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Spinor-helicity representations of
(A)dS4 particles of any mass

Thomas Basile     Euihun Joung     Karapet Mkrtchyan     Matin Mojaza111Matin Mojaza contributed to this work while working at AEI Potsdam until September 2022.
Abstract

The spinor-helicity representations of massive and (partially-)massless particles in four dimensional (Anti-) de Sitter spacetime are studied within the framework of the dual pair correspondence. We show that the dual groups (aka “little groups”) of the AdS and dS groups are respectively O(2N)O(2N) and O(2N)O^{*}(2N). For N=1N=1, the generator of the dual algebra 𝔰𝔬(2)𝔰𝔬(2)𝔲(1)\mathfrak{so}(2)\cong\mathfrak{so}^{*}(2)\cong\mathfrak{u}(1) corresponds to the helicity operator, and the spinor-helicity representation describes massless particles in (A)dS4. For N=2N=2, the dual algebra is composed of two ideals, 𝔰\mathfrak{s} and 𝔪Λ\mathfrak{m}_{\Lambda}. The former ideal 𝔰𝔰𝔬(3)\mathfrak{s}\cong\mathfrak{so}(3) fixes the spin of the particle, while the mass is determined by the latter ideal 𝔪Λ\mathfrak{m}_{\Lambda}, which is isomorphic to 𝔰𝔬(2,1)\mathfrak{so}(2,1), 𝔦𝔰𝔬(2)\mathfrak{iso}(2) or 𝔰𝔬(3)\mathfrak{so}(3) depending on the cosmological constant being positive, zero or negative. In the case of a positive cosmological constant, namely dS4, the spinor-helicity representation contains all massive particles corresponding to the principal series representations and the partially-massless particles corresponding to the discrete series representations leaving out only the light massive particles corresponding to the complementary series representations. The zero and negative cosmological constant cases, which had been addressed in earlier references, are also discussed briefly. Finally, we consider the multilinear form of helicity spinors invariant under (A)dS group, which can be served for the (A)dS counterpart of the scattering amplitude, and discuss technical differences and difficulties of the (A)dS cases compared to the flat spacetime case.

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Imperial-TP-KM-2024-01

1 Introduction

The massless spinor-helicity (SH) representation in flat spacetime (Mink4) has proven very effective in expressing and determining scattering amplitudes (see e.g. [1, 2, 3, 4] for reviews) and their massive counterpart is also prevalent in recent time (see [5, 6] and [7, 8], and more). Moreover, several attempts to generalize it to (Anti)-de Sitter spaces ((A)dS4) were undertaken in the literature (see e.g. [9, 10, 11] for dS4 and [12, 13, 14] for AdS4). In the latter series of references [12, 13, 14], the Mink4 SH representation is deformed to (A)dS4 ones with a term in translation generators proportional to the cosmological constant. Despite this deformation, the main salient structure of the scattering amplitude remains the same, while only the momentum conservation delta function is modified to a Λ\Lambda-dependent function.

In this paper, we generalize the (A)dS4 SH representation used in [9, 12, 10, 13, 14] to include massive and partially-massless cases and carefully analyze their irreducible representation (irrep) content. Our analysis is systematic, using the reductive dual pair correspondence [15, 16] (see [17, 18, 19] for physics-oriented reviews, and [20, 21, 22, 23] for mathematics-oriented ones), the adequate mathematical framework responsible for most of the technical successes, yet always behind the curtain in the physicists’ treatments of the subject.

We show that the dual groups of the AdS4 and dS4 groups are respectively O(2N)O(2N) and O(2N)O^{*}(2N). For the N=1N=1 case, the generator of the dual algebra 𝔰𝔬(2)𝔰𝔬(2)𝔲(1)\mathfrak{so}(2)\cong\mathfrak{so}^{*}(2)\cong\mathfrak{u}(1) corresponds to the standard helicity operator of the SH formalism, and the SH representation describes massless fields222The SH representations describe single-particle states, but we will use the term “field” and “particle” interchangeably, as the most relevant context is scattering amplitudes in quantum field theory. in (A)dS4. For the N=2N=2 case, the dual algebra is composed of two ideals, 𝔰\mathfrak{s} and 𝔪Λ\mathfrak{m}_{\Lambda}. The former ideal 𝔰𝔰𝔬(3)\mathfrak{s}\cong\mathfrak{so}(3) fixes the spin of the (A)dS field, while the mass of the field is determined by the latter ideal 𝔪Λ\mathfrak{m}_{\Lambda}, which is isomorphic to 𝔰𝔬(1,2)\mathfrak{so}(1,2), 𝔦𝔰𝔬(2)\mathfrak{iso}(2) or 𝔰𝔬(3)\mathfrak{so}(3) depending on the cosmological constant being positive, zero, or negative. In the case of positive cosmological constant, namely dS4, the SH representation contains all massive fields corresponding to the principal series representations of 𝔰𝔬(1,4)\mathfrak{so}(1,4) and the partially-massless fields corresponding to the discrete series representations of 𝔰𝔬(1,4)\mathfrak{so}(1,4). The only irreps left out are the light massive fields corresponding to the complementary series representations of 𝔰𝔬(1,4)\mathfrak{so}(1,4). We also comment on the Mink4 and the AdS4 case, analyzed in earlier literature. The Mink4 case was analyzed in details in the earlier work [6] of the two of the authors. See also more widely known later work [7]. The AdS4 case was analyzed in [19] in terms of creation/annihilation operators. We also briefly comment on the dual pairs responsible for the SH representations of (A)dS particles in other dimensions.

Remark that the dual group is also known as “little group”. This terminology is misleading because the dual group differs from the little group of the induced representation à la Wigner: the actual little group is a subgroup of Lorentz, while the dual group commutes with the Lorentz. See the Appendix of [6] for the explicit comparison between the little group and dual group in the case of Poincaré algebra.

Finally, we consider the multilinear form of helicity spinors invariant under (A)dS4 group, which can be used for the (A)dS counterpart of the scattering amplitude. Despite the similarity with the Mink4 case, we find a few technical differences and difficulties in the (A)dS4 cases. We discuss these points and propose potential resolutions.

2 Spinor-helicity Representations of (A)dS fields

The SH representation of massive Mink4 fields [6, 7] and that of massless (A)dS4 fields [9, 12, 13, 14] admit a common and simple generalization,

Pab˙=λIλ~Ib˙a+ΛλIaλ~Ib˙,P_{a\dot{b}}=\lambda^{I}{}_{a}\,\tilde{\lambda}_{I\,\dot{b}}+\Lambda\,\frac{\partial}{\partial\lambda^{I\,a}}\frac{\partial}{\partial\tilde{\lambda}_{I}{}^{\dot{b}}}\,, (2.1)
Lab=2iλIλIb)(a,L~a˙b˙=2iλ~I(a˙λ~Ib˙),L_{ab}=2\,i\,\lambda^{I}{}_{(a}\,\frac{\partial}{\partial\lambda^{I\,b)}}\,,\qquad\tilde{L}_{\dot{a}\dot{b}}=2\,i\,\tilde{\lambda}_{I(\dot{a}}\,\frac{\partial}{\partial\tilde{\lambda}_{I}{}^{\dot{b})}}\,, (2.2)

where I=1,,NI=1,\ldots,N , and the N=1N=1 case corresponds to the massless case and the Λ=0\Lambda=0 limit corresponds to Mink4 case. Here, λ~Ia˙\tilde{\lambda}_{I\dot{a}} is the complex-conjugate of λIa\lambda^{I}{}_{a} for real “momenta”. Round brackets indicate symmetrization with weight one. Both of the indices a,ba,b and a˙,b˙\dot{a},\dot{b} are raised and lowered by the two-dimensional Levi–Civita tensor.333We follow notations and conventions of [6] with (σμ)ab˙=(1,σ)ab˙,(σ¯μ)a˙b=ϵa˙d˙ϵbc(σμ)cd˙=(1,σ)a˙b,\left(\sigma^{\mu}\right)_{a\dot{b}}=\left(1,\vec{\sigma}\right)_{a\dot{b}}\,,\qquad\left(\bar{\sigma}^{\mu}\right)^{\dot{a}b}=\epsilon^{\dot{a}\dot{d}}\,\epsilon^{bc}\,\left(\sigma^{\mu}\right)_{c\dot{d}}=\left(1,-\vec{\sigma}\right)^{\dot{a}b}\,, (2.3) where σi\sigma^{i}, i=1,2,3i=1,2,3, are the usual Pauli matrices, which verify (σμ)aa˙(σμ)bb˙=2ϵaa˙ϵbb˙(\sigma^{\mu})_{a\dot{a}}\,(\sigma_{\mu})_{b\dot{b}}=-2\,\epsilon_{a\dot{a}}\,\epsilon_{b\dot{b}}, and (σμν)a=b14(σμσ¯νσνσ¯μ)a,b(σ¯μν)a˙=b˙14(σ¯μσνσ¯νσμ)a˙.b˙(\sigma^{\mu\nu})_{a}{}^{b}=\frac{1}{4}\,(\sigma^{\mu}\,\bar{\sigma}^{\nu}-\sigma^{\nu}\,\bar{\sigma}^{\mu})_{a}{}^{b}\,,\qquad(\bar{\sigma}^{\mu\nu})^{\dot{a}}{}_{\dot{b}}=-\frac{1}{4}\,(\bar{\sigma}^{\mu}\,\sigma^{\nu}-\bar{\sigma}^{\nu}\,\sigma^{\mu})^{\dot{a}}{}_{\dot{b}}\,. (2.4) Indices are raised and lowered via ψa=ϵabψb,ψa=ϵabψb,ϵacϵcb=δba,\psi_{a}=\epsilon_{ab}\,\psi^{b}\,\,,\quad\psi^{a}=\epsilon^{ab}\,\psi_{b}\,,\quad\quad\epsilon^{ac}\,\epsilon_{cb}=\delta^{a}_{b}\,, (2.5) and similarly for dotted indices. We shall denote this (A)dS4 isometry algebra as 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda}. It is straightforward to check that the commutators of the above operators satisfy the Lie brackets of the (A)dS4 algebra with cosmological constant Λ\Lambda: the generators LabL_{ab} and L~a˙b˙=Lab\tilde{L}_{\dot{a}\dot{b}}=L_{ab}{}^{\dagger} form standard Lorentz subalgebra 𝔰𝔬(1,3)𝔰𝔩(2,)\mathfrak{so}(1,3)\cong\mathfrak{sl}(2,\mathbb{C}) with [Lab,L~c˙d˙]=0[L_{ab},\tilde{L}_{\dot{c}\dot{d}}]=0 and

[Lab,Lcd]=i(ϵacLbd+ϵbcLad+ϵadLbc+ϵbdLac).\displaystyle[L_{ab},L_{cd}]=-i\,(\epsilon_{ac}\,L_{bd}+\epsilon_{bc}\,L_{ad}+\epsilon_{ad}\,L_{bc}+\epsilon_{bd}\,L_{ac})\,. (2.6)

The translation generators Pab˙P_{a\dot{b}} carry a vector representation of 𝔰𝔬(1,3)\mathfrak{so}(1,3), that is a bifundamental representation of 𝔰𝔩(2,)\mathfrak{sl}(2,\mathbb{C}),

[Lab,Pcd˙]=i(ϵcaPbd˙+ϵcbPad˙),[L~a˙b˙,Pcd˙]=i(ϵd˙a˙Pcb˙+ϵd˙b˙Pca˙).[L_{ab},P_{c\dot{d}}]=i\,(\epsilon_{ca}\,P_{b\dot{d}}+\epsilon_{cb}\,P_{a\dot{d}})\,,\qquad[\tilde{L}_{\dot{a}\dot{b}},P_{c\dot{d}}]=i\,(\epsilon_{\dot{d}\dot{a}}\,P_{c\dot{b}}+\epsilon_{\dot{d}\dot{b}}\,P_{c\dot{a}})\,. (2.7)

With the cosmological constant Λ\Lambda, the translation generators no longer commute but satisfy

[Pab˙,Pcd˙]=iΛ(ϵacL~b˙d˙+ϵb˙d˙Lac).[P_{a\dot{b}},P_{c\dot{d}}]=i\,\Lambda\,(\epsilon_{ac}\,\tilde{L}_{\dot{b}\dot{d}}+\epsilon_{\dot{b}\dot{d}}\,L_{ac})\,. (2.8)

Hence, we find 𝔰𝔶𝔪Λ𝔰𝔬(1,4)\mathfrak{sym}_{\Lambda}\simeq\operatorname{\mathfrak{so}}(1,4) for Λ>0\Lambda>0 and 𝔰𝔶𝔪Λ𝔰𝔬(2,3)\mathfrak{sym}_{\Lambda}\simeq\operatorname{\mathfrak{so}}(2,3) for Λ<0\Lambda<0 .444 Note here that Λ\Lambda is related to the actual cosmological constant Λcc\Lambda_{cc} by Λcc=3Λ\Lambda_{cc}=3\,\Lambda.

The (A)dS4 algebra 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} is a subalgebra of 𝔰𝔭(8N,)\operatorname{\mathfrak{sp}}(8N,\mathbb{R}) generated by all bilinears in λaI\lambda^{I}_{a}, λaI\frac{\partial}{\partial\lambda^{I}_{a}} and their complex conjugates. The dual algebra, denoted by 𝔡𝔲𝔞𝔩Λ(N)\mathfrak{dual}^{(N)}_{\Lambda}, is the stabiliser of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} within 𝔰𝔭(8N,)\operatorname{\mathfrak{sp}}(8N,\mathbb{R}), and is generated by

KI=JλIλJaaλ~Ja˙λ~Ia˙,K^{I}{}_{J}=\lambda^{I}{}_{a}\,\frac{\partial}{\partial\lambda^{J}{}_{a}}-\tilde{\lambda}_{J\dot{a}}\,\frac{\partial}{\partial\tilde{\lambda}_{I\,\dot{a}}}\,, (2.9a)
MIJ=λIλJaaΛλ~Ia˙λ~Ja˙,M~IJ=λ~Ia˙λ~Ja˙ΛλIaλJa.M^{IJ}=\lambda^{I}{}_{a}\,\lambda^{Ja}-\Lambda\,\frac{\partial}{\partial\tilde{\lambda}_{I}{}^{\dot{a}}}\frac{\partial}{\partial\tilde{\lambda}_{J\,\dot{a}}}\,,\qquad\tilde{M}_{IJ}=\tilde{\lambda}_{I\dot{a}}\,\tilde{\lambda}_{J}{}^{\dot{a}}-\Lambda\,\frac{\partial}{\partial\lambda^{I\,a}}\frac{\partial}{\partial\lambda^{J}{}_{a}}\,. (2.9b)

The SH representation of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} is reducible and its decomposition into irreps can be carried out on the side of 𝔡𝔲𝔞𝔩Λ(N)\mathfrak{dual}_{\Lambda}^{(N)}. In the following, we shall identify the dual algebra 𝔡𝔲𝔞𝔩Λ(N)\mathfrak{dual}^{(N)}_{\Lambda} and explain the intimate relation between 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} and 𝔡𝔲𝔞𝔩Λ(N)\mathfrak{dual}^{(N)}_{\Lambda}, first through a preliminary analysis on the eigenvalues of Casimir operators, then using the more solid and powerful method of the dual pair correspondence.

3 Preliminary analysis

In this section, we identify the dual algebra 𝔡𝔲𝔞𝔩Λ(N)\mathfrak{dual}^{(N)}_{\Lambda} for N=1,2N=1,2, and establish its relation to 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} at the level of Casimir operators. By comparing the eigenvalues of the Casimir operators of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} and 𝔡𝔲𝔞𝔩Λ(N)\mathfrak{dual}^{(N)}_{\Lambda}, we provide a preliminary assessment of the correspondence between the irreps of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} and 𝔡𝔲𝔞𝔩Λ(N)\mathfrak{dual}^{(N)}_{\Lambda} .

3.1 N=1N=1

In the N=1N=1 case, considered in [12, 13, 14], the dual algebra 𝔡𝔲𝔞𝔩Λ(1)\mathfrak{dual}^{(1)}_{\Lambda} is simply isomorphic to 𝔲(1)\mathfrak{u}(1) generated by

K=λaλaλ~a˙λ~a˙,K=\lambda_{a}\,\frac{\partial}{\partial\lambda_{a}}-\tilde{\lambda}_{\dot{a}}\,\frac{\partial}{\partial\tilde{\lambda}_{\dot{a}}}\,, (3.1)

which is nothing but the standard helicity operator. The K=sK=s state describes massless helicity ss representations in Mink4, AdS4 and dS4. This universal description is due to the conformal symmetry they enjoy: the SH representations of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} can be lifted to a single irreducible representation, typically referred to as ‘singleton’, of the four-dimensional conformal group 𝔰𝔬(2,4)\operatorname{\mathfrak{so}}(2,4) [24, 25, 26, 27] (see also [28, 29, 30] for the oscillator realization, where sometimes the representation is referred to as ‘doubleton’ for a historical reason). This special property of singleton can be easily understood in terms of the dual pair correspondence, as it was shown in [19]. We shall come back to this point in Section 4.3.

3.2 N=2N=2

The N=2N=2 case will turn out to be sufficient to describe all massive spin representations in four dimensions. The generators M=M12M=M^{12} and M~=M~12\tilde{M}=\tilde{M}_{12} commute with the subalgebra 𝔰𝔬(3)𝔰𝔲(2)𝔲(2)\operatorname{\mathfrak{so}}(3)\simeq\operatorname{\mathfrak{su}}(2)\subset\operatorname{\mathfrak{u}}(2) generated by 𝒦I=JKIJ12δJIKKK{\cal K}^{I}{}_{J}=K^{I}{}_{J}-\frac{1}{2}\,\delta^{I}_{J}\,K^{K}{}_{K} while the 𝔲(1)\operatorname{\mathfrak{u}}(1) part K=KIIK=K^{I}{}_{I} satisfies

[M,M~]=ΛK,[K,M]=2M,[K,M~]=2M~.[M,\tilde{M}]=-\Lambda\,K,\qquad[K,M]=2\,M\,,\qquad[K,\tilde{M}]=-2\,\tilde{M}\,. (3.2)

Taking into account that M=M~M^{\dagger}=\tilde{M} and K=KK^{\dagger}=K,555Note that the Hermitian conjugation \dagger is defined with respect to the L2(2N)L^{2}(\mathbb{C}^{2N}) norm, and hence λI=a(λI)a=λ~Ia˙\lambda^{I}{}_{a}{}^{\dagger}=(\lambda^{I}{}_{a})^{*}=\tilde{\lambda}_{I\,\dot{a}} and (/λI)a=/λ~Ia˙(\partial/\partial\lambda^{I}{}_{a})^{\dagger}=-\partial/\partial\tilde{\lambda}_{I\,\dot{a}}. it is easy to show that the Hermitian generators 12K\frac{1}{2}\,K, 12(M+M~)\frac{1}{2}\,(M+\tilde{M}) and i2(MM~)\frac{i}{2}\,(M-\tilde{M}) form 𝔰𝔬(2,1)\operatorname{\mathfrak{so}}(2,1) for Λ>0\Lambda>0, 𝔰𝔬(3)\operatorname{\mathfrak{so}}(3) for Λ<0\Lambda<0 and 𝔦𝔰𝔬(2)\operatorname{\mathfrak{iso}}(2) for Λ=0\Lambda=0. The last case corresponds to the massive Mink4 SH formulation [6, 7]. To summarize, we find that for N=2N=2, the dual algebra is the direct sum,

𝔡𝔲𝔞𝔩Λ(2)𝔰𝔪Λ,\mathfrak{dual}^{(2)}_{\Lambda}\simeq\mathfrak{s}\oplus\mathfrak{m}_{\Lambda}\,, (3.3)

where the two ideals 𝔰\mathfrak{s} and 𝔪Λ\mathfrak{m}_{\Lambda} are

𝔰=𝔰𝔬(3),𝔪Λ={𝔰𝔬(2,1)[Λ>0]𝔰𝔬(3)[Λ<0]𝔦𝔰𝔬(2)[Λ=0].\mathfrak{s}=\mathfrak{so}(3)\,,\quad\mathfrak{m}_{\Lambda}=\left\{\begin{aligned} &\mathfrak{so}(2,1)\quad&[\Lambda>0]\\ &\mathfrak{so}(3)\quad&[\Lambda<0]\\ &\mathfrak{iso}(2)\quad&[\Lambda=0]\end{aligned}\right.. (3.4)

Below, we will show that the common ideal 𝔰\mathfrak{s} for any Λ\Lambda is responsible for the spin label of the 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} irreps, whereas the other subalgebra 𝔪Λ\mathfrak{m}_{\Lambda} determines the mass. In order to see this identification, let us first exploit the relations between Casimir operators of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} and 𝔡𝔲𝔞𝔩Λ(2)\mathfrak{dual}^{(2)}_{\Lambda}.

Since 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} is a rank two Lie algebra 𝔰𝔬(1,4)\mathfrak{so}(1,4) or 𝔰𝔬(2,3)\mathfrak{so}(2,3) for Λ0\Lambda\neq 0, there are two independent Casimir operators: the quadratic and quartic ones, whose expressions in vector notation read

C2(𝔰𝔶𝔪Λ)=12JA1JA2A2,A1\displaystyle C_{2}(\mathfrak{sym}_{\Lambda})=-\frac{1}{2}\,J^{A_{1}}{}_{A_{2}}\,J^{A_{2}}{}_{A_{1}}\,, (3.5a)
C4(𝔰𝔶𝔪Λ)=12WAWA,WA=12ϵABCDEJBCJDE,\displaystyle C_{4}(\mathfrak{sym}_{\Lambda})=\frac{1}{2}\,W_{A}\,W^{A}\,,\qquad W_{A}=\frac{1}{2}\,\epsilon_{ABCDE}\,J^{BC}\,J^{DE}\,, (3.5b)

where the capital indices take the values A,B,=0,1,,4A,B,\dots=0,1,\dots,4 and JAB=JBAJ_{AB}=-J_{BA} are the generators of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda}. Splitting JABJ_{AB} into Lorentz and translation generators as J4μ=Pμ/|Λ|J_{4\mu}=P_{\mu}/\sqrt{|\Lambda|} and Jμν=LμνJ_{\mu\nu}=L_{\mu\nu}, the two Casimirs are

C2(𝔰𝔶𝔪Λ)\displaystyle C_{2}(\mathfrak{sym}_{\Lambda}) =\displaystyle= 12ΛP2+14(L2+L~2),\displaystyle-\frac{1}{2\,\Lambda}\,P^{2}+\frac{1}{4}\,(L^{2}+\tilde{L}^{2})\,, (3.6a)
C4(𝔰𝔶𝔪Λ)\displaystyle C_{4}(\mathfrak{sym}_{\Lambda}) =\displaystyle= 14ΛPaa˙Pbb˙LabL~a˙b˙+116ΛP2(L2+L~2)\displaystyle\frac{1}{4\,\Lambda}\,P^{a\dot{a}}\,P^{b\dot{b}}\,L_{ab}\,\tilde{L}_{\dot{a}\dot{b}}+\frac{1}{16\,\Lambda}\,P^{2}\,(L^{2}+\tilde{L}^{2}) (3.6b)
14(L2+L~2)164(L2L~2)2.\displaystyle-\,\frac{1}{4}\,(L^{2}+\tilde{L}^{2})-\frac{1}{64}\,(L^{2}-\tilde{L}^{2})^{2}\,.

Here, P2=Pab˙Pab˙=2PμPμP^{2}=P_{a\dot{b}}\,P^{a\dot{b}}=-2\,P_{\mu}P^{\mu}, L2=LabLabL^{2}=L_{ab}L^{ab} and LμνLμν=12(L2+L~2)L_{\mu\nu}L^{\mu\nu}=\frac{1}{2}(L^{2}+\tilde{L}^{2}), where we use the mostly-plus signature for ημν\eta_{\mu\nu}. Note that ΛC2(𝔰𝔶𝔪Λ)\Lambda\,C_{2}(\mathfrak{sym}_{\Lambda}) and ΛC4(𝔰𝔶𝔪Λ)\Lambda\,C_{4}(\mathfrak{sym}_{\Lambda}) reproduce the familiar quadratic Casimir and the Pauli–Lubański vector squared in the Λ0\Lambda\to 0 limit.

On the other hand, the dual algebra is composed of two rank-one ideals, so we have one Casimir operator for each:

C2(𝔰)\displaystyle C_{2}(\mathfrak{s}) =\displaystyle= 12𝒦JI𝒦IJ,\displaystyle\frac{1}{2}{\cal K}^{I}_{J}\,{\cal K}^{J}_{I}\,, (3.7)
C2(𝔪Λ)\displaystyle C_{2}(\mathfrak{m}_{\Lambda}) =\displaystyle= 12Λ{M,M~}+14K2.\displaystyle-\frac{1}{2\Lambda}\,\{M,\tilde{M}\}+\frac{1}{4}\,K^{2}\,. (3.8)

The SH representation of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} (2.1) and (2.2) and that of 𝔡𝔲𝔞𝔩Λ(2)\mathfrak{dual}^{(2)}_{\Lambda} (2.9a) and (2.9b) relate these Casimir operators as

C2(𝔰𝔶𝔪Λ)\displaystyle C_{2}(\mathfrak{sym}_{\Lambda}) =\displaystyle= C2(𝔪Λ)+C2(𝔰)2,\displaystyle C_{2}(\mathfrak{m}_{\Lambda})+C_{2}(\mathfrak{s})-2\,, (3.9a)
C4(𝔰𝔶𝔪Λ)\displaystyle C_{4}(\mathfrak{sym}_{\Lambda}) =\displaystyle= C2(𝔪Λ)C2(𝔰).\displaystyle-\,C_{2}(\mathfrak{m}_{\Lambda})\,C_{2}(\mathfrak{s})\,. (3.9b)

From the above relations, we can read off the Casimir eigenvalues of the unitary irreps of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} by fixing an irrep of 𝔡𝔲𝔞𝔩Λ(2)𝔰𝔪Λ\mathfrak{dual}^{{(2)}}_{\Lambda}\simeq\mathfrak{s}\oplus\mathfrak{m}_{\Lambda}. For the ideal 𝔰𝔰𝔬(3)\mathfrak{s}\simeq\mathfrak{so}(3), the (2s+1)(2s+1)-dimensional irreps with

C2(𝔰)=s(s+1),C_{2}(\mathfrak{s})=s(s+1)\,, (3.10)

account for all unitary irreps. About the ideal 𝔪Λ\mathfrak{m}_{\Lambda}, the quadratic Casimir operator can be parameterized as

C2(𝔪Λ)=μ(μ+1),C_{2}(\mathfrak{m}_{\Lambda})=\mu(\mu+1)\,, (3.11)

which is invariant under

μ1μ,\mu\to-1-\mu, (3.12)

and we have the following options:

  • For Λ>0\Lambda>0, apart from the trivial irrep with μ(μ+1)=0\mu(\mu+1)=0, we have three series of unitary irreps for 𝔰𝔬(2,1)\mathfrak{so}(2,1) :

    • The principal series irreps 𝒞μ±{\cal C}_{\mu}^{\pm} with complex μ\mu satisfying

      μ(μ+1)<14,\mu(\mu+1)<-\frac{1}{4}\,, (3.13)

      which is spanned by eigenstates of KK with even/odd integer eigenvalues, related to the label +/+/- respectively. We can parametrize irreps in this series via μ=12+iρ\mu=-\frac{1}{2}+i\,\rho with ρ\rho\in\mathbb{R}. In this case, the map (3.12), ρρ\rho\to-\rho, is an isomorphism, and hence we may restrict to the case ρ>0\rho>0.

    • The complementary series irrep 𝒞μ{\cal C}_{\mu} with 1<μ<0-1<\mu<0 satisfying

      14μ(μ+1)<0,-\frac{1}{4}\leq\mu(\mu+1)<0\,, (3.14)

      spanned by all even KK-eigenstates. The map (3.12) is again an isomorphism.

    • The positive/negative discrete series irrep 𝒟2μ+2±{\cal D}^{\pm}_{2\mu+2} with

      μ=12,0,12,1,32,,\mu=-\tfrac{1}{2},0,\tfrac{1}{2},1,\tfrac{3}{2},\ldots\,, (3.15)

      spanned by the KK-eigenstates with eigenvalues ±2(μ+1),±2(μ+2)\pm 2(\mu+1),\pm 2(\mu+2), etc. These are lowest/highest weight irreps.

  • For Λ0\Lambda\to 0 , the “bosonic/fermionic” irrep of 𝔦𝔰𝔬(2)\operatorname{\mathfrak{iso}}(2) with |μ||\mu|\to\infty while keeping finite

    m=Λμ2,m={\sqrt{-\Lambda\,\mu^{2}}}\,, (3.16)

    which is spanned by KK-eigenstates with even/odd eigenvalues. These irreps can be thought of as the counterpart of the massive scalar and spinor representations of the Poincaré group (depending on the parity of the KK-eigenstates).

    The trivial representation, with m=0m=0, and which can be thought of as the counterpart of the zero-momentum irrep of the Poincaré group.

  • For Λ<0\Lambda<0, the (2μ+1)(2\mu+1)-dimensional irrep of 𝔰𝔬(3)\operatorname{\mathfrak{so}}(3) with

    μ=0,12,1,32,,\mu=0,\tfrac{1}{2},1,\tfrac{3}{2},\ldots\,, (3.17)

    with basis composed of KK-eigenstates with eigenvalues 2μ,2μ+2,,+2μ-2\mu,-2\mu+2,\dots,+2\mu.

These irreps of 𝔡𝔲𝔞𝔩Λ(2)\mathfrak{dual}^{{(2)}}_{\Lambda} are in one-to-one correspondence with the irreps of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} with

C2(𝔰𝔶𝔪Λ)\displaystyle C_{2}(\mathfrak{sym}_{\Lambda}) =μ(μ+1)+s(s+1)2,\displaystyle=\mu(\mu+1)+s(s+1)-2\,, (3.18a)
C4(𝔰𝔶𝔪Λ)\displaystyle C_{4}(\mathfrak{sym}_{\Lambda}) =μ(μ+1)s(s+1),\displaystyle=-\mu(\mu+1)\,s(s+1)\,, (3.18b)

and we can compare these values with those of known irreps of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda}.

Mink4

To begin with, let us consider the Poincaré case with Λ=0\Lambda=0 which has been treated in [5, 7]. The quadratic Casimir,

limΛ0ΛC2(𝔪Λ)=MM~,\lim_{\Lambda\to 0}\Lambda\,C_{2}(\mathfrak{m}_{\Lambda})=-M\,\tilde{M}\,, (3.19)

of the dual algebra 𝔪0\mathfrak{m}_{0} determines the mass:

MM~=PμPμ=m2,M\,\tilde{M}=-P_{\mu}\,P^{\mu}=m^{2}\,, (3.20)

while the ‘spin ss’ representation of the dual algebra 𝔰\mathfrak{s} corresponds to the spin, thus defining a Poincaré representation of mass mm and spin ss . In fact, in all cases of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda}, the irrep label ss of the dual algebra 𝔰\mathfrak{s} simply corresponds to the spin of the four-dimensional field.

dS4

The unitary irreps of dS4 Lie algebra, namely 𝔰𝔬(1,4)\mathfrak{so}(1,4), were first classified in [31] where the eigenvalues of the Casimir operators are also given: see Appendix A for a summary, and [32] for the physical interpretations of these irreps. More recent treatments of dS representations can be found e.g. in [33, 34, 35, 36, 37, 38].

Comparing the result (3.18b) with the Casimir eigenvalues identified in [31], we find that the irrep label μ\mu of the dual algebra 𝔪Λ\mathfrak{m}_{\Lambda} parameterizes the mass squared as666Here, we define the mass m2m^{2} of a field φ\varphi of spin ss in (A)dSd+1 via the wave equation (2+2Λccd(d1)[(s2)(s+d2)s]m2)φ=0.\left(\nabla^{2}+\frac{2\,\Lambda_{cc}}{d(d-1)}\,\big{[}(s-2)(s+d-2)-s\big{]}-m^{2}\right)\varphi=0\,. Parameterizing the eigenvalue of the quadratic Casimir operator of the irrep associated with φ\varphi as C2=Δ(Δd)+s(s+d2),C_{2}=\Delta(\Delta-d)+s(s+d-2)\,, we can write the mass squared as m2=2Λccd(d1)(Δ+s2)(s+d2Δ),m^{2}=\frac{2\,\Lambda_{cc}}{d(d-1)}\,(\Delta+s-2)(s+d-2-\Delta)\,, which reproduces the formula (3.21) upon using μ=Δ2\mu=\Delta-2 (or μ=Δ+1\mu=-\Delta+1) for d=3d=3. (See for instance [39] for an extended discussion of the dS4 case, and [40, 41] including also the AdS4 case.)

m2=Λ[μ(μ+1)+s(s1)].m^{2}=\Lambda\,[-\mu(\mu+1)+s(s-1)]\,. (3.21)

Depending on the spin ss, different ranges of mass are allowed for the unitarity of the 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} irreps:

  • For the scalar case with s=0s=0, the allowed μ\mu are

    • The complex values of μ\mu with (3.13) corresponding to the principal series representations of 𝔰𝔬(1,4)\mathfrak{so}(1,4), with the isomorphism (3.12).

    • The real values of 2<μ<1-2<\mu<1 with

      14μ(μ+1)<2,-\frac{1}{4}\leq\mu(\mu+1)<2\,, (3.22)

      corresponding to the complementary series representations of 𝔰𝔬(1,4)\mathfrak{so}(1,4), with the isomorphism (3.12). The μ=0\mu=0 case (or equivalently, the μ=1\mu=-1 case) corresponds to the conformally coupled scalar.

    • The positive integer values of μ\mu corresponding to the discrete series representations of 𝔰𝔬(1,4)\mathfrak{so}(1,4). The μ=1\mu=1 case corresponds to the minimally coupled massless scalar, whereas μ=2,3,\mu=2,3,\ldots correspond to tachyonic scalars.

    The unitarity of these 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} irreps includes not only all the 𝔪Λ\mathfrak{m}_{\Lambda} unitary regions (3.13), (3.14) and the integer part of (3.15), but also the complementary series region 0<μ(μ+1)<20<\mu(\mu+1)<2 not allowed for the unitarity of 𝔪Λ\mathfrak{m}_{\Lambda} .

  • For integral spins s=1,2,s=1,2,\ldots, the allowed μ\mu are

    • The complex values with (3.13) corresponding to the principal series representations of 𝔰𝔬(1,4)\mathfrak{so}(1,4), with the isomorphism (3.12).

    • The real values of 1<μ<0-1<\mu<0 with (3.14) corresponding to the complementary series representations of 𝔰𝔬(1,4)\mathfrak{so}(1,4), with the isomorphism (3.12).

    • The integer values μ=0,1,,s1\mu=0,1,\ldots,s-1. These integer values correspond to the partially-massless fields of depth sμs-\mu, where the depth 1 corresponds to the massless field.

    The unitarity of these 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} irreps includes the 𝔪Λ\mathfrak{m}_{\Lambda} unitary regions (3.13) and (3.14), but restrict (3.15): any integers greater than s1s-1 are excluded together with the half-integer values.

  • For half-integral spins s=12,32,s=\frac{1}{2},\frac{3}{2},\ldots, the allowed μ\mu are

    • The complex values of μ\mu with (3.13) corresponding to the principal series representation of 𝔰𝔬(1,4)\mathfrak{so}(1,4), with the isomorphism (3.12).

    • The half integer values μ=12,12,,s1\mu=-\frac{1}{2},\frac{1}{2},\ldots,s-1 corresponding to the discrete series representations of 𝔰𝔬(1,4)\mathfrak{so}(1,4). The positive half-integer values correspond to the partially-massless fields of depth sμs-\mu.777The partially-massless fermion irreps are unitary only in dS4 [42]. Note that μ=12\mu=-\frac{1}{2} corresponds to the end point of the continuous spectrum of massive fields, which we may refer to as the lightest massive fermions. For s=12s=\frac{1}{2}, it simply corresponds to the massless spinor.

    The unitarity of these 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} irreps includes the 𝔪Λ\mathfrak{m}_{\Lambda} principal series (3.13) but entirely excludes the complementary series (3.14), and restrict the discrete series (3.15): any half-integers greater than s1s-1 are excluded together with the integer values.

AdS4

In the AdS4 case with Λ<0\Lambda<0, the irrep label μ\mu of the dual algebra 𝔪Λ\mathfrak{m}_{\Lambda} parameterizes the mass squared again as (3.21). The allowed μ\mu for the unitarity of the lowest-energy irreps of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} are μ=s1,s,s+1,\mu=s-1,s,s+1,\ldots for spin s=0,12 1,s=0,\frac{1}{2}\,1,\ldots. The μ=s1\mu=s-1 case corresponds to the massless spin ss field, and higher μ\mu cases correspond to massive fields. The reason that we have a discrete mass spectrum is due to the fact that μ\mu is an eigenvalue of the generator of the compact subgroup SO(2)SO(2) associated with rotations in the plane of temporal directions, and hence is quantized. These representations can be interpreted as the irreps of 3d conformal group: Δ=μ+2\Delta=\mu+2 and ss correspond to the conformal weight and spin of the conformal primaries, respectively. In the scalar case, the μ=1\mu=-1 and μ=0\mu=0 cases mapped by (3.12) are distinct irreps and correspond to different modes of the conformal scalar in AdS4. Note that, moving to a covering group of SO(1,4)SO(1,4), the point μ=32\mu=-\frac{3}{2} can be included for s=0s=0, and it corresponds to the conformal scalar in 3d.

The unitarity of the lowest energy irreps of 𝔰𝔶𝔪Λ𝔰𝔬(2,3)\mathfrak{sym}_{\Lambda}\cong\mathfrak{so}(2,3) excludes the lower μ\mu values with μ<s1\mu<s-1 from (3.17), corresponding to partially-massless fields, together with all integer/half-integer values of μ\mu for half-integral/integral spin.

Let us note that there are a few other types of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} irreps with unbounded energy. These irreps would cover different ranges of C2(𝔰𝔶𝔪Λ)C_{2}(\mathfrak{sym}_{\Lambda}) and C4(𝔰𝔶𝔪Λ)C_{4}(\mathfrak{sym}_{\Lambda}) .

4 Dual pair correspondence

In the previous section we have identified the correspondences between the irreps of 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} and those of 𝔡𝔲𝔞𝔩Λ(2)\mathfrak{dual}^{{(2)}}_{\Lambda} through the Casimir eigenvalues. We have observed that the region of μ\mu allowed by the 𝔰𝔶𝔪Λ\mathfrak{sym}_{\Lambda} unitarity does not match the region allowed by the 𝔪Λ\mathfrak{m}_{\Lambda} unitarity. This mismatch does not lead to a contradiction, because the SH representations cover only a part of unitary irreps of 𝔰𝔶𝔪Λ𝔡𝔲𝔞𝔩Λ(2)\mathfrak{sym}_{\Lambda}\oplus\mathfrak{dual}^{{(2)}}_{\Lambda}. In other words, the SH Fock space contains only a part of unitary irreps of 𝔰𝔶𝔪Λ𝔡𝔲𝔞𝔩Λ(2)\mathfrak{sym}_{\Lambda}\oplus\mathfrak{dual}^{{(2)}}_{\Lambda} . In order to identify the actual content of the unitary irreps that the Fock space contains, we need a more rigorous analysis using the dual pair correspondence.

For general NN, the dual algebras (2.9) are 𝔡𝔲𝔞𝔩Λ>0(N)𝔰𝔬(2N)\mathfrak{dual}^{{(N)}}_{\Lambda>0}\simeq\operatorname{\mathfrak{so}}^{*}(2N) and 𝔡𝔲𝔞𝔩Λ<0(N)𝔰𝔬(2N)\mathfrak{dual}^{{(N)}}_{\Lambda<0}\simeq\operatorname{\mathfrak{so}}(2N), respectively. The interplay between the isometry and the dual algebras can be understood within the general framework of the dual pair correspondence, aka Howe duality, which amounts to the following: when a Sp(2𝒩,)Sp(2{\cal N},\mathbb{R}) group contains a pair of reductive subgroups (G,G~)(G,\tilde{G}) which are mutual stabilisers, there exists a one-to-one correspondence between the irreps of GG and G~\tilde{G} appearing in the decomposition of the oscillator (or metaplectic) representation of Sp(2𝒩,)Sp(2{\cal N},\mathbb{R}) (see e.g. [19] for more details). In our context, the oscillator representation is simply the representation realized by the helicity spinors, or simply SH representation. Hence, the (A)dS4 groups 𝔖𝔶𝔪Λ>0=Sp(1,1)\mathfrak{Sym}_{\Lambda>0}=Sp(1,1) and 𝔖𝔶𝔪Λ<0=Sp(4,)\mathfrak{Sym}_{\Lambda<0}=Sp(4,\mathbb{R}) and their respective dual groups 𝔇𝔲𝔞𝔩Λ>0(N)=O(2N)\mathfrak{Dual}^{{(N)}}_{\Lambda>0}=O^{*}(2N) and 𝔇𝔲𝔞𝔩Λ<0(N)=O(2N)\mathfrak{Dual}^{(N)}_{\Lambda<0}=O(2N) realized by helicity spinors as (2.8) and (2.9) form reductive dual pairs in Sp(8N,)Sp(8N,\mathbb{R}), the group generated by all quadratic operators in helicity spinors and their derivatives. Note that Sp(1,1)Sp(1,1) and Sp(4,)Sp(4,\mathbb{R}) are isomorphic to the double covers of SO(1,4)SO^{\uparrow}(1,4) and SO(2,3)SO^{\uparrow}(2,3), respectively. In fact, the flat space case with Λ=0\Lambda=0 can be viewed as the Inönü–Wigner contraction of the reductive dual pair (Sp(1,1),O(2N))\big{(}Sp(1,1),O^{*}(2N)\big{)} or (Sp(4,),O(2N))\big{(}Sp(4,\mathbb{R}),O(2N)\big{)}.

Let us remark once again that the dual group ought not to be confused with the standard little group of the induced representation à la Wigner: the former commutes with the isometry whereas the latter is a part of the isometry by definition. In the Λ=0\Lambda=0 case, the SU(2)SU(2) subgroup of the dual group and the little group are explicitly shown to be distinguished (see the appendix of [6]) as they represent respectively left and right actions on SU(2)SU(2) which parameterizes a momentum eigenstate.

The dual pair correspondence assures that the irreps of the (A)dS4 group, that is Sp(1,1)Sp(1,1) and Sp(4,)Sp(4,\mathbb{R}), realized by helicity spinors are in one-to-one correspondence with the irreps of the dual group O(2N)O^{*}(2N) or O(2N)O(2N). In other words, by singling out an irrep of the dual group, the reducible SH representation of the (A)dS4 group (2.8) is restricted to an irrep. Then, the remaining task is to establish the dictionary between such irreps of the (A)dS4 group and its dual group O(2N)O^{*}(2N) (or O(2N)O(2N)). For that, we once again focus on the cases of N=1N=1 and 22.

4.1 dS4

Let us consider first the case with Λ>0\Lambda>0. Our aim is to obtain a dictionary between the irreps of Sp(1,1)Sp(1,1) and O(2N)O^{*}(2N) appearing in the decomposition of the SH representation.

For N=1N=1, the dual pair correspondence between Sp(1,1)Sp(1,1) and O(2)O^{*}(2) has been explicitly established in [19]. Here, we just quote the result. Since O(2)O^{*}(2) is isomorphic to U(1)U(1), it has only one-dimensional irreps, each labelled by an integer. This integer corresponds to twice the helicity of a Sp(1,1)Sp(1,1) massless representation. The analysis is based on the decomposition of the Sp(1,1)Sp(1,1) irrep into its maximal subgroup Sp(1)×Sp(1)Sp(1)\times Sp(1), and the SH representation restricted by the O(2)O^{*}(2) irrep condition is shown to have the structure of the massless spin ss irrep of Sp(1,1)Sp(1,1) demonstrated e.g. in [31].

For the N=2N=2 case, we need to begin with identifying irreps of the dual group O(4)O^{*}(4). Thanks to the isomorphism O(4)[SU(2)×SL(2,)]/2O^{*}(4)\cong[SU(2)\times SL(2,\mathbb{R})]/\mathbb{Z}_{2} (here, SU(2)SU(2) and SL(2,)SL(2,\mathbb{R}) are simply the Lie groups associated with 𝔰=𝔰𝔬(3)\mathfrak{s}=\mathfrak{so}(3) and 𝔪Λ>0=𝔰𝔬(2,1)\mathfrak{m}_{\Lambda>0}=\mathfrak{so}(2,1)), we know everything about the unitary irreps of O(4)O^{*}(4): the irreps of SU(2)SU(2) are all given by (2s+1)(2s+1)-dimensional representation, which will be denoted by [2s][2s] henceforth, while SL(2,)SL(2,\mathbb{R}) has three classes of unitary irreps, namely 𝒞μ=12+iρ±{\cal C}^{\pm}_{\mu=-\frac{1}{2}+i\,\rho} (3.13), 𝒞μ{\cal C}_{\mu} (3.14) and 𝒟2μ+2±{\cal D}^{\pm}_{2\mu+2} (3.15). We will denote these O(4)O^{*}(4) irreps as π~s,μ\tilde{\pi}_{s,\mu}.

In the previous section, we have seen that not all O(4)O^{*}(4) irreps correspond to irreps of Sp(1,1)Sp(1,1) based on the match of Casimir operators. We shall see below how they are restricted. For that, we first consider the dual pair (Sp(1),O(4))Sp(8,)\big{(}Sp(1),O^{*}(4)\big{)}\subset Sp(8,\mathbb{R}), whose representations are explicitly identified in [19, Sec. 5.4]: Since Sp(1)SU(2)Sp(1)\cong SU(2) the Sp(1)Sp(1) irreps are again given by [m][m] with non-negative integer mm, and they correspond to the O(4)O^{*}(4) irreps [m]𝒟m+2±[m]\otimes{\cal D}^{\pm}_{m+2} . Note that only discrete series representations appear in the SL(2,)SL(2,\mathbb{R}) side, with the highest/lowest weight m+2m+2 tied with the dimension m+1m+1 of the SU(2)SU(2) irrep (which is a consequence of the fact that the Howe dual is a compact group, namely Sp(1)Sp(1)). Whether the irrep 𝒟m+2±{\cal D}^{\pm}_{m+2} is a highest/lowest weight one is conventional at this stage, and only one sign is chosen depending on the convention of SL(2,)SL(2,\mathbb{R}).

Now we move on to the dS4 group Sp(1,1)Sp(1,1) and consider its maximal compact subgroup, which is Sp(1)×Sp(1)Sp(1)\times Sp(1). This subgroup forms its own dual pair in the same SH space (that is, in Sp(16,)Sp(16,\mathbb{R})) with O(4)×O(4)O^{*}(4)\times O^{*}(4). The latter contains the original dual group O(4)O^{*}(4) as the diagonal subgroup. The situation is conveniently depicted by the “seesaw” diagram,

Sp(1,1)Sp(1,1)\cupSp(1)×Sp(1)Sp(1)\times Sp(1)O(4)O^{*}(4)\cupO(4)×O(4)O^{*}(4)\times O^{*}(4) (4.1)

where the arrows indicate the respective dual pairs. Any irrep of Sp(1,1)Sp(1,1), say πσ\pi_{\sigma} with some label σ\sigma, can be decomposed into irreps of Sp(1)×Sp(1)Sp(1)\times Sp(1) as

πσ=m,nNσm,n[m][n],\pi_{\sigma}=\bigoplus_{m,n}N_{\sigma}^{m,n}\,[m]\otimes[n]\,, (4.2)

where Nσm,nN^{m,n}_{\sigma} are the multiplicities of [m][n][m]\otimes[n], and each of [m][n][m]\otimes[n] correspond to the O(4)×O(4)O^{*}(4)\times O^{*}(4) irrep,

([m]𝒟m+2)([n]𝒟n+2+).\Big{(}[m]\otimes{\cal D}^{-}_{m+2}\Big{)}\otimes\Big{(}[n]\otimes{\cal D}^{+}_{n+2}\Big{)}\,. (4.3)

Here, we used the correspondence between the irreps of Sp(1)Sp(1) and O(4)O^{*}(4) that we introduced earlier. Note that the first SL(2,)SL(2,\mathbb{R}) irrep is a lowest-weight irrep, while the second is a heighest-weight irrep. This is because the Sp(1)×Sp(1)Sp(1)\times Sp(1) is embedded in the opposite signature parts of Sp(1,1)Sp(1,1). The irrep (4.3) of O(4)×O(4)O^{*}(4)\times O^{*}(4) can be decomposed as well into the diagonal subgroup O(4)O^{*}(4) :

([m]𝒟m+2)([n]𝒟n+2+)=s,μN~m,ns,μπ~s,μ,\Big{(}[m]\otimes{\cal D}^{-}_{m+2}\Big{)}\otimes\Big{(}[n]\otimes{\cal D}^{+}_{n+2}\Big{)}=\bigoplus_{s,\mu}\tilde{N}^{s,\mu}_{m,n}\,\tilde{\pi}_{s,\mu}\,, (4.4)

where N~m,ns,μ\tilde{N}^{s,\mu}_{m,n} are the multiplicities of the O(4)O^{*}(4) irrep π~s,μ\tilde{\pi}_{s,\mu} that we have introduced before. The crucial point assured by the seesaw duality (see [20, 21, 22] and also [19, Sec. 2.3]) is the equality between two multiplicities: for any [m][n][m]\otimes[n],

Nσ(s,μ)m,n=N~m,ns,μ.N^{m,n}_{\sigma(s,\mu)}=\tilde{N}^{s,\mu}_{m,n}\,. (4.5)

Here, σ(s,μ)\sigma(s,\mu) is the label of the Sp(1,1)Sp(1,1) irrep dual to the O(4)O^{*}(4) irrep π~s,μ\tilde{\pi}_{s,\mu}.

Now let us identify the multiplicities N~m,ns,μ\tilde{N}^{s,\mu}_{m,n}. The decomposition (4.4) comes in two parts: the decomposition of the SU(2)SU(2) irreps,

[m][n]=[|mn|][|mn|+2][m+n],[m]\otimes[n]=[|m-n|]\oplus[|m-n|+2]\oplus\cdots\oplus[m+n]\,, (4.6)

and the decomposition of the SL(2,)SL(2,\mathbb{R}) irreps [43] (see also [44]),

𝒟m+2𝒟n+2+=0dρ𝒞12+iρ(1)m+n0k<|mn|2𝒟|mn|2ksgn(mn).{\cal D}^{-}_{m+2}\otimes{\cal D}^{+}_{n+2}=\int_{0}^{\infty}{\rm d}\rho\ {\cal C}_{-\frac{1}{2}+i\,\rho}^{(-1)^{m+n}}\oplus\bigoplus_{0\leq k<\frac{|m-n|}{2}}\,{\cal D}^{{\rm sgn}(m-n)}_{|m-n|-2k}\,. (4.7)

We see that the multiplicities are either 11 or 0. Hence, for a fixed π~s,μ\tilde{\pi}_{s,\mu} the above decomposition simply restricts the possible [m][n][m]\otimes[n] which appear in the decomposition (4.2) of πσ(s,μ)\pi_{\sigma(s,\mu)}. Moreover, we find that certain π~s,μ\tilde{\pi}_{s,\mu}’s do not admit any [m][n][m]\otimes[n] implying that such irreps cannot correspond to any (even trivial) Sp(1,1)Sp(1,1) irrep. In other words, they are simply not contained in the SH representation. Let us see the details now. By choosing the SU(2)SU(2) irrep as [2s][2s], mm and nn are restricted as

|mn|2sm+n,m+n2s2.|m-n|\leq 2s\leq m+n\,,\qquad m+n-2s\in 2\,\mathbb{Z}\,. (4.8)

For the SL(2,)SL(2,\mathbb{R}) irreps with label μ\mu, we have three choices, the principal series 𝒞μ=12+iρ±{\cal C}^{\pm}_{\mu=-\frac{1}{2}+i\,\rho}, the complementary series 𝒞μ{\cal C}_{\mu} and the discrete series 𝒟2μ+2±{\cal D}^{\pm}_{2\mu+2}. We notice already that the complementary series is not available since it does not appear in the content of the tensor product decomposition, that is, in the RHS of (4.7).

If we select a principal series representation 𝒞12+iρ(1)m+n{\cal C}_{-\frac{1}{2}+i\,\rho}^{(-1)^{m+n}}, we do not have further restrictions on possible values of mm and nn. Therefore, we find

πσ(s,12+iρ)=|mn|2sm+nm+n2s2[m][n].\pi_{\sigma(s,-\frac{1}{2}+i\,\rho)}=\bigoplus_{\begin{subarray}{c}|m-n|\leq 2s\leq m+n\\ m+n-2s\in 2\mathbb{Z}\end{subarray}}[m]\otimes[n]\,. (4.9)

These correspond to the spin ss principal series representations of Sp(1,1)Sp(1,1), describing massive spin ss fields.

If we select a discrete representation 𝒟2μ+2±{\cal D}^{\pm}_{2\mu+2}, we find a further restriction on the space and obtain

πσ(s,μ)±=|mn|2sm+nm+n2s22μ+2|mn|±(mn)>0[m][n].\pi^{\pm}_{\sigma(s,\mu)}=\bigoplus_{\begin{subarray}{c}|m-n|\leq 2s\leq m+n\\ m+n-2s\in 2\mathbb{Z}\\ 2\mu+2\leq|m-n|\\ \pm(m-n)>0\end{subarray}}[m]\otimes[n]\,. (4.10)

The additional bound on mm and nn restricts also possible values of μ\mu. For integer ss, we find μ=0,1,,s1\mu=0,1,\ldots,s-1, and for half-integer ss, we find μ=12,12,,s1\mu=-\frac{1}{2},\frac{1}{2},\ldots,s-1. These irreps correspond to the spin ss discrete series representation of Sp(1,1)Sp(1,1) describing partially-massless spin ss fields and the lightest massive fermions. One can also see that they always come with two chiralities or helicities ±\pm.

To summarize, we find that the SH representations contain exactly all the unitary representations of Sp(1,1)Sp(1,1) except for the complementary series ones: the Sp(1,1)Sp(1,1) (not SL(2,)SL(2,\mathbb{R})) complementary series representation correspond to the interval 12μ<1-\frac{1}{2}\leq\mu<1 for s=0s=0 and 12μ<0-\frac{1}{2}\leq\mu<0 for s=1,2,s=1,2,\ldots respectively, while fermions do not appear in the complementary series. Interestingly, the SH representation with the dual pair (Sp(1,1),O(4))\big{(}Sp(1,1),O^{*}(4)\big{)} contains also the massless spin ss fields which can be realized by the (Sp(1,1),O(2))\big{(}Sp(1,1),O^{*}(2)\big{)} dual pair. The conformal scalar with μ=0\mu=0 (equivalently μ=1\mu=-1) is in the field content of Vasiliev’s higher spin gravity, together with all integer spin massless fields. This conformal scalar in dS4 can be realized only by the latter dual pair. For more formal treatment of the (Sp(1,1),O(4))\big{(}Sp(1,1),O^{*}(4)\big{)} dual pair, one may consult with [45, 46].

4.2 AdS4

The Λ<0\Lambda<0 case is more straightforward, and it is recently discussed in [19]. We use the seesaw diagram,

Sp(4,)Sp(4,\mathbb{R})\cupU(2)U(2)O(2N)O(2N)\cupU(2N)U(2N) (4.11)

relating the reductive dual pairs (Sp(4,),O(2N))\big{(}Sp(4,\mathbb{R}),O(2N)\big{)} and (U(2),U(2N))\big{(}U(2),U(2N)\big{)} in Sp(8N,)Sp(8N,\mathbb{R}).

For N=1N=1, the irreps of O(2)O(2) are [2s]O(2)[2s]_{O(2)} with 2s2s\in\mathbb{N} and [1,1]O(2)[1,1]_{O(2)} . The one-dimensional irreps [0]O(2)[0]_{O(2)} and [1,1]O(2)[1,1]_{O(2)} corresponds to the scalar irreps of Sp(4,)Sp(4,\mathbb{R}), whereas [2s]O(2)[2s]_{O(2)} correspond to the massless spin ss irreps of Sp(4,)Sp(4,\mathbb{R}). The latter irreps are two dimensional, composed of the helicity ±s\pm s irreps, which are related by the 2\mathbb{Z}_{2} part of O(2)2SO(2)O(2)\cong\mathbb{Z}_{2}\ltimes SO(2), so they assemble into a single irrep for O(2)O(2).

For N=2N=2, the dual representation of [μ+s,μs]O(4)=[s]O(3)[μ]O(3)[\mu+s,\mu-s]_{O(4)}=[s]_{O(3)}\otimes[\mu]_{O(3)} is the discrete series representation 𝒟Sp(4,)(μ+2,s){\cal D}_{Sp(4,\mathbb{R})}(\mu+2,s) with the lowest energy μ+2=s+2,s+3,\mu+2=s+2,s+3,\ldots. Note that in this case the SH representation contains all the massive fields while excludes the massless fields, which can be realised by the (Sp(4,),O(2))\big{(}Sp(4,\mathbb{R}),O(2)\big{)} dual pair.

Above, we had mentioned that Sp(4,)Sp(4,\mathbb{R}) contains many representations other than the discrete series ones. These irreps would correspond to rather exotic fields such as tachyon, continuous spin [47, 48, 49] and even the ones living in bitemporal counterpart of AdS4 (see [50] for related discussions). These irreps might be also realized using proper SH representations, namely dual pairs with different dual groups O(1,1)O(1,1), O(2,1)O(2,1), O(3,1)O(3,1) and O(2,2)O(2,2). In the simplest O(1)O(1) case, the dual pair describes the conformal scalar and spinor fields in 3d3d. Let us remark also that this different signature variety is not available for dS4 with Sp(1,1)Sp(1,1) since O(2N)O^{*}(2N) does not allow any signature variations and 2N2N must be even.

4.3 Conformal group

As we had commented above, the four-dimensional conformal group 𝔰𝔬(2,4)\operatorname{\mathfrak{so}}(2,4) [24, 25, 26, 27] has a special representation called ‘singleton’ which reduces to the massless irreps of (A)dS4 with multiplicity one.888In fact, the scalar irrep of 𝔰𝔬(2,4)\operatorname{\mathfrak{so}}(2,4) reduces into two irreps of 𝔰𝔬(2,3)\operatorname{\mathfrak{so}}(2,3) which can be interpreted as the two possible boundary conditions of the AdS4 scalar field. This can be easily seen from the dual pair correspondence [19, Sec. 8.2]. First, within the SH representation, the conformal symmetry SU(2,2)SU(2,2) that the massless fields enjoy is enhanced to U(2,2)U(2,2) with the dual group U(1)U(1). The dS4 group reduction can be understood from the dual pairs,

U(2,2)U(2,2)\cupSp(1,1)Sp(1,1)U(1)U(1)\cupO(2)O^{*}(2) (4.12)

where the reduction of O(2)U(1)O^{*}(2)\cong U(1) to U(1)U(1) is trivial, thereby explaining the singleton property of the massless Sp(1,1)Sp(1,1) irrep. Similarly, the AdS4 group reduction follows the dual pairs,

U(2,2)U(2,2)\cupSp(4,)Sp(4,\mathbb{R})U(1)U(1)\cupO(2)O(2) (4.13)

where again O(2)U(1)2O(2)\cong U(1)\rtimes\mathbb{Z}_{2} reduces to U(1)U(1) trivially except for the scalar case, and hence the same mechanism works for the massless Sp(4,)Sp(4,\mathbb{R}) irreps.

4.4 Other dimensions

The SH formalism for massless fields in Mink4 can be extended to 3d [51], 5d [52], 6d [53] and 10d [54]. In case of 3 and 6 dimensions, such SH representations can be uplifted to the irreps of conformal groups SO~(2,3)Sp(4,)\widetilde{SO}^{\uparrow}(2,3)\cong Sp(4,\mathbb{R}) and SO~(2,6)O(8)\widetilde{SO}^{\uparrow}(2,6)\cong O^{*}(8). Together with the four-dimensional one SO~(2,4)SU(2,2)\widetilde{SO}^{\uparrow}(2,4)\cong SU(2,2), the conformal groups can be regarded as symplectic groups 𝖲𝗉(4,𝔽)\mathsf{Sp}(4,\mathbb{F})999Here, the symplectic group 𝖲𝗉(4,𝔽)\mathsf{Sp}(4,\mathbb{F}) is defined as the matrices AGL(4,𝔽)A\in GL(4,\mathbb{F}) satisfying AΩ(4)A=Ω(4)A^{\dagger}\,\Omega_{\scriptscriptstyle(4)}\,A=\Omega_{\scriptscriptstyle(4)} where \dagger is the conjugation with respect to 𝔽\mathbb{F} and Ω(4)\Omega_{\scriptscriptstyle(4)} is the four-dimensional symplectic matrix [55]. This definition differs from the standard definition of symplectic groups. over 𝔽=,\mathbb{F}=\mathbb{R},\mathbb{C} and \mathbb{H},

𝖲𝗉(4,)=Sp(4,),𝖲𝗉(4,)U(2,2),𝖲𝗉(4,)O(8).\mathsf{Sp}(4,\mathbb{R})=Sp(4,\mathbb{R})\,,\qquad\mathsf{Sp}(4,\mathbb{C})\cong U(2,2)\,,\qquad\mathsf{Sp}(4,\mathbb{H})\cong O^{*}(8)\,. (4.14)

These groups naturally include as subgroups the 3, 4 and 6 dimensional Lorentz groups isomorphic to SL(2,)SL(2,\mathbb{R}), SL(2,)SL(2,\mathbb{C}) and SL(2,)SL(2,\mathbb{H}), respectively.

For the SH representations of (A)dS fields, the (A)dS groups in the spinor representation need to contain the Lorentz group in the spinor representation. In 4 dimensions, this was possible thanks to the embedding of the Lorentz group Sp(2,)Sp(2,\mathbb{C}) into Sp(4,)Sp(4,\mathbb{R}) as well as Sp(1,1)Sp(1,1). We can summarize the situation by the following diagram where the middle column corresponds to the Lorentz group and its dual, while the left and right columns correspond to the AdS4 and dS4 groups and their duals, respectively.

Sp(4,)Sp(4,\mathbb{R})\subsetSp(2,)Sp(2,\mathbb{C})\supsetSp(1,1)Sp(1,1)O(2n)O(2n)\supsetO(2n,)O(2n,\mathbb{C})\subsetO(2n)O^{*}(2n) (4.15)

In 3 dimensions, we find an analogous structure which ensures the SH representations of (A)dS3 fields. The relevant diagram is the following.

Sp(2,)×Sp(2,)Sp(2,\mathbb{R})\times Sp(2,\mathbb{R})\subsetSp(2,)Sp(2,\mathbb{R})\supsetSp(2,)Sp(2,\mathbb{C})O(n)×O(n)O(n)\times O(n)\supsetO(2n)O(2n)\subsetO(n,)O(n,\mathbb{C}) (4.16)

In five dimensions, we find the following structure (SU(4)SO~(1,5)SU^{*}(4)\cong\widetilde{SO}^{\uparrow}(1,5) is the dS5 group).

U(2,2)U(2,2)\subsetSp(1,1)Sp(1,1)\supsetU(4)U^{*}(4)U(2n)U(2n)\supsetO(4n)O^{*}(4n)\subsetU(2n)U^{*}(2n) (4.17)

Note that the flat limit of the above should agree with the 5d SH representations constructed in [52].

5 Multilinear invariants

5.1 Generalities

The (A)dS4 SH representation can be utilized in physical observables like scattering amplitudes in flat space. Of course, nn-particle scattering amplitudes in (A)dS4 would not make a literal sense, and one should regard them rather as boundary nn-point correlation functions. See e.g. [56, 57, 58, 59, 60] for the recent application of SH formalism to CFT correlators. At the technical level, they are nothing but the functions of nn helicity spinors invariant under 𝔖𝔶𝔪Λ\mathfrak{Sym}_{\Lambda}, which is essentially the branching rule under the restriction 𝔖𝔶𝔪Λ×n𝔖𝔶𝔪Λ\mathfrak{Sym}_{\Lambda}^{\times n}\downarrow\mathfrak{Sym}_{\Lambda} . This leads to the dual pair

𝔖𝔶𝔪Λ××𝔖𝔶𝔪Λ\mathfrak{Sym}_{\Lambda}\times\cdots\times\mathfrak{Sym}_{\Lambda}\cup𝔖𝔶𝔪Λ\mathfrak{Sym}_{\Lambda}𝔇𝔲𝔞𝔩Λ(N1)××𝔇𝔲𝔞𝔩Λ(Nn)\mathfrak{Dual}^{(N_{1})}_{\Lambda}\times\cdots\times\mathfrak{Dual}^{(N_{n})}_{\Lambda}\cup𝔇𝔲𝔞𝔩Λ(N1,,Nn)\mathfrak{Dual}^{(N_{1},\ldots,N_{n})}_{\Lambda} (5.1)

where 𝔇𝔲𝔞𝔩Λ(N1,,Nn)\mathfrak{Dual}^{(N_{1},\ldots,N_{n})}_{\Lambda} is given by

𝔇𝔲𝔞𝔩Λ>0(N1,,Nn)\displaystyle\mathfrak{Dual}^{(N_{1},\ldots,N_{n})}_{\Lambda>0} =\displaystyle= O(2(N1++Nn)),\displaystyle O^{*}(2(N_{1}+\cdots+N_{n}))\,,
𝔇𝔲𝔞𝔩Λ<0(N1,,Nn)\displaystyle\mathfrak{Dual}^{(N_{1},\ldots,N_{n})}_{\Lambda<0} =\displaystyle= O(2(N1++Np),2(Np+1++Nn)),\displaystyle O(2(N_{1}+\cdots+N_{p}),2(N_{p+1}+\cdots+N_{n}))\,, (5.2)

where pp and npn-p are respectively the number of incoming and outgoing particles. Note that in dS4 case, there is no distinction between incoming and outgoing particles as the energy of a particle is not a conserved quantity.

In (5.1), we require that the down-right factor 𝔇𝔲𝔞𝔩Λ(N1)××𝔇𝔲𝔞𝔩Λ(Nn)\mathfrak{Dual}^{(N_{1})}_{\Lambda}\times\cdots\times\mathfrak{Dual}^{{(N_{n})}}_{\Lambda} carry an irrep correspondingly to the particle species entering the scattering, and the down-left 𝔖𝔶𝔪Λ\mathfrak{Sym}_{\Lambda} carry the trivial representation, that is invariance under (A)dS4 symmetry. The translation invariance condition is deformed by the derivative part in Pab˙P_{a\dot{b}} (2.8), and becomes more involved to solve, while the Lorentz invariance can be easily achieved, like in the flat space case, by assuming that the amplitude is a function of the contracted variables,

iIjJ=λiIλjJaa,[iIjJ]=λ~iIa˙λ~jJ.a˙\langle iI\,jJ\rangle=\lambda^{iI}{}_{a}\,\lambda^{jJ\,a}\,,\qquad[iI\,jJ]=\tilde{\lambda}_{iI\,\dot{a}}\,\tilde{\lambda}_{jJ}{}^{\dot{a}}\,. (5.3)

Here, iI,jJiI,jJ are collective indices in which i,j=1,2,,ni,j=1,2,\ldots,n label the particles entering to the scattering, whereas I=1,2,,NiI=1,2,\ldots,N_{i} and J=1,2,,NjJ=1,2,\ldots,N_{j} are the dual group indices for each particle. The 𝔇𝔲𝔞𝔩Λ(N)\mathfrak{Dual}^{(N)}_{\Lambda} irrep condition depends on NN, and it is sufficient for us to consider N=1N=1 and N=2N=2. For N=1N=1, it is the usual helicity condition. For N=2N=2 with 𝔡𝔲𝔞𝔩Λ(2)=𝔰𝔪Λ\mathfrak{dual}^{{(2)}}_{\Lambda}=\mathfrak{s}\oplus\mathfrak{m}_{\Lambda}, the irrep condition of 𝔰\mathfrak{s} can be imposed like in the flat space case as in [5, 7], and we need to impose the irrep condition of 𝔪Λ\mathfrak{m}_{\Lambda} which becomes involved due to the derivative parts of MM and M~\tilde{M} given in (2.9).

As a side remark, let us point out that the complex positive Grassmannian structure of scattering amplitudes of nn massless fields [61, 62, 63] naturally appears within the framework of the dual pair correspondence, as explained in [19, Sec. 7]. When the scattering particles are all massless, that is N1==Nn=1N_{1}=\cdots=N_{n}=1, the spacetime symmetry 𝔖𝔶𝔪Λ\mathfrak{Sym}_{\Lambda} is enhanced to U(2,2)U(2,2), while the dual group 𝔇𝔲𝔞𝔩Λ(1,,1)\mathfrak{Dual}^{(1,\ldots,1)}_{\Lambda} becomes the indefinite unitary group U(p,np)U(p,n-p) in the dual pairs (5.1). In this enhanced setting, we do not require the full invariance under U(2,2)U(2,2) but only under the subgroup 𝔖𝔶𝔪Λ\mathfrak{Sym}_{\Lambda}, which contains the Lorentz subgroup SL(2,)SL(2,\mathbb{C}). Together with the diagonal subgroup ×\mathbb{C}^{\times} generated by the total helicity and the dilation operator, the Lorentz SL(2,)SL(2,\mathbb{C}) can be uplifted to GL(2,)GL(2,\mathbb{C}), which has GL(n,)GL(n,\mathbb{C}) as its dual group. The situation can be again summarized by the following seesaw diagram.

U(2,2)××U(2,2)U(2,2)\times\cdots\times U(2,2)\cupU(2,2)U(2,2)\cupGL(2,)GL(2,\mathbb{C})GL(n,)GL(n,\mathbb{C})\cupU(p,np)U(p,n-p)\cupU(1)××U(1)U(1)\times\cdots\times U(1) (5.4)

The Lorentz invariance is equivalent to the condition that under restriction to GL(2,)GL(2,\mathbb{C}), the amplitudes carry a one-dimensional representation, wherein SL(2,)SL(2,\mathbb{C}) acts trivially, and GL(1,)×GL(1,\mathbb{C})\cong\mathbb{C}^{\times} acts diagonally. The corresponding GL(n,)GL(n,\mathbb{C}) representation is a degenerate principal series representation (see e.g. [64]), which is realized as the space of functions on the complex positive Grassmannian manifold Gr2,n()Gr_{2,n}(\mathbb{C}).

Coming back to the picture (5.1), the only non-trivial part of the conditions are the translational invariance condition, and the irrep condition of 𝔪Λ\mathfrak{m}_{\Lambda} for N=2N=2. When Λ=0\Lambda=0, both of these conditions are algebraic and could be solved by imposing the helicity spinors to be constrained on the shell of the momentum conservation and constant mass-squared. When Λ0\Lambda\neq 0, both of these conditions become differential equations.

5.2 Translational invariance

Let us consider first the condition of translation invariance,

Pab˙𝒜=(λλ~b˙a+Λλaλ~b˙)𝒜=0,P_{a\dot{b}}\,{\cal A}=\left(\lambda^{{\cal I}}{}_{a}\,\tilde{\lambda}_{{\cal I}\,\dot{b}}+\Lambda\,\frac{\partial}{\partial\lambda^{{\cal I}\,a}}\frac{\partial}{\partial\tilde{\lambda}_{{\cal I}}{}^{\dot{b}}}\right){\cal A}=0\,, (5.5)

where =iI,𝒥=jJ{\cal I}=iI,{\cal J}=jJ denote the collective indices. In the Mink4 case, the solution is nothing but the momentum conservation delta distribution δ4(p)\delta^{4}(p) with

pab˙=λλ~b˙a,p_{a\dot{b}}=\lambda^{{\cal I}}{}_{a}\,\tilde{\lambda}_{{\cal I}\,\dot{b}}\,, (5.6)

and hence we expect a similar kind of distributional property for the Λ0\Lambda\neq 0 solution. For the massless 3pt case, this equation has been analyzed in detail in [13, App. E], where the authors made an ansatz as a function of 12[12]\langle 12\rangle[12], 23[23]\langle 23\rangle[23] and 31[31]\langle 31\rangle[31] and derived a system of four PDEs. Instead of solving these equations directly, they checked that the amplitudes obtained from field theoretical approach (that is, spacetime integral of three AdS plane wave solutions) solve the equations. The solution is spanned by four independent distributions of 12[12]+23[23]+31[31]=12pab˙pab˙\langle 12\rangle\,[12]+\langle 23\rangle\,[23]+\langle 31\rangle\,[31]=\tfrac{1}{2}\,p_{a\dot{b}}\,p^{a\dot{b}}.

Let us revisit the problem slightly differently for the general case (massive or massless nn-pt). Since 𝒜{\cal A} should involve the momentum conservation delta function in the flat limit, we consider the ansatz 𝒜=𝒜(pab˙,𝒥,[𝒥]){\cal A}={\cal A}(p_{a\dot{b}},\langle{\cal I}{\cal J}\rangle,[{\cal I}{\cal J}]) .101010Note that the variables pab˙p_{a\dot{b}} are not independent from 𝒥\langle{\cal I}{\cal J}\rangle and [𝒥][{\cal I}{\cal J}], as they are related by pab˙pab˙=𝒥[𝒥]p_{a\dot{b}}\,p^{a\dot{b}}=\langle{\cal I}{\cal J}\rangle[{\cal I}{\cal J}]. Therefore, whenever the latter combination appears, we have to regard them as a function of pab˙p_{a\dot{b}} to avoid the related ambiguities. Then the condition (5.5) sets up the differential equation,

[pab˙+Λ(pcd˙pad˙pcb˙+Hpab˙+λ𝒥λ~𝒦b˙a𝒥[𝒦])]𝒜=0,\left[p_{a\dot{b}}+\Lambda\left(p^{c\dot{d}}\,\frac{\partial}{\partial p^{{a\dot{d}}}}\,\frac{\partial}{\partial p^{{c\dot{b}}}}+H\,\frac{\partial}{\partial p^{a\dot{b}}}+\lambda^{{\cal J}}{}_{a}\,\tilde{\lambda}_{{\cal K}\dot{b}}\frac{\partial}{\partial\langle{\cal I}{\cal J}\rangle}\frac{\partial}{\partial[{\cal I}{\cal K}]}\right)\right]{\cal A}=0\,, (5.7)

with the number operator HH,

H=𝒩+12𝒥𝒥+12[𝒥][𝒥],H={\cal N}+\frac{1}{2}\,\langle{\cal I}{\cal J}\rangle\,\frac{\partial}{\partial\langle{\cal I}{\cal J}\rangle}+\frac{1}{2}\,[{\cal I}{\cal J}]\,\frac{\partial}{\partial[{\cal I}{\cal J}]}\,, (5.8)

where 𝒩=i=1nNi{\cal N}=\sum_{i=1}^{n}N_{i} is the sum of the ranks of the dual groups for all nn particles, and the factor 1/21/2 has been introduced to take the antisymmetry of 𝒥{\cal I}{\cal J} into account. The last term of the differential equation (5.7) is problematic since it is not expressed in terms of the variables pab˙p_{a\dot{b}}, 𝒥\langle{\cal I}{\cal J}\rangle and [𝒥][{\cal I}{\cal J}] only. We can bypass the problem by focusing on the “longitudinal part” of the equation: contracting (5.7) with pab˙p^{a\dot{b}}, we find

[pab˙pab˙+Λ(pab˙pcd˙pad˙pcb˙+Hpab˙pab˙+2R)]𝒜=0,\left[p^{a\dot{b}}\,p_{a\dot{b}}+\Lambda\left(p^{a\dot{b}}\,p^{c\dot{d}}\,\frac{\partial}{\partial p^{a\dot{d}}}\,\frac{\partial}{\partial p^{c\dot{b}}}+H\,p^{a\dot{b}}\,\frac{\partial}{\partial p^{a\dot{b}}}+2\,R\right)\right]{\cal A}=0\,, (5.9)

where RR is a differential operator acting on the Lorentz invariant variables as

R=12𝒥𝒥[𝒦][𝒦].R=\frac{1}{2}\,\langle{\cal I}{\cal J}\rangle\,\frac{\partial}{\partial\langle{\cal J}{\cal L}\rangle}\,[{\cal I}{\cal K}]\,\frac{\partial}{\partial[{\cal K}{\cal L}]}\,. (5.10)

Viewing Λ\Lambda as a deformation parameter, our aim is to find the deformation of the delta distribution solution of the Λ=0\Lambda=0 case. We can better control the situation by going to the Fourier space qab˙q^{a\dot{b}} where the constant solution corresponds to the correct delta distribution in the Λ=0\Lambda=0 case. Since the constant solution is isotropic, we assume that 𝒜~\tilde{\cal A} is a function of t=12qab˙qab˙t=\frac{1}{2}\,q^{a\dot{b}}\,q_{a\dot{b}}, and this reduces the equation to the simple second order differential equation in the tt variable,

[(tt+2)((1Λt)t+Λ(H4))ΛR]𝒜~=0.\left[\left(t\,\frac{\partial}{\partial t}+2\right)\,\left((1-\Lambda\,t)\,\frac{\partial}{\partial t}+\Lambda\,(H-4)\right)-\Lambda\,R\right]\,\tilde{\cal A}=0\,. (5.11)

We can use the separation of variables,

R𝒜~r=r𝒜~r,R\,\tilde{\cal A}_{r}=r\,\tilde{\cal A}_{r}\,, (5.12)

to decompose the PDE (5.11) into hypergeometric differential equations with two types of solutions, the first one being,

𝒜~r=F12(a+,a,2;Λt)fr,\tilde{\cal A}_{r}={}_{2}F_{1}\Big{(}a_{+},a_{-},2\,;\,\Lambda\,t\Big{)}\,f_{r}\,, (5.13)

where a±a_{\pm} are

a±=12(6H±(H2)2r),a_{\pm}=\frac{1}{2}\left(6-H\pm\sqrt{(H-2)^{2}-r}\right), (5.14)

and frf_{r} is an arbitrary function of 𝒥\langle{\cal I}{\cal J}\rangle and [𝒥][{\cal I}{\cal J}]. The second solution of the hypergeometric differential equation takes the form,

1t+Λn=0(a+1)n+1(a1)n+1(n+1)!n![ln(Λt)(Λt)n+cn(Λt)n+1],\frac{1}{t}+\Lambda\,\sum_{n=0}^{\infty}\frac{(a_{+}-1)_{n+1}\,(a_{-}-1)_{n+1}}{(n+1)!\,n!}\left[\ln(\Lambda\,t)\,(\Lambda\,t)^{n}+c_{n}\,(\Lambda\,t)^{n+1}\right]\,, (5.15)

with

cn=m=0n1(1a++m+1a+m1m+21m+1).c_{n}=\sum_{m=0}^{n-1}\left(\frac{1}{a_{+}+m}+\frac{1}{a_{-}+m}-\frac{1}{m+2}-\frac{1}{m+1}\right). (5.16)

The hypergeometric function F12(a+,a,2;Λt){}_{2}F_{1}(a_{+},a_{-},2;\Lambda\,t) reduces to 11 for Λ=r=0\Lambda=r=0, while the second solution (5.15) to 1/t1/t. Since the constant solution corresponds to the desired delta distribution, we retain only the hypergeometric function. Remark that for r=0r=0, the hypergeometric function gets simplified to give

𝒜~0=(1Λt)H4f0.\tilde{\cal A}_{0}=(1-\Lambda\,t)^{H-4}\,f_{0}\,. (5.17)

This is consistent with the expressions obtained in [12, 13, 14] for massless 3pt. Remark also that the hypergeometric function (5.13) has a branch point at Λt=1\Lambda\,t=1,111111In [12, 13, 14], the qab˙q_{a\dot{b}} variables carry a spacetime coordinate interpretation, and the branch point corresponds to the boundary of the coordinate chart. which might be interpreted as the cosmological horizon and related to the alpha vacua.121212In de Sitter space, there is a one-parameter family of dS invariant vacuum states [65]. This vacuum ambiguity would lead to an analogous ambiguity in nn-point correlation functions. Eventually, the most general invariant will be linear combinations of 𝒜r{\cal A}_{r} with different rr values.

5.3 Mass condition

Let us move on to the irrep condition of 𝔪Λ\mathfrak{m}_{\Lambda} for each of the nn particles, fixing their masses. For the discrete series irreps of 𝔡𝔲𝔞𝔩Λ>0(2)\mathfrak{dual}^{(2)}_{\Lambda>0} in the dS4 case and the finite-dimensional irreps of 𝔡𝔲𝔞𝔩Λ<0(2)\mathfrak{dual}^{(2)}_{\Lambda<0} in the AdS4 case, we can impose the highest weight condition Mi𝒜=0M_{i}\,{\cal A}=0 or the lowest weight condition M~i𝒜=0\tilde{M}_{i}\,{\cal A}=0 , on the KiK_{i} eigenstate with

Kif=2(μi+1)f,K_{i}\,f=\mp 2\,(\mu_{i}+1)\,f\,, (5.18)

for dS4 and

Kif=±2μif,K_{i}\,f=\pm 2\mu_{i}\,f\,, (5.19)

for AdS4. Here, the KiK_{i}, upon acting on ff, reduces to the differential operator,

Kif=(iI𝒥iI𝒥[iI𝒥][iI𝒥])f,K_{i}\,f=\left(\langle iI\,{\cal J}\rangle\,\frac{\partial}{\partial\langle iI\,{\cal J}\rangle}-[iI\,{\cal J}]\,\frac{\partial}{\partial[iI\,{\cal J}]}\right)f\,, (5.20)

where the repeated indices 𝒥{\cal J} and II are summed over except for the particle label ii. The highest weight condition M𝒜=0M\,{\cal A}=0 can be translated as well into the differential equations,

Mif=[i1i2+Λ(2[i1i2]+[𝒥𝒦][i1𝒥][i2𝒦])]f=0,M_{i}\,f=\left[\langle i1\,i2\rangle+\,\Lambda\left(2\,\frac{\partial}{\partial[i1\,i2]}+[{\cal J}{\cal K}]\,\frac{\partial}{\partial[i1\,{\cal J}]}\,\frac{\partial}{\partial[i2\,{\cal K}]}\right)\right]f=0\,,

where the repeated indices 𝒥,𝒦{\cal J},{\cal K} include ii’th particle’s values iIiI, and the lowest weight condition is simply given by the complex conjugate of the above.

Note that the KK eigenstate conditions (5.18) and (5.19) become singular in the flat limit where μ\mu is sent to infinity while μ|Λ|\mu\sqrt{|\Lambda|} held fixed. Moreover, the principal series irreps of dS4 have neither a highest nor a lowest weight state. Therefore, the above conditions are inapplicable in that case. We may consider to use the KK eigenstate with eigenvalue 0 or ±1\pm 1 to avoid this problem, but in that case we cannot use any more the simple condition M=0M=0 (or M~=0\tilde{M}=0). Instead we need to use the Casimir condition involving the anticommutator {M,M~}\{M,\tilde{M}\} resulting in a fourth-order differential equation instead of (5.3).

In fact, for the principal series irreps, it is more natural to impose

(MiM~i)f=2Λμif,\displaystyle(M_{i}-\tilde{M}_{i})\,f=2\,\sqrt{\Lambda}\,\mu_{i}\,f\,, (5.21a)
(Mi+M~iΛKi)f=0,\displaystyle(M_{i}+\tilde{M}_{i}-\sqrt{\Lambda}\,K_{i})\,f=0\,, (5.21b)

which has also a well-defined flat limit, and can be expressed as second order differential equations in 𝒥\langle{\cal I}{\cal J}\rangle and [𝒥][{\cal I}{\cal J}]. Solving these conditions is beyond the scope of the current work. Instead, let us make a few remarks on the change of basis where the O(4)O^{*}(4) actions become more natural.

For the change of basis, we fix the convention as a,b,a˙,b˙=+,a,b,\dot{a},\dot{b}=+,- and ϵ+=ϵ+=1\epsilon_{-+}=\epsilon^{+-}=1 and perform Fourier transform with respect to λI\lambda^{I}_{-} and its complex conjugate as

(λIΛ,ΛλI,λ~IΛ,Λλ~I)i(ζI,ζI,ζ~I,ζ~I).\left(\,\frac{\lambda^{I}{}_{-}}{\sqrt{\Lambda}}\,,\,\sqrt{\Lambda}\,\frac{\partial}{\partial\lambda^{I}{}_{-}}\,,\,\frac{\tilde{\lambda}_{I-}}{\sqrt{\Lambda}}\,,\,\sqrt{\Lambda}\,\frac{\partial}{\partial\tilde{\lambda}_{I-}}\,\right)\ \longrightarrow\ i\left(\,\frac{\partial}{\partial\zeta_{I}}\,,\,\zeta_{I}\,,\,\frac{\partial}{\partial\tilde{\zeta}^{I}}\,,\,\tilde{\zeta}^{I}\,\right). (5.22)

Then, the dual algebra generators read

KI=JλIλJζJζIλ~Jλ~I+ζ~Iζ~J,\displaystyle K^{I}{}_{J}=\lambda^{I}\,\frac{\partial}{\partial\lambda^{J}}-\zeta_{J}\,\frac{\partial}{\partial\zeta_{I}}-\tilde{\lambda}_{J}\,\frac{\partial}{\partial\tilde{\lambda}_{I}}+\tilde{\zeta}^{I}\,\frac{\partial}{\partial\tilde{\zeta}^{J}}\,, (5.23a)
MIJΛ=i(λIζJλJζI+ζ~Iλ~Jζ~Jλ~I),\displaystyle\frac{M^{IJ}}{\sqrt{\Lambda}}=i\left(\lambda^{I}\,\frac{\partial}{\partial\zeta_{J}}-\lambda^{J}\,\frac{\partial}{\partial\zeta_{I}}+\tilde{\zeta}^{I}\,\frac{\partial}{\partial\tilde{\lambda}_{J}}-\tilde{\zeta}^{J}\,\frac{\partial}{\partial\tilde{\lambda}_{I}}\right), (5.23b)

where we used λI=λ+I\lambda^{I}=\lambda^{I}_{+} and λ~I=λ~I+\tilde{\lambda}_{I}=\tilde{\lambda}_{I+} . In this basis, the 𝔬(2N)\mathfrak{o}^{*}(2N) generators become first order differential operators, and hence can be easily integrated to a Lie group. This basis admits in fact a natural realization in terms of quaternions: see Appendix B for the details. While the new basis (5.23a) and (5.23b) renders the dual algebra as simple first-order differential operators, the Lorentz algebra becomes second-order instead. In other words, in the basis where the dual algebra is linearly realized, the dS4 algebra is not. And vice-versa: we can go to another basis where the dS4 algebra is realized linearly, but then the dual algebra is not.

For N=2N=2, we can consider a different Fourier transformation,

(λ2aΛ,Λλ2a,λ~2a˙Λ,Λλ~2a˙)i(ξa,ξa,ξ~a˙,ξ~a˙),\left(\,\frac{\lambda^{2}{}_{a}}{\sqrt{\Lambda}}\,,\,\sqrt{\Lambda}\,\frac{\partial}{\partial\lambda^{2}{}_{a}}\,,\,\frac{\tilde{\lambda}_{2\dot{a}}}{\sqrt{\Lambda}}\,,\,\sqrt{\Lambda}\,\frac{\partial}{\partial\tilde{\lambda}_{2\dot{a}}}\,\right)\ \longrightarrow\ i\left(\,\frac{\partial}{\partial\xi^{a}}\,,\,\xi^{a}\,,\,\frac{\partial}{\partial\tilde{\xi}^{\dot{a}}}\,,\,\tilde{\xi}^{\dot{a}}\,\right), (5.24)

where only the I=2I=2 variables are transformed. Upon a further change of basis,

za=ξaiλ1a2,wa=ξa+iλ1a2,z~a˙=ξ~a˙+iλ~1a˙2,w~a˙=ξ~a˙iλ~1a˙2,z^{a}=\frac{\xi^{a}-i\,\lambda^{1a}}{2}\,,\qquad w^{a}=\frac{\xi^{a}+i\,\lambda^{1a}}{2}\,,\qquad\tilde{z}^{\dot{a}}=\frac{\tilde{\xi}^{\dot{a}}+i\,\tilde{\lambda}_{1}{}^{\dot{a}}}{2}\,,\qquad\tilde{w}^{\dot{a}}=\frac{\tilde{\xi}^{\dot{a}}-i\,\tilde{\lambda}_{1}{}^{\dot{a}}}{2}\,, (5.25)

the conditions (5.21a) and (5.21b) become simple:

MM~Λ=zaza+z~a˙z~a˙wawaw~a˙w~a˙,\displaystyle\frac{M-\tilde{M}}{\sqrt{\Lambda}}=z^{a}\,\frac{\partial}{\partial z^{a}}+\tilde{z}^{\dot{a}}\,\frac{\partial}{\partial\tilde{z}^{\dot{a}}}-w^{a}\,\frac{\partial}{\partial w^{a}}-\tilde{w}^{\dot{a}}\,\frac{\partial}{\partial\tilde{w}^{\dot{a}}}\,, (5.26a)
M+M~ΛK=2(zawaz~a˙w~a˙).\displaystyle\frac{M+\tilde{M}}{\sqrt{\Lambda}}-K=2\left(z^{a}\,\frac{\partial}{\partial w^{a}}-\tilde{z}^{\dot{a}}\,\frac{\partial}{\partial\tilde{w}^{\dot{a}}}\right). (5.26b)

The condition (5.21b) can be solved by an arbitrary function of zaz^{a}, z~a˙\tilde{z}^{\dot{a}}, and zaw~b˙+waz~b˙z^{a}\,\tilde{w}^{\dot{b}}+w^{a}\,\tilde{z}^{\dot{b}}. Furthermore, the condition (5.21a), which fixes the principal series label, becomes a simple homogeneity condition with respect to the number operator (5.26a). The variables zaw~b˙+waz~b˙z^{a}\,\tilde{w}^{\dot{b}}+w^{a}\,\tilde{z}^{\dot{b}} have weight zero and hence are not constrained, while the homogeneity of |z|=zaz~a˙|z|=\sqrt{z^{a}\,\tilde{z}^{\dot{a}}} is restricted to μ\mu. The spin condition further restricts the variables zaw~b˙+waz~b˙z^{a}\,\tilde{w}^{\dot{b}}+w^{a}\,\tilde{z}^{\dot{b}} and za/|z|z^{a}/|z|. In the end, the remaining freedom corresponds to the massive irrep of Sp(1,1)Sp(1,1). However, in this basis, the spin part 𝔰\mathfrak{s} of the dual algebra, that is generated by KIJK^{I}{}_{J}, is realized by second-order differentials.

Therefore, the dS4 invariance condition and the O(4)O^{*}(4) irrep condition for each of the particles cannot be solved within a single basis, but by employing muliple bases that are related by Fourier transformations. These conditions may be solved for concrete examples of interest. We leave this to future investigations.

Acknowledgments

We are grateful to Eduardo Conde for agreeable communications. The work of T.B. was supported by the European Union’s Horizon 2020 research and innovation program under the Marie Skłodowska-Curie grant agreement No 101034383. E. J. was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT) (No. 2022R1F1A1074977). K. M. was supported by the European Union’s Horizon 2020 Research and Innovation Programme under the Marie Skłodowska-Curie Grant No. 844265, and STFC Consolidated Grants ST/T000791/1 and ST/X000575/1.

Appendix A UIRs of dS4 group and Casimirs

Unitary and irreducible representations of the dS4 isometry group were first classified by J. Dixmier in [31]. In this appendix, we recall this classification and the eigenvalues of the quadratic and quartic Casimir operators.

  • πp,q±\pi^{\pm}_{p,q} :  [p=12,1,32,p=\frac{1}{2},1,\frac{3}{2},\ldots ; q=p,p1,,1q=p,p-1,\ldots,1 or 12\frac{1}{2}] with

    C2=p(p+1)(q1)q+2=p(p+1)(q+1)(q2),\displaystyle C_{2}=-p(p+1)-(q-1)q+2=-p(p+1)-(q+1)(q-2)\,,
    C4=p(p+1)(q1)q,\displaystyle C_{4}=-p(p+1)(q-1)q\,, (A.1)

    corresponding to the discrete series.

  • πp,0\pi_{p,0} : [p=1,2,p=1,2,\ldots] with the quadratic and quartic Casimir operators taking the values

    C2=p(p+1)2,\displaystyle C_{2}=p(p+1)-2\,,
    C4=0.\displaystyle C_{4}=0\,. (A.2)

    These UIRs form the discrete series.

  • νp,σ\nu_{p,\sigma} :  [p=0p=0 ; σ>2\sigma>-2] and [p=1,2,p=1,2,\ldots ; σ>0\sigma>0] and [p=12,32,p=\frac{1}{2},\frac{3}{2},\ldots ; σ>14\sigma>\frac{1}{4}] with

    C2=p(p+1)σ2,\displaystyle C_{2}=p(p+1)-\sigma-2\,,
    C4=p(p+1)σ,\displaystyle C_{4}=-p(p+1)\,\sigma\,, (A.3)

    corresponding to the principal and complementary series.

Appendix B Quaternion realization of dS4 group

The dual pair (Sp(M,M),O(2N))\big{(}Sp(M,M),O^{*}(2N)\big{)} can be naturally realized in terms of quaternions. The oscillator representation is the space of functions on MN\mathbb{H}^{MN}, where O(2N)O^{*}(2N) acts on a function Φ\Phi by right multiplication,

𝖰|UO(2N)(𝖠)Φ=𝖰𝖠|Φ,\big{\langle}\mathsf{Q}\,\big{|}\,U_{O^{*}(2N)}(\mathsf{A})\,\Phi\big{\rangle}=\big{\langle}\mathsf{Q}\,\mathsf{A}\,\big{|}\Phi\big{\rangle}\,, (B.1)

where 𝖰\mathsf{Q} is an M×NM\times N quaternionic matrix and 𝖠\mathsf{A} is an N×NN\times N quaternionic matrix satisfying131313Here, 𝗃\mathsf{j} denotes the basis element of quarternions that can be represented by the Pauli matrix iσ2i\,\sigma_{2}.

𝖠𝗃𝖠=𝗃,\mathsf{A}^{\dagger}\,\mathsf{j}\,\mathsf{A}=\mathsf{j}\,, (B.2)

thereby representing an arbitrary element of O(2N)O^{*}(2N). For M=1M=1, each of the quaternionic elements of 𝖰=(𝗊I)\mathsf{Q}=(\mathsf{q}_{I}), seen as a 2×22\times 2 complex matrix, can be parameterized by two complex numbers as

𝗊I=(λI+iζIζI+iλIζ~I+iλ~Iλ~Iiζ~I).\mathsf{q}_{I}=\begin{pmatrix}\lambda^{I}+i\,\zeta_{I}&\zeta_{I}+i\,\lambda^{I}\\ -\tilde{\zeta}^{I}+i\,\tilde{\lambda}_{I}&\tilde{\lambda}_{I}-i\,\tilde{\zeta}^{I}\end{pmatrix}\,. (B.3)

Note that we recover the expressions (5.23a) and (5.23b) from the above parameterization of 𝗊I\mathsf{q}_{I}.

For even N=2LN=2L, the Sp(M,M)Sp(M,M) action can also be represented by the left multiplication of a quaternionic matrix,

(𝖰1𝖯2)|USp(M,M)(𝖡)Φ=𝖡t(𝖰1𝖯2)|Φ,\bigg{\langle}\binom{\mathsf{Q}_{1}}{\mathsf{P}_{2}}\,\bigg{|}\,U_{Sp(M,M)}(\mathsf{B})\,\Phi\bigg{\rangle}=\bigg{\langle}\mathsf{B}^{t}\,\binom{\mathsf{Q}_{1}}{\mathsf{P}_{2}}\,\bigg{|}\,\Phi\bigg{\rangle}\,, (B.4)

where 𝖡\mathsf{B} is an element of Sp(M,M)Sp(M,M), and hence a 2M×2M2M\times 2M quaternionic matrix satisfying

𝖡(0IMIM0)𝖡=(0IMIM0).\mathsf{B}^{\dagger}\begin{pmatrix}0&I_{M}\\ I_{M}&0\end{pmatrix}\mathsf{B}=\begin{pmatrix}0&I_{M}\\ I_{M}&0\end{pmatrix}. (B.5)

The sub-matrices 𝖰1\mathsf{Q}_{1} and 𝖯2\mathsf{P}_{2} are M×LM\times L quaternionic matrices, and 𝖯2\mathsf{P}_{2} is the Fourier conjugate of 𝖰2\mathsf{Q}_{2} where 𝖰1\mathsf{Q}_{1} and 𝖰2\mathsf{Q}_{2} form the M×2LM\times 2L matrix 𝖰=(𝖰1𝖰2)\mathsf{Q}=(\mathsf{Q}_{1}\,\mathsf{Q}_{2}).

References