Abstract
Abstract
In our previous article (Letsios 2023 J. High Energy Phys. JHEP05(2023)015), we showed that the strictly massless spin-3/2 field, as well as the strictly and partially massless spin-5/2 fields, on N-dimensional (
N
⩾
3
) de Sitter (dS) spacetime (dS
N
) are non-unitary unless N = 4. The (non-)unitarity was demonstrated by simply observing that there is a (mis-)match between the representation-theoretic labels that correspond to the unitary irreducible representations (UIR’s) of the dS algebra spin
(
N
,
1
)
and the ones corresponding to the space of eigenmodes of the field theories. In this paper, we provide a technical representation-theoretic explanation for this fact by studying the (non-)existence of positive-definite, dS invariant scalar products for the spin-3/2 and spin-5/2 strictly/partially massless eigenmodes on dS
N
(
N
⩾
3
). Our basic tool is the examination of the action of spin
(
N
,
1
)
generators on the space of eigenmodes, leading to the following findings. For odd N, any dS invariant scalar product is identically zero. For even N > 4, any dS invariant scalar product must be indefinite. This gives rise to positive-norm and negative-norm eigenmodes that mix with each other under spin
(
N
,
1
)
boosts. In the N = 4 case, the positive-norm sector decouples from the negative-norm sector and each sector separately forms a UIR of spin(4, 1). Our analysis makes extensive use of the analytic continuation of tensor-spinor spherical harmonics on the N-sphere (S
N
) to dS
N
and also introduces representation-theoretic techniques that are absent from the mathematical physics literature on half-odd-integer-spin fields on dS
N
.
Funder
Studentship from the Department of Mathematics, University of York
Reference62 articles.
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2. Null propagation of partially massless higher spins in (A)dS and cosmological constant speculations;Deser;Phys. Lett. B,2001
3. Arbitrary spin representations in de Sitter from dS/CFT with applications to dS supergravity;Deser;Nucl. Phys.,2003
4. The imaginary values of M in equation (1.3) imply that the action functional for strictly/partially massless half-odd-integer-spin theories on dS N is not hermitian. The fact that the strictly massless spin-3/2 field theory in de Sitter spacetime has an imaginary mass parameter had been already observed in cosmological supergravity [11]
5. Symmetric tensor spherical harmonics on the N-sphere and their application to the de Sitter group SO(N,1);Higuchi;J. Math. Phys.,1987
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