2018
DOI: 10.1088/1361-6382/aac30c
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Symmetry enhancement of extremal horizons in D   =  5 supergravity

Abstract: We consider the near-horizon geometry of supersymmetric extremal black holes in ungauged and gauged 5-dimensional supergravity, coupled to abelian vector multiplets. By analyzing the global properties of the Killing spinors, we prove that the near-horizon geometries undergo a supersymmetry enhancement. This follows from a set of generalized Lichnerowicz-type theorems we establish, together with an index theory argument. As a consequence, these solutions always admit a sl(2, R) symmetry group.

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Cited by 4 publications
(5 citation statements)
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“…Note in this context that rotating supersymmetric Nil and SL(2, R) near-horizon geometries were found in [30]. Moreover, it is worth mentioning that the near-horizon limit of all supersymmetric extremal black holes in gauged (and ungauged) five-dimensional supergravity coupled to abelian vector multiplets must admit an SL(2, R) symmetry group [31].…”
Section: Jhep12(2019)151mentioning
confidence: 83%
“…Note in this context that rotating supersymmetric Nil and SL(2, R) near-horizon geometries were found in [30]. Moreover, it is worth mentioning that the near-horizon limit of all supersymmetric extremal black holes in gauged (and ungauged) five-dimensional supergravity coupled to abelian vector multiplets must admit an SL(2, R) symmetry group [31].…”
Section: Jhep12(2019)151mentioning
confidence: 83%
“…Establishing the horizon conjecture relies on establishing Lichnerowicz-type theorems and an index theory argument. A similar analysis has been conducted for IIA, Roman's Massive IIA and IIB, D = 5 gauged with vector multiplets and D = 4 gauged [16,17,18,19,20,21]. We shall also establish the sl(2, R) symmetry algebra for nearhorizon geometries.…”
Section: Introductionmentioning
confidence: 79%
“…Another avenue for future research would be to extend the analysis for an arbitrary number of tensor and vector multiplets; similar to the calculation in D = 4, 5 with vector multiplets [21,20]. In six dimensions, near horizon geometries have been classified in N = (1, 0) for many cases and for those with an arbitrary number of tensor multiplets [45] have near horizon geometries locally given by R 1,1 × T 4 , R 1,1 × K 3 or AdS 3 × S 3 .…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…The conjecture has been proven for various theories which include d = 11 [221], (massive) IIA [223,224] , IIB [222] and heterotic supergravities [225]. It has also been demonstrated for the minimal gauged N = 1 d = 5 supergravity [226], the N = 2 d = 4 gauged supergravity coupled to any number of vector fields [227] and the N = 1 d = 5 supergravity coupled to any number of vector fields [228].…”
Section: The Horizon Conjecturementioning
confidence: 87%