2018
DOI: 10.1007/jhep02(2018)024
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Supersymmetric dS/CFT

Abstract: We put forward new explicit realisations of dS/CFT that relate N = 2 supersymmetric Euclidean vector models with reversed spin-statistics in three dimensions to specific supersymmetric Vasiliev theories in four-dimensional de Sitter space. The partition function of the free supersymmetric vector model deformed by a range of low spin deformations that preserve supersymmetry appears to specify a well-defined wave function with asymptotic de Sitter boundary conditions in the bulk. In particular we find the wave f… Show more

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Cited by 16 publications
(37 citation statements)
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“…12 we should fuse the two previously independent quiver tails into a single tail giving rise to a single SU (n) symmetry. 32 Indeed, note that the line of nodes in the red oval in Fig. 12 have a bifundamental connecting the two previously independent tails and consist of n − 1 total balanced nodes.…”
Section: Wave Function Relations and Topology Of 3d Mirrorsmentioning
confidence: 98%
See 1 more Smart Citation
“…12 we should fuse the two previously independent quiver tails into a single tail giving rise to a single SU (n) symmetry. 32 Indeed, note that the line of nodes in the red oval in Fig. 12 have a bifundamental connecting the two previously independent tails and consist of n − 1 total balanced nodes.…”
Section: Wave Function Relations and Topology Of 3d Mirrorsmentioning
confidence: 98%
“…Next let us discuss the case of T 2,AD (m 1 ,m 2 ,m 3 ) . For ease of reference, we again write the 32 In fact, since the wave functions have conjugate fugacities, it is tempting to write f Y full y), whereR is the SU (n) representation conjugate to R. We may then write the product of SU (n) wave functions in (5.2) as…”
Section: Wave Function Relations and Topology Of 3d Mirrorsmentioning
confidence: 99%
“…For further developments in this direction, see [6][7][8][9][10][11][12]. These studies mostly exploit the higher spin symmetries.…”
Section: Jhep03(2018)153mentioning
confidence: 99%
“…According to these proposals, the rigid symmetries of the vacuum should leave the extensive variables invariant while acting nontrivially on the microscopic variables; for related remarks, see [18,46]. 10 The full field configurations are thus assumed to contain contain asymptotically (anti-)de Sitter regions where the full tensor gauge fields φ a(s) approach Fronsdal fields give on shell in terms of polarization tensors that are non-linear functionals of the zero-form initial data C.…”
Section: Gauge Functionsmentioning
confidence: 99%
“…[23][24][25]) because in dS space there is no positive conserved quantity whereas supersymmetry would allow one to construct one. However supersymmetric HS gravity theories in de Sitter circumvent this problem since the Hermitian conjugate in the theories in [26] is an anti-involution [22]. In a similar spirit one may object that de Sitter space 'has a temperature' and therefore cannot be supersymmetric.…”
mentioning
confidence: 99%