2014
DOI: 10.1007/jhep10(2014)163
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Higher spin AdS3 holography with extended supersymmetry

Abstract: We propose a holographic duality between a higher spin AdS 3 gravity with so(p) extended supersymmetry and a large N limit of a 2-dimensional Grassmannian-like model with a specific critical level k = N and a non-diagonal modular invariant. As evidence, we show the match of one-loop partition functions. Moreover, we construct symmetry generators of the coset model for low spins which are dual to gauge fields in the supergravity. Further, we discuss a possible relation to superstring theory by noticing an N = 3… Show more

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Cited by 59 publications
(119 citation statements)
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“…This yields the higher spin algebra ho(4|1)[0] in the case of S 0 , which is broken down to ho(3|1)[0] when taking the Z 2 -orbifold. This shows that the higher spin dualities of [36] are not directly embeddable in the stringy duality, similar to what was concluded in the large N = 4 case for the higher spin duality of [31].…”
Section: Jhep07(2018)143 7 Conclusionsupporting
confidence: 81%
“…This yields the higher spin algebra ho(4|1)[0] in the case of S 0 , which is broken down to ho(3|1)[0] when taking the Z 2 -orbifold. This shows that the higher spin dualities of [36] are not directly embeddable in the stringy duality, similar to what was concluded in the large N = 4 case for the higher spin duality of [31].…”
Section: Jhep07(2018)143 7 Conclusionsupporting
confidence: 81%
“…corresponding to (3.21) of [18]. We observe that the levels are given by (N +2M ), (2N +M ) and 2N M (N + M ) 2 corresponding to the SU(N ), SU(M ) and U(1) factors appearing on the denominator of the coset (1.1) respectively.…”
Section: C3 the Opes Between The Spin-1 Currents And Itselfmentioning
confidence: 79%
“…For the N = 3 holography [18], the deformation breaks the higher spin symmetry and induces the mass to the higher spin fields [19,20]. The masses are not generated for the SO(3) R singlet higher spin fields at the leading order of 1 c while the mass formula for the SO(3) R triplet higher spin fields looks like the Regge trajectory on the flat spacetime.…”
Section: Jhep12(2016)001mentioning
confidence: 99%
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