficient in front of the Lagrangian term should be of mass dimension zero. The conventional Lagrangian parameter mass dimensions can be recovered when we re-scale the bare spinor field which will be discussed later in this subsection.

Leveraging these spinor bilinears EE and HH, we can write down the diffeomorphism-invariant Lagrangian terms of the pre-condensation primordial world
Fermion+CC\displaystyle\mathcal{L}_{Fermion+CC} IEEEE,\displaystyle\sim\left\langle IE\wedge E\wedge E\wedge E\right\rangle, (196a)
Yukawa+CC\displaystyle\mathcal{L}_{Yukawa+CC} IEEEEH2,\displaystyle\sim\left\langle IE\wedge E\wedge E\wedge EH^{2}\right\rangle, (196b)
YangMills\displaystyle\mathcal{L}_{Yang-Mills} (IEEF^)(IEEF^)IEEEE,\displaystyle\sim\frac{\left\langle(IE\wedge E\wedge\hat{F})(IE\wedge E\wedge\hat{F})\right\rangle}{\left\langle IE\wedge E\wedge E\wedge E\right\rangle}, (196c)
Gravity\displaystyle\mathcal{L}_{Gravity} IEER^,\displaystyle\sim\left\langle IE\wedge E\wedge\hat{R}\right\rangle, (196d)

where F^\hat{F} stands for any Yang-Mills-type gauge field curvature 22-form and R^\hat{R} is the spin connection curvature 22-form (82). Note that Yukawa+CC\mathcal{L}_{Yukawa+CC} could have some variations, such as IEEEHEH\left\langle IE\wedge E\wedge E\wedge HEH\right\rangle which corresponds to the top quark-type Yukawa interaction term (181).

Diffeomorphism-invariance is guaranteed since all the Lagrangian terms are 4-forms on the 4-dimensional space-time manifold. As mentioned earlier, the coefficients in front of the Lagrangian terms (for brevity sake not explicitly written out) are all of mass dimension zero. And we further assume that these dimensionless coefficients should be of order O(1)O(1). In other words, there shouldn’t be any unnaturally small or large coefficients.

It’s worth mentioning that there are even numbers of fermion-antifermion pairs in each Lagrangian term. It’s mandated by the two imperatives: The pre-condensation Lagrangian shall be real and there shall be no explicit imaginary number ii in the Lagrangian. Note that a bare cosmological constant term is not allowed, since diffeomorphism-invariance demands that the Lagrangian terms must be 4-forms and the available gauge-covariant differential forms are either the fermion field-related EE spinor bilinear 1-form or the gauge field-related curvature 2-forms.

The fermion Fermion+CC\mathcal{L}_{Fermion+CC} and the Yukawa Yukawa+CC\mathcal{L}_{Yukawa+CC} Lagrangian terms are comprised of 8 and 12 Grassmann-odd fermion fields respectively. This is very different from the typical fermion Lagrangian. Upon quantum condensation, they will give rise to the conventional fermion kinetic and mass terms as well as the effective cosmological constant term. More specifically, when the three EE spinor bilinears in Fermion+CC\mathcal{L}_{Fermion+CC} are replaced by their condensation values, the Lagrangian term Fermion+CC\mathcal{L}_{Fermion+CC} is left with one EE spinor bilinear and is turned into the effective fermion kinetic term. Similarly, when the four EE spinor bilinears and one HH spinor bilinear in Yukawa+CC\mathcal{L}_{Yukawa+CC} are replaced by their condensation values, the Lagrangian term Yukawa+CC\mathcal{L}_{Yukawa+CC} is left with one HH spinor bilinear and is turned into the effective Dirac mass term. Lastly, when all spinor bilinears in Fermion+CC\mathcal{L}_{Fermion+CC} and Yukawa+CC\mathcal{L}_{Yukawa+CC} are replaced by their condensation values, these two Lagrangian terms are left with no spinor bilinear and are turned into the effective cosmological constant term.

Upon DSB-generated quantum condensation, the diffeomorphism-invariance is broken and the effective fermion propagator S(p)S(p) assumes the flat space-time form

S(p)=a0m0,\displaystyle S(p)=\frac{a_{0}}{\not{p}-m_{0}}, (197)

where the emergent mass m0m_{0} arises from the Yukawa+CC\mathcal{L}_{Yukawa+CC} term, and the parameter a0a_{0} comes from the Fermion+CC\mathcal{L}_{Fermion+CC} term. The parameter a01a_{0}^{-1} is of mass dimension three, since it’s related to the condensations of three mass dimension-one EμE_{\mu} spinor bilinears. The parameters a0a_{0} and m0m_{0} can be determined self-consistently via their respective mean-field “gap” equations in a similar fashion as the NJL-type model [137, 31].

Leveraging the Clifford generating functional Z[η]Z[\eta] (Eq. (179)), the mean-field VEVs of EμE_{\mu} and HH can be calculated as

EμiM0γμ=a0γμd4p(2π)4p2p2m02,\displaystyle E_{\mu}\sim iM_{0}\gamma_{\mu}=a_{0}\gamma_{\mu}\int\frac{d^{4}p}{(2\pi)^{4}}\frac{p^{2}}{p^{2}-m_{0}^{2}}, (198a)
Hiυ0=a0d4p(2π)4m0p2m02,\displaystyle H\sim i\upsilon_{0}=a_{0}\int\frac{d^{4}p}{(2\pi)^{4}}\frac{m_{0}}{p^{2}-m_{0}^{2}}, (198b)

where the VEV magnitudes M0M_{0} and υ0\upsilon_{0} are of mass dimension one and zero, respectively. The VEV of HH takes value in the Clifford-scalar space, while the VEV of EμE_{\mu} takes value in the Clifford-vector space {γμ\gamma_{\mu}} as expected for an effective vierbein field. We can see that the above primitive quantum loop integrals for EμE_{\mu} and HH are quartically and quadratically divergent, respectively. According to the contour integral rule on the complex plane of p0p_{0}, these integrals pick up an imaginary number ii factor. The VEV magnitudes M0M_{0} and υ0\upsilon_{0} are subject to the renormalization procedure <>R<\cdots>_{R} as delineated in Section 4.2.

As we know, EμE_{\mu} is of mass dimension one. To be consistent with the conventional formalism of the dimensionless vierbein, the correspondence between the spinor bilinear EμE_{\mu} and the dimensionless vierbein e^μ\hat{e}_{\mu} should be

EμiM0e^μ,\displaystyle E_{\mu}\sim iM_{0}\hat{e}_{\mu}, (199)

which means e^μ=γμ\hat{e}_{\mu}=\gamma_{\mu} according to (198a), as expected for the flat space-time. The above calculation of VEVs are based on the flat space-time fermion propagator S(p)S(p) (197). In the following discussion, we will assume that the assignment of EμiM0e^μE_{\mu}\sim iM_{0}\hat{e}_{\mu} is applicable for the general cases of curved space-time as well.

After replacing the condensated EμE_{\mu} and HH with iM0e^μiM_{0}\hat{e}_{\mu} and iυ0i\upsilon_{0} respectively and retaining the lowest order terms in the non-condensated EE and HH, the effective Lagrangian terms take the form
FermionKinetic\displaystyle\mathcal{L}_{Fermion-Kinetic} i<M03>RIe^e^e^E,\displaystyle\sim i<M_{0}^{3}>_{R}\;\;\left\langle I\hat{e}\wedge\hat{e}\wedge\hat{e}\wedge E\right\rangle, (200a)
FermionMass\displaystyle\mathcal{L}_{Fermion-Mass} i<M04υ0>RIe^e^e^e^H,\displaystyle\sim i<M_{0}^{4}\upsilon_{0}>_{R}\;\;\left\langle I\hat{e}\wedge\hat{e}\wedge\hat{e}\wedge\hat{e}H\right\rangle, (200b)
YangMills\displaystyle\mathcal{L}_{Yang-Mills} <M04>R<M04>R(Ie^e^F^)(Ie^e^F^)Ie^e^e^e^,\displaystyle\sim\frac{<M_{0}^{4}>_{R}}{<M_{0}^{4}>_{R}}\;\;\frac{\left\langle(I\hat{e}\wedge\hat{e}\wedge\hat{F})(I\hat{e}\wedge\hat{e}\wedge\hat{F})\right\rangle}{\left\langle I\hat{e}\wedge\hat{e}\wedge\hat{e}\wedge\hat{e}\right\rangle}, (200c)
Gravity\displaystyle\mathcal{L}_{Gravity} <M02>RIe^e^R^,\displaystyle\sim<M_{0}^{2}>_{R}\;\;\left\langle I\hat{e}\wedge\hat{e}\wedge\hat{R}\right\rangle, (200d)
CCFermion\displaystyle\mathcal{L}_{CC-Fermion} <M04>RIe^e^e^e^,\displaystyle\sim<M_{0}^{4}>_{R}\;\;\left\langle I\hat{e}\wedge\hat{e}\wedge\hat{e}\wedge\hat{e}\right\rangle, (200e)
CCYukawa\displaystyle\mathcal{L}_{CC-Yukawa} <M04υ02>RIe^e^e^e^,\displaystyle\sim<M_{0}^{4}\upsilon_{0}^{2}>_{R}\;\;\left\langle I\hat{e}\wedge\hat{e}\wedge\hat{e}\wedge\hat{e}\right\rangle, (200f)
where the FermionKinetic\mathcal{L}_{Fermion-Kinetic} and CCFermion\mathcal{L}_{CC-Fermion} terms are derived from Fermion+CC\mathcal{L}_{Fermion+CC}, while the FermionMass\mathcal{L}_{Fermion-Mass} and CCYukawa\mathcal{L}_{CC-Yukawa} terms are derived from Yukawa+CC\mathcal{L}_{Yukawa+CC}.

Now we can trace the origin of the imaginary number ii in the “classical” Lagrangian terms. The imaginary number ii stems from the primitive divergent integrals (198) related to the quantum condensations of the EμE_{\mu} and HH spinor bilinears. If there are odd number of condensations (or equivalently odd number of quantum loop integrals), there is an ii in the coefficient of the effective “classical” Lagrangian, such as the fermion kinetic (200a) and mass (200b) terms. On the other hand, if there are even number of condensations (or equivalently even number of quantum loop integrals), there is no ii in the coefficient of the effective “classical” Lagrangian since ii squares to 1-1, such as the Yang-Mills (200c), gravity (200d), and cosmological constant (200e) (200f) terms.

We can verify that the fermion kinetic (200a) and mass (200b) terms conform with the corresponding terms specified in the Lagrangian of the world in Section 2.4 (see Eq. (89) and (92)). The only difference is in the coefficients, given that we have adopted the dimensionless bare spinor field in this subsection. To map to the traditional mass dimension 3/23/2 spinor field (a.k.a. dressed spinor field) in Section 2.4, we can leverage the field renormalization relationship

ψdressed=<M03>Rψbare,\displaystyle\psi_{dressed}=\sqrt{<M_{0}^{3}>_{R}}\;\;\psi_{bare}, (201)

where ψbare\psi_{bare} stands for the dimensionless bare spinor field and ψdressed\psi_{dressed} stands for the mass dimension 3/23/2 dressed spinor field. With the substitution of ψbare\psi_{bare} with ψdressed\psi_{dressed}, we can see that the fermion kinetic term (200a) regains the conventional form (89) with the coefficient normalized to one. The same substitution in the fermion mass (200b) term implies that the fermion mass for the dressed spinor field is

m0<M04υ0>R<M03>R.\displaystyle m_{0}\sim\frac{<M_{0}^{4}\upsilon_{0}>_{R}}{<M_{0}^{3}>_{R}}. (202)

For the effective Yang-Mills-type Lagrangian (200c), the <M04>R<M_{0}^{4}>_{R} factors from the numerator and the denominator cancel out. As we mentioned earlier, the dimensionless coefficient in front of the original Yang-Mills-type Lagrangian term (196c) is assumed to be of order O(1)O(1). Therefore we expect that the effective Yang-Mills-type coupling constants should not be far from being of order O(1)O(1) as well. As a verification, the QED’s fine-structure constant is α1/137\alpha\approx 1/137, which meets our expectation.

For the effective gravity Lagrangian (200d), the coefficient <M02>R<M_{0}^{2}>_{R} is of mass dimension two and can be identified with the Planck mass MplM_{\mathrm{pl}}

<M02>RMpl2.\displaystyle<M_{0}^{2}>_{R}\;\approx\;M_{\mathrm{pl}}^{2}. (203)

The effective cosmological constant Λ\Lambda is of mass-dimension two. It is defined by the ratio between the CCFermion\mathcal{L}_{CC-Fermion}/CCYukawa\mathcal{L}_{CC-Yukawa} and Gravity\mathcal{L}_{Gravity} Lagrangian coefficients

Λ<M04>R+<M04υ02>R<M02>R<M04>R+<M04υ02>RMpl2,\displaystyle\Lambda\sim\frac{<M_{0}^{4}>_{R}+<M_{0}^{4}\upsilon_{0}^{2}>_{R}}{<M_{0}^{2}>_{R}}\approx\;\frac{<M_{0}^{4}>_{R}+<M_{0}^{4}\upsilon_{0}^{2}>_{R}}{M_{\mathrm{pl}}^{2}}, (204)

where <M04>R<M_{0}^{4}>_{R} is the vacuum energy contribution from the fermion Lagrangian, and <M04υ02>R<M_{0}^{4}\upsilon_{0}^{2}>_{R} is the Higgs ground state energy contribution from the Yukawa Lagrangian.

According to the conventional wisdom, each M0M_{0} factor in the above equations can be identified with the Planck mass MplM_{\mathrm{pl}}. Resultantly, the effective fermion mass m0m_{0} (202) is estimated as

m0υ0Mpl.\displaystyle m_{0}\sim\upsilon_{0}M_{\mathrm{pl}}. (205)

Using the top quark mass as an example, υ0\upsilon_{0} is calculated as of order υ01017\upsilon_{0}\approx 10^{-17}. Similarly, Λ\Lambda is estimated as of order

Λ(1+υ02)Mpl2Mpl2,\displaystyle\Lambda\sim(1+\upsilon_{0}^{2})M_{\mathrm{pl}}^{2}\approx M_{\mathrm{pl}}^{2}, (206)

which is astronomically larger than the commonly accepted estimation of Λ10120Mpl2\Lambda\sim 10^{-120}M_{\mathrm{pl}}^{2}.

However, there is a loophole in the above reasoning. According to the supplementary rule No. 1 of the implicit regularization in Section 4.2, the renormalization procedure can not be applied recursively to the multiplication of primitive divergent integrals

<M04>R<M02>R<M02>RMpl4.\displaystyle<M_{0}^{4}>_{R}\;\neq\;<M_{0}^{2}>_{R}\;<M_{0}^{2}>_{R}\;\approx\;M_{\mathrm{pl}}^{4}. (207)

As such, <M04>R<M_{0}^{4}>_{R} should be deemed as a parameter completely decoupled from the scale of Mpl4M_{\mathrm{pl}}^{4}. The magnitudes of these two could differ vastly from each other. By the same token, each of the renormalized primitive divergent integrals <M03>R<M_{0}^{3}>_{R}, <M04υ0>R<M_{0}^{4}\upsilon_{0}>_{R}, and <M04υ02>R<M_{0}^{4}\upsilon_{0}^{2}>_{R} should be regarded as an individual parameter which can only be determined by comparing with measurable results. This means that even though we have seemingly only one divergent Feynman integral M0M_{0}, there could be multiple unrelated scales such as the Planck mass MplM_{\mathrm{pl}} and the cosmological constant Λ\Lambda, in stark contrast to the conventional QFT renormalization procedure (or the Wilsonian renormalization group approach) characterized by a single renormalization scale.

Therefore, Eq. (204) can not be used to predict the size of the cosmological constant. Rather, one should use the measured magnitude of Λ\Lambda to impute that <M04>R+<M04υ02>R10120Mpl4<M_{0}^{4}>_{R}+<M_{0}^{4}\upsilon_{0}^{2}>_{R}\;\sim 10^{-120}M_{\mathrm{pl}}^{4}. Hence the cosmological constant problem can be evaded.

It’s also worth mentioning that there are other contributions to the cosmological constant, such as the Majorana-Higgs-induced phase transitions. In principal, these phase transitions can be treated in a similar way as delineated above.

In the last part of this subsection, we turn our attention to the possible experimental evidences of the composite vierbein. When we write out the effective Lagrangian (200), we only retain the lowest order terms of the non-condensated EE/HH spinor bilinears, under the assumption that the other terms are negligible at low energies. At an elevated energy level, additional terms could become relevant. As an example, let’s examine the fermion Lagrangian term with two non-condensated EE spinor bilinears. Therefore there are four remaining spinor fields in the effective Lagrangian

<M02>R(<M03>R)2γμγνψμψ¯ψνψ¯,\displaystyle\frac{<M_{0}^{2}>_{R}}{(<M_{0}^{3}>_{R})^{2}}\left\langle\gamma^{\mu}\gamma^{\nu}\psi\partial_{\mu}\bar{\psi}\;\psi\partial_{\nu}\bar{\psi}\right\rangle, (208)

where μν\mu\neq\nu and ψ\psi denotes the dressed spinor field with the field renormalization (201). We specifically write down the Lagrangian term in flat space-time to highlight the fact that the partial derivatives μ\partial_{\mu} and ν\partial_{\nu} are orthogonal as opposed to being aligned, which is very different from a typical scalar field Lagrangian that involves two partial derivatives.

The Lagrangian term could be considered as two perpendicular fermion currents interacting with each other. If such an event is detected experimentally, it would be a telltale sign that one of the composite e^\hat{e} fields in the effective fermion kinetic Lagrangian term (200a) is broken down into the underlying fermion fields. In other words, such an event exposes the fermion compositeness of the space-time metric. The coefficient of the above four-fermion term is of mass dimension 4-4. It implies an energy scale

Mcomp((<M03>R)2<M02>R)14(<M03>RMpl)12,\displaystyle M_{comp}\sim\left(\frac{(<M_{0}^{3}>_{R})^{2}}{<M_{0}^{2}>_{R}}\right)^{\frac{1}{4}}\approx\left(\frac{<M_{0}^{3}>_{R}}{M_{\mathrm{pl}}}\right)^{\frac{1}{2}}, (209)

above which the space-time fabric disintegrates into the underlying fermionic components. Note that we have no theoretical recourse to pinpoint the exact compositeness scale McompM_{comp}, since it involves the primitive divergent integral <M03>R<M_{0}^{3}>_{R} which could only be ascertained via empirical means as per the IR tenet. Of particular interest is the fact that the compositeness scale McompM_{comp} is different from the Planck scale MplM_{\mathrm{pl}}. They are two unrelated scales. The compositeness scale is the scale above which there could be measurable evidences of the composite vierbein broken down into the fermionic components, whereas the Planck scale is the scale at which the higher-order gravitational Lagrangian terms become relevant. Therefore, if Mcomp<MplM_{comp}<M_{\mathrm{pl}}, we could have a chance of probing the so-called Planck-scale physics at an energy level below the Planck scale.

4.4 Extended symmetries and gravi-weak interaction

In the case of the composite Higgs fields, we have benefited from various clues guiding us towards the conclusion that there are three specific fermions catalyzing the electroweak symmetry breaking process, namely, the top quark, tau neutrino, and tau lepton condensations [30]. When it comes to the composite vierbeins, due to lack of evidences we are not able to speculate which of the standard model fermions are involved in the vierbein-related condensations. Nonetheless, we can still make progress by investigating the general symmetry properties of the composite vierbeins.

Considering the gauge transformation characteristics of the standard model fermions, we cast the effective vierbeins into three categories

ie^L\displaystyle i{\hat{e}_{L}} EL=ψLDLψL¯,\displaystyle\sim E_{L}=\psi_{L}\overline{D_{L}{\psi_{L}}}, (210)
ie^Ru\displaystyle i{\hat{e}_{Ru}} Eu=ψRuDRψRu¯,\displaystyle\sim E_{u}=\psi_{Ru}\overline{D_{R}{\psi_{Ru}}}, (211)
ie^Rd\displaystyle i{\hat{e}_{Rd}} Ed=ψRdDRψRd¯,\displaystyle\sim E_{d}=\psi_{Rd}\overline{D_{R}{\psi_{Rd}}}, (212)

where DLD_{L} and DRD_{R} are the left-handed and right-handed gauge-covariant derivatives, ψL\psi_{L} is any left-handed doublet such as uL+dLu_{L}+d_{L}, ψRu\psi_{Ru} is any right-handed up-type singlet such as uRu_{R}, and ψRd\psi_{Rd} is any right-handed down-type singlet such as dRd_{R}.

Given the freedom afforded by the above chiral vierbeins unconstrained by the Clifford subspace {γa\gamma_{a}}, the gauge symmetry groups (52) we studied earlier can be expanded to (but still a subset of the enveloping symmetries (44) and (45))

Spin(1,3)L×Spin(1,3)R×Spin(1,3)WL×Spin(1,1)WR×U(1)WR\displaystyle Spin(1,3)_{L}\times Spin(1,3)_{R}\times Spin(1,3)_{WL}\times Spin(1,1)_{WR}\times U(1)_{WR}
×SU(3)C×U(1)BL,\displaystyle\times SU(3)_{C}\times U(1)_{B-L}, (213)

where Spin(1,3)LSpin(1,3)_{L} and Spin(1,3)RSpin(1,3)_{R} are the left-handed and right-handed Lorentz gauge groups respectively. The extended left-handed weak group Spin(1,3)WLSpin(1,3)_{WL} generators are

Γ2Γ3,Γ3Γ1,Γ1Γ2,Γ0Γ1,Γ0Γ2,Γ0Γ3,\displaystyle\Gamma_{2}\Gamma_{3},\;\Gamma_{3}\Gamma_{1},\;\Gamma_{1}\Gamma_{2},\;\Gamma_{0}\Gamma_{1},\;\Gamma_{0}\Gamma_{2},\;\Gamma_{0}\Gamma_{3}, (214)

where Γ0=γ1γ2γ3\Gamma_{0}=\gamma_{1}\gamma_{2}\gamma_{3} and the pseudo-weak portion of the extended right-handed Spin(1,1)WRSpin(1,1)_{WR} group generator is

Γ0Γ3.\displaystyle\Gamma_{0}\Gamma_{3}. (215)

The left-handed and right-handed fermions transform independently under the chiral left-sided gauge transformations Spin(1,3)L×Spin(1,3)WLSpin(1,3)_{L}\times Spin(1,3)_{WL} and Spin(1,3)R×Spin(1,1)WR×U(1)WRSpin(1,3)_{R}\times Spin(1,1)_{WR}\times U(1)_{WR} respectively, whereas the left-handed and right-handed fermions transform in unison under the right-sided gauge transformation SU(3)C×U(1)BLSU(3)_{C}\times U(1)_{B-L}.

Note that the extended left-handed weak group Spin(1,3)WLSpin(1,3)_{WL} comprises the regular weak group SU(2)WLSU(2)_{WL} generated by {ΓiΓj\Gamma_{i}\Gamma_{j}} as well as the weak-boosts generated by {Γ0Γi\Gamma_{0}\Gamma_{i}}. These are the counterparts of the spacial rotations generated by {γiγj\gamma_{i}\gamma_{j}} and the Lorentz boosts generated by {γ0γi\gamma_{0}\gamma_{i}}. The weak-boost is not a group on its own, it’s rather the coset Spin(1,3)WL/SU(2)WLSpin(1,3)_{WL}/SU(2)_{WL}. Given the relationships such as Γ0Γ3=IΓ1Γ2\Gamma_{0}\Gamma_{3}=I\Gamma_{1}\Gamma_{2}, we also call {Γ0Γi\Gamma_{0}\Gamma_{i}} the pseudo-weak generators. Henceforth, we will use the terms weak-boost and pseudo-weak interchangeably. We would like to highlight the fact that both the local Lorentz symmetry and the extended left-handed weak symmetry are Spin(1,3)Spin(1,3), hinting at an interesting duality between Lorentz gravity and weak interactions. Historically, there have been various attempts [166, 167, 168, 169] trying to explore the possible connection between the gravitational and weak interactions.

Given that both the vierbeins and the left-side gauge transformations VV are acting on the left side of a spinor, the left-handed and right-handed vierbeins should transform as vectors (e^Ve^V1\hat{e}\rightarrow V\hat{e}V^{-1}) under the gauge transformations Spin(1,3)L×Spin(1,3)WLSpin(1,3)_{L}\times Spin(1,3)_{WL} and Spin(1,3)R×Spin(1,1)WRSpin(1,3)_{R}\times Spin(1,1)_{WR} respectively to ensure the gauge-invariance of the spinor Lagrangian. Consequently, the left-handed e^L{\hat{e}_{L}} ought to be valued in the extended Clifford algebraic subspace spanned by the 44=164*4=16 multivectors

γa,γaΓ0Γi,\displaystyle\gamma_{a},\quad\gamma_{a}\Gamma_{0}\Gamma_{i}, (216)

where a=0,1,2,3a=0,1,2,3 and i=1,2,3i=1,2,3. The right-handed e^Ru{\hat{e}_{Ru}} is valued in the Clifford algebraic subspace spanned by the 44 multivectors

γaP+,\displaystyle\gamma_{a}P_{+}, (217)

while the right-handed e^Rd{\hat{e}_{Rd}} is valued in the Clifford algebraic subspace spanned by the 44 multivectors

γaP,\displaystyle\gamma_{a}P_{-}, (218)

where P±P_{\pm} are the projection operators (24).

Alternatively, e^L{\hat{e}_{L}} may take values in the complimentary Clifford algebraic subspace spanned by the 44=164*4=16 multivectors

γaI,γaΓiΓj.\displaystyle\gamma_{a}I,\quad\gamma_{a}\Gamma_{i}\Gamma_{j}. (219)

As such, e^L{\hat{e}_{L}} could develop VEVs valued in the pseudo-vector subspace {γaI\gamma_{a}I}, rather than the regular vector subspace {γa\gamma_{a}}. The same logic goes for e^Ru{\hat{e}_{Ru}} and e^Rd{\hat{e}_{Rd}}. Nevertheless, our discussion in this paper is concentrated on the regular vector-type e^L{\hat{e}_{L}}, e^Ru{\hat{e}_{Ru}}, and e^Rd{\hat{e}_{Rd}} vierbeins.

Note that if the left-handed e^L{\hat{e}_{L}} were restricted to the vector space γa\gamma_{a}, it could not accommodate the left-handed weak-boost transformation e^Le12θ0iΓ0Γie^Le12θ0iΓ0Γi\hat{e}_{L}\rightarrow e^{\frac{1}{2}\theta^{0i}\Gamma_{0}\Gamma_{i}}\;\hat{e}_{L}\;e^{-\frac{1}{2}\theta^{0i}\Gamma_{0}\Gamma_{i}}. The left-handed e^L{\hat{e}_{L}} has 164=6416*4=64 individual components eLμa{e}^{a}_{L\mu} with a=116a=1\dots 16 and μ=0,1,2,3\mu=0,1,2,3. We keep using the term “vierbein” (4-legs) for e^L\hat{e}_{L} given the 4-dimensional space-time indexed by μ=0,1,2,3\mu=0,1,2,3. If we want to accentuate the 16-dimensional Clifford algebraic subspace indexed by a=116a=1\dots 16, we could refer to e^L\hat{e}_{L} as “vielbein” (multi-legs). The metric gμνg_{\mu\nu}, defined as gμν=e^μe^νg_{\mu\nu}=\left\langle\hat{e}_{\mu}\hat{e}_{\nu}\right\rangle, is still a 4×44\times 4 tensor regardless of the dimension of the Clifford algebraic subspace of the vierbeins, since the underlying space-time (indexed by μ\mu and ν\nu ) is 4-dimensional. It’s worth mentioning that historically various proposals [48, 49, 50, 51, 54, 56, 170, 171] have been made to extend the vierbein (vielbein) space while keeping the 4-dimensional space-time.

With the extended symmetries, the chiral gauge-covariant derivatives of the left- and right-handed spinor fields ψL/R(x)\psi_{L/R}(x) are defined by

DLψL=(d+ω^L+W^L+W^L)ψL+ψL(G^+A^BL),\displaystyle D_{L}\psi_{L}=(d+\hat{\omega}_{L}+\hat{W}_{L}+\hat{W^{\prime}}_{L})\psi_{L}+\psi_{L}(\hat{G}+\hat{A}_{BL}), (220)
DRψR=(d+ω^R+W^R+W^R)ψR+ψR(G^+A^BL),\displaystyle D_{R}\psi_{R}=(d+\hat{\omega}_{R}+\hat{W}_{R}+\hat{W^{\prime}}_{R})\psi_{R}+\psi_{R}(\hat{G}+\hat{A}_{BL}), (221)

where the left-hand weak SU(2)WLSU(2)_{WL} gauge field W^L\hat{W}_{L}, the right-hand weak U(1)WRU(1)_{WR} gauge field W^R\hat{W}_{R}, the color SU(3)CSU(3)_{C} gauge field G^\hat{G}, and the BL U(1)BLU(1)_{B-L} gauge field A^BL\hat{A}_{BL} follow the same definition as specified previously (75). The newly introduced gauge fields are the left- and right-handed spin connections of the Spin(1,3)LSpin(1,3)_{L} and Spin(1,3)RSpin(1,3)_{R} Lorentz gauge groups

ω^L=14ωLμabγaγbdxμ,\displaystyle\hat{\omega}_{L}=\frac{1}{4}\omega_{L\mu}^{ab}\gamma_{a}\gamma_{b}dx^{\mu}, (222)
ω^R=14ωRμabγaγbdxμ,\displaystyle\hat{\omega}_{R}=\frac{1}{4}\omega_{R\mu}^{ab}\gamma_{a}\gamma_{b}dx^{\mu}, (223)

the pseudo-weak portion of the extended left-handed weak gauge field

W^L=12(WLμ1Γ0Γ1+WLμ2Γ0Γ3+WLμ3Γ0Γ3)dxμ,\displaystyle\hat{W^{\prime}}_{L}=\frac{1}{2}(W^{\prime 1}_{L\mu}\Gamma_{0}\Gamma_{1}+W^{\prime 2}_{L\mu}\Gamma_{0}\Gamma_{3}+W^{\prime 3}_{L\mu}\Gamma_{0}\Gamma_{3})dx^{\mu}, (224)

and the pseudo-weak portion of the extended right-handed weak gauge field

W^R=12WRμ3Γ0Γ3dxμ.\displaystyle\hat{W^{\prime}}_{R}=\frac{1}{2}W^{\prime 3}_{R\mu}\Gamma_{0}\Gamma_{3}dx^{\mu}. (225)

The combination of the regular weak W^L\hat{W}_{L} and the pseudo-weak W^L\hat{W^{\prime}}_{L} constitutes the overall gauge field of Spin(1,3)WLSpin(1,3)_{WL}

ω^IsoL=W^L+W^L.\displaystyle\hat{\omega}_{Iso-L}=\hat{W}_{L}+\hat{W^{\prime}}_{L}. (226)

We call ω^IsoL\hat{\omega}_{Iso-L} the isospin connection since it is in many ways analogous to the regular spin connection (222) of the Lorentz group.

The chiral spin connections ω^L\hat{\omega}_{L} and ω^R\hat{\omega}_{R} are crucial in maintaining the chiral Lorentz gauge covariance of DLψLD_{L}\psi_{L} and DRψRD_{R}\psi_{R}, which are leveraged in conjunction with the chiral vierbeins to ensure the chiral Lorentz gauge invariance of the Lagrangian terms.

The gauge interaction curvature 22-forms for ω^L\hat{\omega}_{L}, ω^R\hat{\omega}_{R}, W^L\hat{W^{\prime}}_{L}, and W^R\hat{W^{\prime}}_{R} are expressed as

R^L=dω^L+ω^Lω^L,\displaystyle\hat{R}_{L}=d\hat{\omega}_{L}+\hat{\omega}_{L}\wedge\hat{\omega}_{L}, (227)
R^R=dω^R+ω^Rω^R,\displaystyle\hat{R}_{R}=d\hat{\omega}_{R}+\hat{\omega}_{R}\wedge\hat{\omega}_{R}, (228)
F^WL=dW^L+W^LW^L+W^LW^L,\displaystyle\hat{F}_{W^{\prime}L}=d\hat{W^{\prime}}_{L}+\hat{W^{\prime}}_{L}\wedge\hat{W}_{L}+\hat{W}_{L}\wedge\hat{W^{\prime}}_{L}, (229)
F^WR=dW^R,\displaystyle\hat{F}_{W^{\prime}R}=d\hat{W^{\prime}}_{R}, (230)

where the outer product between gauge fields vanishes for the abelian interaction F^WR\hat{F}_{W^{\prime}R}. The regular left-handed weak force is appended with an additional cross product term of W^L\hat{W^{\prime}}_{L}

F^WL=dW^L+W^LW^L+W^LW^L.\displaystyle\hat{F}_{WL}=d\hat{W}_{L}+\hat{W}_{L}\wedge\hat{W}_{L}+\hat{W^{\prime}}_{L}\wedge\hat{W^{\prime}}_{L}. (231)

The combination of the weak F^WL\hat{F}_{WL} and the pseudo-weak F^WL\hat{F}_{W^{\prime}L} constitutes the overall gauge curvature 2-form of the weak Spin(1,3)WLSpin(1,3)_{WL}

R^IsoL=F^WL+F^WL=dω^IsoL+ω^IsoLω^IsoL.\displaystyle\hat{R}_{Iso-L}=\hat{F}_{WL}+\hat{F}_{W^{\prime}L}=d\hat{\omega}_{Iso-L}+\hat{\omega}_{Iso-L}\wedge\hat{\omega}_{Iso-L}. (232)

We call R^IsoL\hat{R}_{Iso-L} the isospin connection curvature 2-form (or the extended weak force) in parallel with the spin connection curvature 2-form R^L\hat{R}_{L} (227) of the Lorentz group.

The local gauge- and diffeomorphism-invariant Lagrangian terms of the world are similar to the ones we inspected earlier in Section 2.4, provided that the chirality and isospin conjugations are taken care of. The following are some examples

Fermion\displaystyle\mathcal{L}_{Fermion}\sim iIe^Le^Le^L(ψLDLψL¯)\displaystyle\;i\left\langle I\hat{e}_{L}\wedge\hat{e}_{L}\wedge\hat{e}_{L}\wedge(\psi_{L}\overline{D_{L}\psi_{L}})\right\rangle (233a)
+iIe^Rde^Rue^Rd(ψRuDRψRu¯)\displaystyle+\;i\left\langle I\hat{e}_{Rd}\wedge\hat{e}_{Ru}\wedge\hat{e}_{Rd}\wedge(\psi_{Ru}\overline{D_{R}\psi_{Ru}})\right\rangle (233b)
+iIe^Rue^Rde^Ru(ψRdDRψRd¯),\displaystyle+\;i\left\langle I\hat{e}_{Ru}\wedge\hat{e}_{Rd}\wedge\hat{e}_{Ru}\wedge(\psi_{Rd}\overline{D_{R}\psi_{Rd}})\right\rangle, (233c)
GravityLeft\displaystyle\mathcal{L}_{Gravity-Left}\sim Ie^Le^LR^L,\displaystyle\;\left\langle I\hat{e}_{L}\wedge\hat{e}_{L}\wedge\hat{R}_{L}\right\rangle, (233d)
GravityRight\displaystyle\mathcal{L}_{Gravity-Right}\sim I(e^Rue^Rd+e^Rde^Ru)R^R,\displaystyle\;\left\langle I(\hat{e}_{Ru}\wedge\hat{e}_{Rd}+\hat{e}_{Rd}\wedge\hat{e}_{Ru})\wedge\hat{R}_{R}\right\rangle, (233e)
CCLeft\displaystyle\mathcal{L}_{CC-Left}\sim Ie^Le^Le^Le^L,\displaystyle\;\left\langle I\hat{e}_{L}\wedge\hat{e}_{L}\wedge\hat{e}_{L}\wedge\hat{e}_{L}\right\rangle, (233f)
CCRight\displaystyle\mathcal{L}_{CC-Right}\sim Ie^Rue^Rde^Rue^Rd,\displaystyle\;\left\langle I\hat{e}_{Ru}\wedge\hat{e}_{Rd}\wedge\hat{e}_{Ru}\wedge\hat{e}_{Rd}\right\rangle, (233g)

where the alternation between e^Ru\hat{e}_{Ru} and e^Rd\hat{e}_{Rd} is because of the properties e^Ru=Pe^RuP+\hat{e}_{Ru}=P_{-}\hat{e}_{Ru}P_{+} and e^Rd=P+e^RdP\hat{e}_{Rd}=P_{+}\hat{e}_{Rd}P_{-}.

In view of the extended symmetries (4.4) of the Lagrangian of the world, let’s revisit the diffeomorphism and Lorentz gauge symmetry breaking triggered by the nonzero VEVs of the vierbeins. It can be checked that the flat space-time VEV (103) of the vierbein violates the gauge symmetries Spin(1,3)L×Spin(1,3)R×Spin(1,1)WRSpin(1,3)_{L}\times Spin(1,3)_{R}\times Spin(1,1)_{WR} and the coset Spin(1,3)WL/SU(2)WLSpin(1,3)_{WL}/SU(2)_{WL}. The remaining gauge symmetries are SU(3)C×SU(2)WL×U(1)WR×U(1)BLSU(3)_{C}\times SU(2)_{WL}\times U(1)_{WR}\times U(1)_{B-L} plus the residual global Lorentz symmetry as the combined remnant of the local Lorentz and diffeomorphism symmetries. We would like to highlight the fact that our model has no conflict with the Coleman-Mandula theorem [40], since neither the local Lorentz symmetry nor the residual global Lorentz symmetry has nontrivial mixing with the internal gauge symmetries. The interested reads are encouraged to read the discussion in the literature [166] regarding why the residual global Lorentz symmetry, rather than the broken local Lorentz symmetry, is the symmetry relevant to the Coleman-Mandula theorem.

Note that the VEV magnitudes and orientations of the three vierbeins e^L\hat{e}_{L}, e^Ru\hat{e}_{Ru}, and e^Rd\hat{e}_{Rd} may not align with each other. That said, we have the freedom to re-scale and re-orientate (via the global Lorentz rotations) the corresponding fermions, so that every vierbein takes the same flat space-time VEV everywhere all at once. Hence it is ensured that all fermions, regardless of their chirality and isospin types, share the universal Minkowski flat space-time metric.

However, there are some factors that can not be re-scaled away. These are the differences between the coefficients of the chiral gravity (233d) (233e) Lagrangian terms and the differences between the coefficients of the chiral cosmological constant (233f) (233g) Lagrangian terms. As a result, the left- and right-handed fermions experience different strengths of gravitational interactions. Under normal conditions, this is not a problem since the left- and right-handed matters are usually commensurate with each other. Thus we can’t really discern which chiral gravity is stronger since we routinely observe the collective gravitational interaction governed by a combined effective gravitational constant.

The only exception is when there is imbalance between the left- and right-handed matters. For example, let’s assume that the left-handed gravitational constant is larger than the right-handed counterpart. We could observe an unexplainable drop of gravitational force compared with expectation if there is an excess of right-handed matter. In this regard, we would like to draw attention to the right-handed neutrinos, since they are endowed with extremely large Majorana masses. If there is a large concentration of the right-handed neutrinos in certain parts of the universe, the discrepancies between the chiral gravitational forces would possibly be revealed.

In the last part of this subsection, we turn to a novel kind of gravi-weak Lagrangian terms

GravityWeakLeft\displaystyle\mathcal{L}_{Gravity-Weak-Left}\sim Ie^Le^LR^IsoL,\displaystyle\;\left\langle I\hat{e}_{L}\wedge\hat{e}_{L}\wedge\hat{R}_{Iso-L}\right\rangle, (234a)
HolstWeakLeft\displaystyle\mathcal{L}_{Holst-Weak-Left}\sim e^Le^LR^IsoL,\displaystyle\;\left\langle\hat{e}_{L}\wedge\hat{e}_{L}\wedge\hat{R}_{Iso-L}\right\rangle, (234b)

where R^IsoL\hat{R}_{Iso-L} is the left-handed isospin connection curvature 2-form (232). As indicated by the Lagrangian names, these terms bear close resemblance to the regular gravity (90) and Holst (95) Lagrangian terms. We mentioned earlier that under normal circumstances a Lagrangian term with a single Yang-Mills field curvature 2-form is identically zero. This is because the traditional vierbein is invariant under the Yang-Mills field-related gauge transformations. However, the extended left-handed vierbein e^L{\hat{e}_{L}} transforms as a vector under the extended left-handed weak symmetry Spin(1,3)WLSpin(1,3)_{WL}, which makes the above single-curvature gravi-weak terms possible.

Let’s derive the field equations for the left-handed gravity Lagrangian (233d) and the left-handed gravi-weak Lagrangian (234a) by varying with e^L\hat{e}_{L}, ω^L\hat{\omega}_{L}, and ω^IsoL\hat{\omega}_{Iso-L}, respectively. The resultant extended Einstein-Cartan equations read (for brevity sake we drop the LL subscripts and quantities are implicitly left-handed)

18πG(R^e^+e^R^)I+18πGIso(R^Isoe^+e^R^Iso)I=𝕋,\displaystyle\frac{1}{8\pi G}(\hat{R}\wedge\hat{e}+\hat{e}\wedge\hat{R})I+\frac{1}{8\pi G_{Iso}}(\hat{R}_{Iso}\wedge\hat{e}+\hat{e}\wedge\hat{R}_{Iso})I=\mathbb{T}, (235)
18πG(T^e^e^T^)I=𝕊,\displaystyle\frac{1}{8\pi G}(\hat{T}\wedge\hat{e}-\hat{e}\wedge\hat{T})I=\mathbb{S}, (236)
18πGIso(T^Isoe^e^T^Iso)I=𝕊Iso,\displaystyle\frac{1}{8\pi G_{Iso}}(\hat{T}_{Iso}\wedge\hat{e}-\hat{e}\wedge\hat{T}_{Iso})I=\mathbb{S}_{Iso}, (237)

where GG is the gravitational constant, GIsoG_{Iso} is the iso-gravitation constant for the gravi-weak Lagrangian (234a), 𝕋\mathbb{T} is the energy-momentum current 33-form, 𝕊\mathbb{S} is the spin current 33-form, 𝕊Iso\mathbb{S}_{Iso} is the isospin current 33-form, T^\hat{T} is the torsion 22-form (101), and T^Iso\hat{T}_{Iso} is the iso-torsion 22-form

T^Iso\displaystyle\hat{T}_{Iso} =de^+ω^Isoe^+e^ω^Iso.\displaystyle=d\hat{e}+\hat{\omega}_{Iso}\wedge\hat{e}+\hat{e}\wedge\hat{\omega}_{Iso}. (238)

Compared with the regular Einstein-Cartan equations, we have an additional equation for the iso-torsion T^Iso\hat{T}_{Iso}. Given that the weak gauge field W^L\hat{W}_{L} (as part of the isospin connection ω^IsoL\hat{\omega}_{Iso-L}) is susceptible to the SSB effects from the electroweak Higgs mechanism, we expect that the isospin connection ω^IsoL\hat{\omega}_{Iso-L} would have a different kind of impact on gravity than the regular spin connection ω^L\hat{\omega}_{L}.

This sort of gravi-weak modification to the gravitational equations could have cosmological implications. As we know, the concordance Λ\LambdaCDM cosmological model is besieged with a multitude of discordances [172, 173, 174], with the most acute one being the Hubble tension [175, 176, 177]. Various modified gravity models [178, 179, 180] have been proposed to remediate the shortcomings of the Λ\LambdaCDM model. There are two noteworthy modified gravity theories invoking two different scales: a characteristic Hubble scale h0h_{0} and a characteristic acceleration scale a0a_{0}. In cosmology, the characteristic Hubble scale h0h_{0} marks the boundary between the validity domains of Friedmann equation and modified Friedmann equation (MOFE) which could explain the late-time accelerated expansion of the universe without dark energy [28, 31], whereas in galactic dynamics the characteristic acceleration scale a0a_{0} marks the boundary between the validity domains of Newtonian dynamics and modified Newtonian dynamics (MOND) which could explain the galactic rotation curves without dark matter [181]. We hope that the gravi-weak interplay delineated above could possibly shed some light on the dark side of the universe.

5 Conclusions

The naturalness problems have been front and center in physics researches [155, 156, 157, 119, 120, 121]. The cosmological constant problem is arguably the most severe naturalness problem in physics, with the runner-up being the Higgs mass/electroweak hierarchy problem. With the goal of addressing the naturalness problems, we propose that each and every symmetry-breaking bosonic field is an effective representation of a unique multi-fermion quantum condensation via the dynamical symmetry breaking mechanism. Note that while these symmetry-breaking fields such as the vierbein and Higgs fields are composite fields, all the standard model fermion fields and all the gauge fields in our model are still fundamental non-composite fields.

Our research originated from drawing a previously unappreciated distinction between two imaginary numbers [30, 31]: The first one is the bona fide imaginary number ii which governs the quantum world, whereas the other one is the unit pseudoscalar II of Clifford algebra Cl(0,6)Cl(0,6) masquerading as imaginary number which shows up in the definition of spinors, gauge fields, and their transformations. In the Clifford algebra approach, we can manage to completely avoid imaginary number ii in classical field equations with classical spinors and gauge fields defined as Clifford multivectors. This is demonstrated by the Clifford algebraic Dirac equation (142), where the conventional ii is replaced by pseudoscalar II as long as we stick to the regime of applying pseudoscalar II to the right side of the algebraic spinor.

However, when it comes to the fermion Lagrangian, the imaginary number ii is irreplaceable in both the kinetic and mass terms. The conundrum of the quantum ii enmeshed in the classical spinor Lagrangian indicates that the regular classical Lagrangian terms might be of quantum origin. We propound that the imaginary number in the fermion Lagrangian stems from the odd number of quantum loop integrals related to the odd number of fermion-antifermion quantum condensations. On the other hand, if there are even fermion-antifermion pairs involved in the quantum condensations with even number of quantum loop integrals, there is no ii in the Lagrangian term, such as the Yang-Mills, gravity, and cosmological constant terms.

We would like to underscore the fact that there is no fixed mass/energy scale in the pre-symmetry breaking world, since the original Lagrangian coefficients are dimensionless. In other words, the pre-condensation Lagrangian terms are scale-invariant. Each mass scale of the universe, including the Planck scale, is associated with a particular symmetry and the corresponding symmetry breaking process via quantum condensation. This pan-emergence paradigm of mass scales parallels Landau’s symmetry breaking scheme in condensed matter physics characterized by the nonzero order parameter. One exception to this rule might be the QCD scale ΛQCD\Lambda_{QCD} which is possibly generated by a topological order in quark-gluon plasma and nucleons akin to the fractional quantum Hall effect [32].

Let’s take stock of various symmetry-breaking quantum condensations examined in this paper. The first category of quantum condensation involves a standard model fermion-antifermion pair of the same chirality, with a gauge-covariant derivative sandwiched in between. The effective representation of this sort of condensation corresponds to the vierbein field e^\hat{e} in the Lorentz gauge theory of gravity. In the composite vierbein scenario, the standard model fermions play the dual role of interacting with the space-time metric as well as being the metric. Consequently, quantum gravity is realized indirectly via the quantized spinor fields which underlie the composite space-time metric. Allowed by the extended vierbein valued in the 16-dimensional multivector subspace spanned by { γaΓ0Γi\gamma_{a}\Gamma_{0}\Gamma_{i} } in addition to { γa\gamma_{a}}, our model accommodates an extended left-handed weak gauge group Spin(1,3)WLSpin(1,3)_{WL} which encompasses the standard model left-handed weak gauge group SU(2)WLSU(2)_{WL}. A gravi-weak interplay is thus permitted between the extended vierbein field and the extended weak gauge field.

The local Lorentz and pseudo-weak symmetries are broken when the vierbeins acquire nonzero VEVs via the dynamical symmetry breaking mechanism. One interesting implication is that there are two different energy scales related to this symmetry breaking process. One is the compositeness scale above which there are measurable evidences of the composite vierbeins broken down into the underlying fermionic components, while the other is the Planck scale at which the higher-order gravitational Lagrangian terms become relevant in the effective field theory of quantum gravity. The second implication is that the coefficients of the effective cosmological constant and gravity Lagrangian terms are dictated by the divergent Feynman integrals of quantum condensations. We advocate a paradigm shift from the conventional single-scale renormalization procedure. The cosmological constant problem can thus be evaded if we adopt a multi-scale renormalization procedure (RR procedure) for quantum condensations that entail multiplications of divergent Feynman integrals.

The second category of quantum condensation involves a neutrino-antineutrino pair with right-handed chirality which breaks the BSM symmetries. The effective description of this sort of condensation is the Majorana-Higgs field ϕM\phi_{M}. It is a Higgs-like field whose VEV generates mass for the ZZ^{\prime} gauge field and the Majorana mass for the right-handed neutrino. The Majorana mass is capable of directly mixing neutrinos from different generations, which is evidenced in the observation of neutrino oscillations[78, 79, 80]. The Clifford algebra Cl(0,6)Cl(0,6) allows for a weaker form of charge conjugation which does not invoke particle-antiparticle interchange. Consequently, the Clifford algebraic Majorana mass conserves lepton number, which is different from the traditional Majorana mass term. This might be the underlying reason that no evidence has ever been found for the neutrinoless double beta decay [91, 92].

The third category of quantum condensation involves a standard model fermion-antifermion pair with opposite chirality. Belonging to this category, the standard model Higgs field ϕt\phi_{t} is an effective description of the top quark condensation, while the other two yet-to-be-detected composite Higgs fields ϕντ\phi_{\nu_{\tau}} and ϕτ\phi_{\tau} correspond to the tau neutrino and tau lepton condensations, respectively. The VEVs of these three composite Higgs fields break the electroweak symmetries and generate masses for the Z0Z^{0}/W±W^{\pm} gauge fields and the Dirac masses for the standard model fermions. The composite Higgs mass is naturally small, since at the electroweak scale there is no elementary Higgs mass term to be modified by any higher order quantum perturbation from external sources.

The three estimated Higgs VEVs have a hierarchical structure υt246GeV\upsilon_{t}\approx 246\;GeV, υντ42GeV\upsilon_{\nu_{\tau}}\approx 42\;GeV and υτ2.5GeV\upsilon_{{\tau}}\approx 2.5\;GeV. The top-quark Higgs VEV υt\upsilon_{t} is much larger than the other two. Nonetheless, the tau-neutrino Higgs VEV υντ\upsilon_{\nu_{\tau}} plays a non-negligible role in the electroweak scale saturation, which might be the root cause of the significant deviation of the measured W-boson mass from the standard model prediction [114]. Additionally, given the intrinsic connection between the muon and the tau-neutrino Higgs field ϕντ\phi_{\nu_{\tau}}, it is worthwhile to investigate the tau-neutrino Higgs field’s contribution to the muon anomalous magnetic moment, especially in light of the recent muon g2g-2 measurement which confirms a deviation from the standard model prediction [115].

The fourth category of quantum condensation involves a standard model fermion-antifermion pair with opposite chirality, similar to the regular composite Higgs field in the third category. However, the Clifford algebra framework allows for a non-scalar antisymmetric-tensor composite Higgs field ϕAT\phi_{AT} which could potentially break both the electroweak and Lorentz symmetries. The magnitude of its VEV could be extremely small compared with the electroweak scale, rendering its effects unobservable in laboratories. The ethereal VEV of the antisymmetric-tensor Higgs field might manifest itself as the large-scale anisotropies of the universe [96, 97, 98, 99, 100, 101].

The fifth category of quantum condensation involves two standard model fermion-antifermion pairs. There are six composite Φ\Phi fields corresponding to this sort of four-fermion condensations. In contrast to the other four types of composite fields, these scalar Φ\Phi fields are invariant under all the local gauge transformations. Instead, three of the Φ\Phi fields are tied to a Uα(1)U_{\alpha}(1) global symmetry, which transforms all the right-handed fermions by the same phase eαIe^{\alpha I}, in a manner similar to the Peccei-Quinn U(1)PQU(1)_{PQ} symmetry. The other three of the Φ\Phi fields are tied to a Uβ(1)U_{\beta}(1) global symmetry. It transforms the up-type quarks (uRu_{R}, cRc_{R}, tRt_{R}) and down-type leptons (eRe_{R}, μR\mu_{R}, τR\tau_{R}) by the phase eβIe^{\beta I}, whereas it transforms the down-type quarks (dRd_{R}, sRs_{R}, bRb_{R}) and up-type leptons (νeR\nu_{eR}, νμR\nu_{{\mu}R}, ντR\nu_{{\tau}R}) by the opposite phase eβIe^{-\beta I}.

Upon acquiring nonzero VEVs, these six composite fields break the Uα(1)U_{\alpha}(1) and Uβ(1)U_{\beta}(1) global symmetries respectively. Their VEVs play a pivotal role in establishing the relative magnitudes of the effective Yukawa coupling constants, and consequently giving rise to the fermion mass hierarchies. According to the effective Yukawa coupling ansatz, the Dirac masses of the ντ\nu_{\tau}, νμ{{\nu_{\mu}}} and νe{{\nu_{e}}} neutrinos are estimated as 29,500MeV29,500MeV, 40MeV40MeV and 21MeV21MeV, respectively. Note that these estimations are meant to be the Dirac masses, as opposed to the significantly smaller seesaw effective masses.

Due to the explicit symmetry breaking originated from the quantum anomaly and instanton effects, the otherwise massless Nambu-Goldstone bosons of the α\alpha-type Φ\Phi fields acquire masses and turn into the pseudo-Nambu-Goldstone bosons in a similar fashion as the axions. Historically the axions have been proposed as a possible solution to the strong CP and dark matter problems. In this regard, we speculate that the (pseudo-)Nambu-Goldstone bosons of the β\beta-type Φ\Phi fields could also be viable dark matter candidates.

In summary, the proposition in this paper is at the conservative end of the spectrum of physics modeling. Our thesis is that the space-time manifold is 4-dimensional and the fundamental building blocks of the universe are just the garden-variety standard model fermions plus the right-handed neutrinos, accompanied by a handful of “good old-fashioned” gauge fields such as the spin connection Lorentz gauge fields and the Yang-Mills-type gauge fields. That is all there is. There are neither compactified extra space dimensions nor exotic wiggling p-branes. The novel bit we bring to the table is the insight that there is a kaleidoscope of quantum condensations which make the world as complex and enchanting as it is.

Acknowledgement

I am grateful to Matej Pavšič and Grigory Volovik for helpful discussions.

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