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Exploring the 00^{-} bound state with dressed quarks in Minkowski space

A. Castro abigail@ita.br Instituto Tecnológico de Aeronáutica, DCTA, 12228-900 São José dos Campos, Brazil W. de Paula wayne@ita.br E. Ydrefors ydrefors@kth.se Institute of Modern Physics, Chinese Academy of Sciences, Lanzhou 730000, China T. Frederico tobias@ita.br G. Salmè Giovanni.Salme@roma1.infn.it INFN, Sezione di Roma, P.le A. Moro 2, 00185 Rome, Italy
(September 23, 2025)
Abstract

The Bethe-Salpeter equation for a pseudoscalar bound-system, with i) a ladder kernel with massive gluons, ii) dynamically-dressed quark mass function and iii) an extended quark-gluon vertex, is solved in Minkowski space by using the Nakanishi integral representation of the Bethe-Salpeter amplitude. The quark dressing is implemented through a phenomenological ansatz, which was tuned by lattice QCD calculations of the quark running mass. The latter were also used for assigning the range of the gluon mass and the parameter featuring the extended color density. This framework allows to investigate the gluon dynamics that manifest itself in the quark dressing, quark-gluon vertex and the binding, directly in the physical space. We present the first results for low-density pseudoscalar systems in order to elucidate the onset of the interplay between the above mentioned gluonic phenomena, and we discuss both static and dynamical quantities, like valence longitudinal and transverse distributions.

keywords:
Bethe-Salpeter equation, Dressed quark propagator, Minkowski-space dynamics.

Introduction Understanding the relation between dynamical chiral symmetry breaking (DCSB) (see, e.g., Refs. [1, 2, 3] for a general introduction) and bound-state formation in Minkowski space is a fundamental issue for shedding light on the generation of the hadronic masses. In fact, many valuable theoretical and experimental efforts are underway and/or planned in the near future (see, e.g., Refs. [4, 5] for the experimental state-of-the-art). The attempt to describe the hadronic bound-states in Minkowski space by using a dynamical equation, living in a genuine relativistic quantum-field theory realm, deserves attention, in view of the possible cross-fertilization with the main tool represented by the lattice Quantum-Chromodynamics (LQCD) and also the continuum approach to QCD, extensively pursued in Euclidean space (see Ref. [6, 7] for recent overviews). Our approach is based on the qq¯q\bar{q} homogeneous Bethe-Salpeter equation (BSE) in Minkowski space (see also Refs. [8, 9, 10] for different approaches in Minkowski space), with phenomenologically dressed quarks that interact through a ladder exchange of massive gluons. Therefore, we do not rely on the equivalence between the relativistic quantum-field theory and the Euclidean version, well-established within the formal framework elaborated in the 70’s by Osterwalder and Schrader (see Ref. [11, 12] where necessary and sufficient conditions for ensuring the validity of the Wick rotation are demonstrated). In what follows, we adopt the well-established Nakanishi integral representation (NIR) of the Bethe-Salpeter (BS) amplitude and the light-front (LF) projection of the BSE, in order to obtain a fully equivalent system of integral equations that allows to determine the Nakanishi weight functions (NWFs), and eventually the BS amplitude (see Refs. [13, 14] for the general application to a 00^{-} bound system with undressed propagator, and Refs. [15, 16, 17, 18] for the weak decay constant, valence probability, Ioffe distribution, electromagnetic form factor, parton distribution function and unpolarized transverse-momentum-dependent distribution functions for a pion with mass mπm_{\pi} equal to 140140 MeV). After assigning the mass of the bound system, one solves the BSE and gets the corresponding coupling constant and BS amplitude, that in turn allows one to calculate the valence longitudinal and transverse momentum distributions. Both static and dynamical quantities are used for investigating how the interplay between three fundamental gluonic phenomena, i.e. quark dressing, extended quark-gluon vertex and binding, evolves in a system-mass range 3mπ<M<5mπ3m_{\pi}<M<5m_{\pi}, corresponding to a relatively diluted bound system with constrained quark-masses (see below). The primary focus is on the combined effect of the quark dressing and the increase of the color-density extension around the quark-gluon vertex, which allows to enhance gluon fluctuations with low-momentum.

The homogeneous BSE for a 00^{-} system. In the adopted ladder approximation with a massive gluon-exchange, the BSE for a 00^{-} quark-antiquark bound state, with total momentum PP and mass MM, is given by  [19] (see also Ref. [20])

Φ(k,P)=S(k+P2)d4k(2π)4Dμν(q)Γμ(q)×Φ(k,p)Γ^ν(q)S(kP2),\Phi(k,P)=S\left(k+{P\over 2}\right)\int\frac{d^{4}k^{\prime}}{(2\pi)^{4}}~D^{\mu\nu}(q)\Gamma_{\mu}(q)\\ \times~\Phi(k^{\prime},p)~\hat{\Gamma}_{\nu}(q)~S\left(k-{P\over 2}\right)\,, (1)

where k=(pqpq¯)/2k=(p_{q}-p_{\bar{q}})/2, with pq(q¯)p_{q(\bar{q})} the off-shell (anti-) quark momentum, and q=kkq=k-k^{\prime}. Γμ\Gamma_{\mu} is the quark-gluon vertex and Γ^μ=CΓμTC1{\hat{\Gamma}}_{\mu}=C\,\Gamma^{T}_{\mu}\,C^{-1}, where C=iγ2γ0C=i\,\gamma^{2}\,\gamma^{0} is the charge-conjugation operator. In Eq. (1), we inserted the following three relevant ingredients. First, a dressed Dirac propagator, that for a parity-conserving interaction, reads

S(p)=SV(p2)/p+SS(p2)=i0𝑑sρV(s)/p+ρS(s)p2s+iϵ,S(p)=S^{V}(p^{2})/\!\!\!p+S^{S}(p^{2})\\ =i\int_{0}^{\infty}ds~\frac{\rho^{V}(s)\,/\!\!\!p+\rho^{S}(s)}{p^{2}-s+i\epsilon}~, (2)

where in the first line one has the decomposition in terms of allowed Dirac structures and corresponding scalar functions, while in the second line one has the dispersive representation (see, e.g., Ref. [21] for the Källen-Lehman representation in QED), with two weights to be phenomenologically parametrized (at the present stage), as explained below. Second, a massive gluon-propagator, Dμν(q)D^{\mu\nu}(q), in the Feynman gauge, written as follows

Dμν(q)=igμν(q2μ2+iϵ),D^{\mu\nu}(q)=-i{g^{\mu\nu}\over(q^{2}-\mu^{2}+i\epsilon)}\,, (3)

where μ\mu is the gluon mass. Last but not least, a quark-gluon vertex, Γμ(q)\Gamma^{\mu}(q), dressed through a simple form factor, is adopted, i.e.

Γμ(q)=igμ2Λ2q2Λ2+iϵγμ,\displaystyle\Gamma^{\mu}(q)=i\,g\,\frac{\mu^{2}-\Lambda^{2}}{q^{2}-\Lambda^{2}+i\epsilon}\,\gamma^{\mu}\,, (4)

where Λ\Lambda features the extension of the color distribution dressing the interaction vertex.

For a 00^{-} qq¯q\bar{q}-system, the BS amplitude can be decomposed as follows [22]

Φ(k,P)=i=14Si(k,P)ϕi(k,P),\Phi(k,P)=\sum^{4}_{i=1}S_{i}(k,P)\phi_{i}(k,P), (5)

where i) ϕi\phi_{i} are scalar functions, that under a kkk\to-k transformations are even for i=1,2,4i=1,2,4 and odd for i=3i=3 (assuming isospin symmetry), and ii) the SiS_{i} matrices compose the following orthogonal basis

S1(k,P)=γ5,S2(k,P)=/PMγ5,\displaystyle S_{1}(k,P)=\gamma^{5}\,,\quad S_{2}(k,P)=\frac{/\!\!\!{P}}{M}\gamma^{5}\,,
S3(k,P)=kPM3/Pγ5/kMγ5,\displaystyle S_{3}(k,P)=\frac{k\cdot{P}}{M^{3}}/\!\!\!{P}\gamma^{5}-\frac{/\!\!\!{k}}{M}\gamma_{5}\,,\quad
S4(k,P)=iσμνPμkνM2γ5.\displaystyle S_{4}(k,P)=\frac{i\sigma^{\mu\nu}P_{\mu}k_{\nu}}{M^{2}}\gamma^{5}. (6)

Dressing the quark propagator. As is well-known, in a given gauge, the dressed quark propagator can be written as follows

S(p)=iZ(p2)/p+(p2)p22(p2),S(p)=i\,Z(p^{2})~{/\!\!\!p+{\cal M}(p^{2})\over p^{2}-{\cal M}^{2}(p^{2})}~, (7)

where (p2){\cal M}(p^{2}) is the quark-mass function and Z(p2)Z(p^{2}) the wave-function renormalization. In the present work, disregarding the gauge dependence, we adopt a phenomenological approach proposed in Ref. [23], where Z(p2)=1Z(p^{2})=1 and the quark-mass function (p2){\cal M}(p^{2}) was obtained by fitting a recent LQCD quark mass-function [24, 25] 111Notice that in Ref. [23], the Landau-gauge LQCD calculations of Ref. [26] were used. by using for p20p^{2}\leq 0 the following simple expression (with a pole in the timelike region)

(p2)=m0m3p2λ2+iϵ,\displaystyle{\cal M}(p^{2})=m_{0}-{m^{3}\over p^{2}-\lambda^{2}+i\epsilon}~, (8)

where the three parameters are chosen as follows: i) the bare mass m0m_{0} and the infrared (IR) mass (0)=m0+m3/λ2{\cal M}(0)=m_{0}+m^{3}/\lambda^{2} are taken equal to the values of the accurate parameterization proposed in Ref. [25] of the LQCD calculations presented in Ref. [24], i.e. m0=m0LQCD=0.008m_{0}=m^{LQCD}_{0}=0.008 GeV and (0)=LQCD(0)=0.344{\cal M}(0)={\cal M}^{LQCD}(0)=0.344 GeV; ii) while λ\lambda is properly adjusted. In conclusion we have the following values in Eq. (8)

m0=0.008GeV,m=0.648GeV,λ=0.9GeV.m_{0}=0.008\,GeV~,\quad m=0.648\,~GeV,\quad\lambda=0.9\,GeV.

Notice that mm allows to interpolate between a current-mass quark scenario and a fully-dressed one, while λ\lambda yields the width at the half height of the difference (0)m0{\cal M}(0)-m_{0}. The comparison between our fit and the mass function given in Ref. [24] is shown in the upper panel of Fig. 1, where in abscissa there is the Euclidean momentum pE=p2p_{E}=\sqrt{-p^{2}}.

The propagator in Eq. (7) has poles whenever mi=(mi2)m_{i}={\cal M}(m^{2}_{i}). In particular, one has only three poles, solutions of the cubic equation

mi(mi2λ2)=±[m0(mi2λ2)m3].m_{i}(m^{2}_{i}-\lambda^{2})=\pm[m_{0}(m_{i}^{2}-\lambda^{2})-m^{3}]\,. (9)

It turns out that ρV(S)(s)\rho^{V(S)}(s) in Eq. (2) are given by a sum of three Dirac delta-functions [23], viz.

ρS(V)(s)=a=13RaS(V)δ(sma2),\displaystyle\rho^{S(V)}(s)=\sum_{a=1}^{3}R^{S(V)}_{a}\delta(s-m_{a}^{2})~, (10)

where RaS(V)R^{S(V)}_{a} are the residues, that read

RaV=(λ2ma2)2(ma2mb2)(ma2mc2),\displaystyle R^{V}_{a}=\frac{(\lambda^{2}-m^{2}_{a})^{2}}{(m_{a}^{2}-m_{b}^{2})(m^{2}_{a}-m^{2}_{c})}~,
RaS=RaV(ma2),\displaystyle R^{S}_{a}=R^{V}_{a}~{\cal M}(m_{a}^{2}), (11)

with the indices {a,b,c}\{a,b,c\} following the cyclic permutation {1,2,3}\{1,2,3\}. They fulfill the following relations

a=13RaV=1,a=13RaS=m0,\displaystyle\sum_{a=1}^{3}R_{a}^{V}=1\,,\quad\sum_{a=1}^{3}R_{a}^{S}=m_{0}\,\,, (12)
a=13ma2RaV=2λ2+a=13ma2.\displaystyle\sum_{a=1}^{3}m_{a}^{2}R_{a}^{V}=-2\lambda^{2}+\sum_{a=1}^{3}m^{2}_{a}\,. (13)

The actual values of both poles and residues are given in Table 1.

Table 1: Poles, mim_{i}, and residues, RiR_{i},(cf Eqs. (10) and (11)) for the fit to the LQCD mass function in Ref. [24]. The IR mass (0)=m0+m3/λ2{\cal M}(0)=m_{0}+m^{3}/\lambda^{2} is 0.344 GeV, and the parameters of the running mass are also given in the Table.
  ii mi/(0)m_{i}/{\cal M}(0) RiVR^{V}_{i} RiS/(0)R^{S}_{i}/{\cal M}(0)
1 1.365 3.7784 5.1578
2 1.667 -2.8863 -4.8099
3 3.008 0.1079 -0.3244
m0/(0)m_{0}/{\cal M}(0) m/(0)~~m/{\cal M}(0) λ/(0)~~\lambda/{\cal M}(0)
0.0233 1.883 2.616

Let us recall that for a physical particle belonging to the S-matrix representation, the Källen-Lehmann spectral densities satisfy the positivity constraints [27]:

ρV(s)0andsρV(s)ρS(s)0.\rho^{V}(s)\geq 0\,\,\,\,\text{and}\,\,\,\,\sqrt{s}\,\rho^{V}(s)-\rho^{S}(s)\geq 0\,. (14)

Differently, in QCD the colored quark cannot be an asymptotic state and therefore the weights in Eq. (2) should violate the positivity constraints, which actually happens in the present model. For example, if ma<mb<mcm_{a}<m_{b}<m_{c} one has RbV<0R^{V}_{b}<0, which trivially implies the violation of the positivity constraint ρV(s)0\rho^{V}(s)\geq 0 for s=mb2s=m_{b}^{2}.

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Figure 1: (Color online) Upper panel. The quark running-mass, (p2){\cal M}(p^{2}), as a function of the Euclidean momentum pE=p2{p_{E}=\sqrt{-p^{2}}}, in units of the IR mass (0)=0.344{\cal M}(0)=0.344\,GeV. Solid line: Eq. (8) with m0=0.008m_{0}=0.008\,GeV, m=0.648m=0.648\,GeV and λ=0.9\lambda=0.9\,GeV. Dashed line: parameterization proposed in Ref. [25] of the LQCD calculations in Ref.  [24]. Lower panel. The two quantities SV(p2)[p22(0)]S^{V}(p^{2})~[p^{2}-{\cal M}^{2}(0)] (solid line) and SS(p2)[p22(0)]/(0)S^{S}(p^{2})~[p^{2}-{\cal M}^{2}(0)]/{\cal M}(0) (dashed line) vs. pE/(0)p_{E}/{\cal M}(0).

The lower panel of Fig. 1 shows the two quantities SV(p2)[p22(0)]S^{V}(p^{2})~[p^{2}-{\cal M}^{2}(0)] and SS(p2)[p22(0)]/(0)S^{S}(p^{2})~[p^{2}-{\cal M}^{2}(0)]/{\cal M}(0) (cf. Eq. (2), first line), obtained by means of Eq. (10), with poles and residues given in Table 1. It is worth noting that, for both functions, the tails are the expected ones in the limit pE(0)p_{E}\gg{\cal M}(0), i.e. the ones pertaining to a massless quark propagator, /p/p2/\!\!\!p/p^{2}.

Solving the 00^{-} BSE with dressed quarks. To solve the BSE for a pseudoscalar qq¯q\bar{q} bound-system, with momentum-dependent dressed quark-propagators, in Minkowski space, we apply the same technique already adopted in Refs. [13, 14], but for the same BSE with massive free-quark propagators. We use the NIR [28] of the scalar function ϕi(k,P)\phi_{i}(k,P), that reads

ϕi(k,P)=11𝑑z0𝑑γgi(γ,z)[k2+zPkγκ2+iϵ]3,\hskip-8.5359pt\phi_{i}(k,P)=\hskip-2.84544pt\int_{-1}^{1}\hskip-5.69046ptdz^{\prime}\int_{0}^{\infty}\hskip-5.69046ptd\gamma^{\prime}{g_{i}(\gamma^{\prime},z^{\prime})\over\left[{k}^{2}+z^{\prime}P\cdot k-\gamma^{\prime}-\kappa^{2}+i\epsilon\right]^{3}}, (15)

where κ2=m12M2/4\kappa^{2}=m_{1}^{2}-M^{2}/4, with m1m_{1} the lightest pole (cf. Table 1), and gi(γ,z)g_{i}(\gamma^{\prime},z^{\prime}) are the NWFs. The role of the NIR is to give to the BS amplitude an analytical structure in terms of the external momenta, which makes it possible to analytically perform the needed loop-momentum integration present in the interaction kernel. Hence, from the initial BSE, through the so-called LF projection, i.e. the integration on the component k=k0k3k^{-}=k^{0}-k^{3} (see details in Refs. [13, 14]) and taking into account Eq. (2), one can formally obtain the following system of integral equations for the NWFs

0𝑑γgi(γ,z)[γ+z2M2/4+γ+κ2iϵ]2=α2πj11𝑑z0𝑑γij(γ,z;γ,z)gj(γ,z).\int_{0}^{\infty}d\gamma^{\prime}\frac{g_{i}(\gamma^{\prime},z)}{\Big{[}\gamma+z^{2}M^{2}/4+\gamma^{\prime}+\kappa^{2}-i\epsilon\Big{]}^{2}}=\\ {\alpha\over 2\pi}\sum_{j}\int_{-1}^{1}dz^{\prime}\int_{0}^{\infty}d\gamma^{\prime}{\cal L}_{ij}(\gamma,z;\gamma^{\prime},z^{\prime})\,g_{j}(\gamma^{\prime},z^{\prime})\,. (16)

where α=g2/4π\alpha={g^{2}/4\pi}, with gg the dimensionless coupling constant, γ=|𝐤|2\gamma=|{\bf k}_{\perp}|^{2}, and the kernel ij{\cal L}_{ij} is obtained by a lengthy, but straightforward analytical steps (see Ref. [29] for details).

It should be pointed out that if the system in (16) admits a solution (N.B. one has to deal with a generalized eigenvalue problem) the use of the NIR is validated, and one can reconstruct the BS amplitude via Eq. (15).

Results. The solutions of the BSE for a pseudoscalar qq¯q\bar{q} bound-state have been obtained for masses ranging from M=0.653M=0.653\,GeV to M=0.447M=0.447\,GeV, and suitable values of both gluon mass μ\mu and vertex parameter Λ\Lambda to explore the interplay between these gluonic scales. The effective gluon mass is taken around 2ΛQCD\sim 2\Lambda_{QCD} [30], and the size of the quark- gluon vertex of the order ΛQCD\sim\Lambda_{QCD} (see, e.g., Ref. [25]).

In previous studies of the pion with physical mass [15, 17], by using a fixed quark mass of 0.2550.255 GeV (corresponding almost to the inflection point of the mass function shown in the upper panel of Fig. 1), a gluon mass of 0.6380.638 GeV and a vertex parameter Λ=0.306\Lambda=0.306\,GeV, we obtained: i) a decay constant fπ=130f_{\pi}=130\,MeV, in agreement with the experimental value [31] and ii) a valence probability of 70%, with 57% for the antialigned combination of the quark spins and 13% for the aligned one (see below). In this case, the gluon contribution to the pion state from the higher light-front Fock-components amounts to 30%, which reflects the fluctuation of the pion in a qq¯q\bar{q} pair plus any number of gluons (recall that we are using a ladder kernel). Such massive gluon fluctuations are generated by a color source, which has a size of about c/Λ=0.645\hbar c/\Lambda=0.645\,fm (not far from the size of the pion) and is able to reproduce the pion properties like the electromagnetic form factor [16] and longitudinal parton distribution [17]. In the present study we have a IR mass of 0.3440.344\, GeV equal to the one of the LQCD quark mass-function [24], and we tune the gluon mass to μ=0.469\mu=0.469\, GeV and Λ=0.1\Lambda=0.1\,GeV, so that the size of the color source considerably swells to c/Λ2\sim\hbar c/\Lambda\approx 2\,fm. Thus, the gluon fluctuations are produced at large distances. Both the combined effect of the somewhat smaller gluon mass and the strong IR enhancement of the interaction is expected to increase the Fock components of the pion containing the dynamical gluons and simultaneously reduce the valence probability. Indeed, at the pion mass, the fixed-mass approach, with a quark mass equal to 0.3440.344 GeV and the previous values of μ\mu and Λ\Lambda, provides a percentage of 51% for the Fock components beyond the valence one and a decay constant fπ=89.8f_{\pi}=89.8\, MeV. Due to a quark-mass larger than the one in the previous studies, the pion becomes more dilute, and the relevance of Fock components beyond the valence one increases from 30%30\% to 51%51\%. Moreover, the valence fraction of the aligned component reduces to 7%, compared to the previous case of 18.6% (stemming from the probability ratio 13/7013/70).

To gain a first insight into the dynamics generated by a large color source when the running quark mass is considered, with the corresponding parametrization that favors a large gluonic content of the bound state, i.e. with μ=0.469\mu=0.469\,GeV and Λ=0.1\Lambda=0.1\,GeV, we have calculated the valence wave function, i.e. the amplitude of the leading component in the Fock expansion of the state (see, e.g., Ref. [15]) for masses of the bound system in the range 3mπ<M<5mπ3m_{\pi}<M<5m_{\pi} (cf. Table 2). The valence wave function is obtained by LF-projecting the BS amplitude, and notably, it can be decomposed into its quark-spin configurations, S=0S=0 and S=1S=1. One writes the anti-aligned and aligned configurations, respectively, as [15]

Ψ(γ,z)=\displaystyle\Psi_{\uparrow\downarrow}(\gamma,z)= Ψ(γ,z)=ψ2(γ,z)+z2ψ3(γ,z)\displaystyle\Psi_{\downarrow\uparrow}(\gamma,z)=\psi_{2}(\gamma,z)+{z\over 2}\psi_{3}(\gamma,z) (17)
+iM30\displaystyle+{i\over M^{3}}~\int_{0}^{\infty} dγg3(γ,z;κ2)/zγ+γ+z2m2+(1z2)κ2,\displaystyle d\gamma^{\prime}~~{\partial g_{3}(\gamma^{\prime},z;\kappa^{2})/\partial z\over\gamma+\gamma^{\prime}+z^{2}m^{2}+(1-z^{2})\kappa^{2}}\,,
Ψ(γ,z)=\displaystyle\Psi_{\uparrow\uparrow}(\gamma,z)= Ψ(γ,z)=γMψ4(γ,z),\displaystyle\Psi_{\downarrow\downarrow}(\gamma,z)=\frac{\sqrt{\gamma}}{M~}\psi_{4}(\gamma,z)\,,

where m=m1m=m_{1} for the running mass case, and the amplitudes ψi(γ,z)\psi_{i}(\gamma,z) are obtained by integrating on kk^{-} the scalar functions in Eq. (15). In correspondence, one defines the valence probability density as follows

ρval(γ,z)=ρ(γ,z)+ρ(γ,z),\rho_{val}(\gamma,z)=\rho_{\uparrow\downarrow}(\gamma,z)+\rho_{\uparrow\uparrow}(\gamma,z)\,, (18)

where

ρ()(γ,z)=Nc16π2|Ψ()(γ,z)|2.\displaystyle\rho_{\uparrow\downarrow(\uparrow\uparrow)}(\gamma,z)=\frac{N_{c}}{16\pi^{2}}|{\Psi}_{\uparrow\downarrow(\uparrow\uparrow)}(\gamma,z)|^{2}\,\,. (19)

Finally, by normalizing ρval\rho_{val} to 11, we have calculated: i) the percentage of each spin components, PP_{\uparrow\downarrow} and PP_{\uparrow\uparrow}, and ii) the longitudinal and transverse distributions, that in turn can be decomposed in their spin components. Namely, the longitudinal and the transverse momentum distributions are given by

ϕ(ξ)=ϕ(ξ)+ϕ(ξ),\displaystyle\phi(\xi)=\phi_{\uparrow\downarrow}(\xi)+\phi_{\uparrow\uparrow}(\xi)\,, (20)
𝒫(γ)=𝒫(γ)+𝒫(γ),\displaystyle{\cal P}(\gamma)={\cal P}_{\uparrow\downarrow}(\gamma)+{\cal P}_{\uparrow\uparrow}(\gamma)\,, (21)

where

ϕ()(ξ)=0𝑑γρ()(γ,z),\displaystyle\phi_{\uparrow\downarrow(\uparrow\uparrow)}(\xi)=\int^{\infty}_{0}d\gamma~\rho_{\uparrow\downarrow(\uparrow\uparrow)}(\gamma,z)\,, (22)
𝒫()(γ)=11𝑑zρ()(γ,z).\displaystyle{\cal P}_{\uparrow\downarrow(\uparrow\uparrow)}(\gamma)=\int^{1}_{-1}dz~\rho_{\uparrow\downarrow(\uparrow\uparrow)}(\gamma,z)\,. (23)

with ξ=(1z)/2\xi=(1-z)/2.

Table 2: The chosen masses, MM, of the 00^{-} bound-system (in unit of the IR mass (0)=0.344{\cal M}(0)=0.344 GeV) are presented along with the coupling constants α=g2/4π\alpha=g^{2}/4\pi and the percentages of the spin configurations in the valence wave function. Recall that in addition to MM the set of model parameters is completed by : i) the gluon mass μ/(0)=1.363\mu/\mathscr{M}(0)=1.363, ii) a the vertex parameter Λ/(0)=0.291\Lambda/\mathscr{M}(0)=0.291 and iii) λ/(0)=2.616\lambda/\mathscr{M}(0)=2.616 (see Eq. (8)). For each MM, the first line represents the dressed case, while the second line is the undressed one with a quark mass equal to 0.3440.344\,GeV.
M/(0){M}/{{\cal M}(0)} g2g^{2} α\alpha P(%)P_{\uparrow\downarrow}(\%) P(%)P_{\uparrow\uparrow}(\%)
1.9 7.62 0.61 93 7
3.76 0.30 96 4
1.6 12.46 0.99 93 7
11.29 0.90 93 7
1.5 14.13 1.12 93 7
13.67 1.09 93 7
1.4 15.78 1.26 94 6
15.93 1.27 93 7
1.3 17.38 1.38 94 6
18.07 1.44 93 7
1.2 18.93 1.51 94 6
20.06 1.60 93 7

Table 2, for given values of MM, μ\mu and Λ\Lambda shows some outputs of our calculations: coupling constant and percentages of the spin configurations in the valence wave function. In general, the pattern for running and fixed mass cases is the expected one: when the mass of the system decreases the coupling constant increases. Loosely speaking, if the binding energy, i.e. the difference between the bound-system mass, MM, and some typical constituent mass increases also the depth of the well does. Heuristically, by defining the binding energy as B=2mqMB=2m_{q}-M where mqm_{q} is an effective quark mass, one can choose mq=(0)m_{q}=\mathscr{M}(0), for the fixed mass case, while one necessarily has mq=m¯(0)m_{q}=\bar{m}\leq\mathscr{M}(0), for the running mass one. In the latter case, the effective mass m¯\bar{m} stems from the suitable combination of the mass function, shown in the upper panel of Fig. 1, and the quark momentum-distribution, dictated by the BSE. Hence, one expects a decreasing m¯\bar{m} when the binding increases, since the system shrinks and the momentum-distribution tail grows, emphasizing the small mass region in (p2){\cal M}(p^{2}). In conclusion for given MM, the coupling constant for the running-mass case is larger than the one for the fixed-mass case and increases more slowly (m¯\bar{m} saturates to some value in the IR region).

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Figure 2: Longitudinal momentum distributions defined in Eqs. (20) and (22), with Λ=0.1\Lambda=0.1\,GeV and μ=0.469\mu=0.469\,GeV. Thick solid line: running mass model for M=0.653M=0.653\,GeV. Thin solid line: the same as the thick one, but for M=0.447M=0.447\,GeV. Thick dashed Line: fixed quark mass equal to 0.3440.344\,GeV and M=0.653M=0.653\,GeV. Thin dashed line: the same as the thick one, but for M=0.447M=0.447\,GeV. Dotted line: the same as the thick one, but for M=mπ=0.141M=m_{\pi}=0.141\,GeV.
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Figure 3: Transverse momentum distributions defined in Eqs. (21) and (23), with Λ=0.1\Lambda=0.1\,GeV and μ=0.469\mu=0.469\,GeV. The legend of the lines is the same as in Fig. 2.

Table 2 also shows the relative weight in the valence state between the anti-aligned spin component, which is dominant (recall that one has an orbital-angular momentum equal to 0 for a spin singlet), and the aligned spin component. On the spanned range of the mass MM, the two spin configurations keep almost the same percentage for both running and fixed quark masses. This could be interpreted as a feature dictated by the adopted interaction kernel.

In Figs. 2 and 3, the longitudinal and transverse distributions for the two examples of M/(0)=1.9M/{\cal M}(0)=1.9 and 1.31.3 are shown for the momentum-dependent dressed case (solid lines) and the undressed one (dashed lines).

As shown in Fig. 2, for the largest value of the system mass, M/(0)=1.9M/{\cal M}(0)=1.9, the total longitudinal distribution for the fixed-mass case is narrower than the running-mass one, implying that it decreases faster when approaching the end-points. Such a property can be understood by smaller value of the coupling constant (cf. the first two lines in Table 2) that leads to a larger size of the system and hence a smaller average relative momentum. Independently of the dressing of the quarks and bound state mass, the aligned longitudinal momentum distribution is broader than the anti-aligned one due to the relativistic nature of the former. For M/(0)=1.3M/{\cal M}(0)=1.3, the running mass-case and the fixed-mass one yield similar results, as one could expect given the similar values of the corresponding coupling constants (cf. Table 2).

The transverse distributions in Fig. 3 show that the dressing of the quark-propagator generates a larger momentum tail than in the undressed case, regardless of the spin component, but it decreases when the mass-system does. Moreover, the effect of the dressed quark-gluon vertex is manifested in the damping of the kernel at a scale of Λ2/2(0)γ/2(0)0.1\Lambda^{2}/\mathscr{M}^{2}(0)\sim\gamma/\mathscr{M}^{2}(0)\sim 0.1, as clearly recognized in the plots for the larger binding corresponding to M/(0)=1.3M/\mathscr{M}(0)=1.3 in both dressed and undressed quark cases. Finally, one should notice that the aligned transverse distribution vanishes for γ=0\gamma=0, as expected for an orbital-angular momentum L=1L=1 component. The insets in Fig. 3 show the tail of the transverse distributions which acquire a close functional dependence on γ\gamma, as it is expected, once the dressed and undressed propagators for large momentum are dominated by their gluon component and tend to be identical (cf. bottom panel of Fig. 1).

Summary. We have solved the 00^{-} homogeneous Bethe-Salpeter equation in Minkowski space by using i) the NIR of the BS amplitude; ii) an extended interaction kernel based on the ladder exchange of massive gluons, in the Feynman gauge, and iii) a phenomenologically dressed quark propagator, already adopted in Ref. [23]. The quark-mass function has only one adjusted parameter that was tuned on LQCD calculations of the running mass in Ref. [32]. It has been chosen a gluon mass close to 2ΛQCD2\Lambda_{QCD} and an extended color density with size 2\sim 2\,fm, that enforces the gluonic content of the bound system. The explored range of the system mass was 3mπ<M<5mπ3m_{\pi}<M<5m_{\pi}, and we obtained both static (cf. Table 2) and dynamical (cf. figs. 2 and 3) quantities. The main features have been discussed and heuristically interpreted, in order to enhance our physical intuition of the outcomes of our approach, that soon will be extended to the realistic case of the pion. In particular, we stressed the role of the interplay between three gluonic phenomena: dressing of the quark propagator, extension of the quark-gluon vertex and ladder exchange of massive gluons. For instance, we found that the quark dressing widens the transverse momentum distribution when compared to the case of the undressed quark tuned to have the IR mass, and interestingly, the aligned spin component of the valence wave function is suppressed with respect to the anti-aligned one, regardless of whether a running quark-mass is used or not, pointing to a ladder kernel effect.

Plainly, the present application of our approach based on the BSE plus a phenomenological running quark-mass should be considered as an initial step towards a description of the strongly-bound pion within a more consistent framework, based on realistic solutions of the quark gap-equation able to yield (p2){\cal M}(p^{2}) directly in Minkowski space (see also, e.g., Refs. [33, 34, 35, 36, 37, 38, 39, 40]).

A. C. gratefully thank INFN Sezione di Roma for providing the computer resources to perform all the calculations shown in this work. W. d. P. acknowledges the partial support of CNPQ under Grants No. 313030/2021-9 and the partial support of CAPES under Grant No. 88881.309870/2018-01. T. F. thanks the financial support from the Brazilian Institutions: CNPq (Grant No. 308486/2015-3), CAPES (Finance Code 001) and FAPESP (Grants No. 2017/05660-0 and 2019/07767-1). E. Y. acknowledges the support of FAPESP Grants No. 2016/25143-7 and No. 2018/21758-2. This work is a part of the project Instituto Nacional de Ciência e Tecnologia - Física Nuclear e Aplicações Proc. No. 464898/2014-5.

References