Rotating black holes in 4d gauged supergravity

Gnecchi, Alessandra; Hristov, Kiril; Klemm, Dietmar; Toldo, Chiara; Vaughan, Owen

doi:10.1007/jhep01(2014)127

Cited by 101 publications

(144 citation statements)

References 88 publications

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“…The final equation to be imposed is the condition (3.4), so we compute each term individually 22) JHEP09 (2014)027 where (2.9) was used for the real part of the section and (3.17) was used repeatedly to simplify the result. We therefore find that (3.4) is satisfied if we set…”

Section: Jhep09(2014)027mentioning

confidence: 99%

Static BPS black holes in U(1) gauged supergravity

Katmadas

2014

J. High Energ. Phys.

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We consider the flow equations for 1/4-BPS asymptotically AdS 4 static black holes in Fayet-Iliopoulos gauged supergravity, using very special geometry identities to obtain a simplified form in the most general case. Under mild assumptions on the form of the solution, we analyse the flow equations and find an explicit solution for arbitrary gauging and charge vectors. Comparing with the corresponding attractor equations, we find that the solution is given in terms of exactly the same vector of parameters, implying that all regular attractors can be extended to full black hole solutions. We present explicit examples of black hole solutions with all complex scalars and allowed charges turned on, within the STU model and its truncations.

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Section: Jhep09(2014)027mentioning

confidence: 99%

Static BPS black holes in U(1) gauged supergravity

Katmadas

2014

J. High Energ. Phys.

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“…These rotating black holes were discovered respectively in [22] for F = −2i X 0 (X 1 ) 3 model and recently in [23,24] for the F = −iX 0 X 1 one. They have spherical horizon topology and are characterized by electromag-netic charges, mass and angular momentum.…”

Section: Introductionmentioning

confidence: 99%

“…We refer to [24] for details. Denoting once again the radial coordinate of the event horizon by q h , entropy and temperature read…”

Section: Thermodynamics Quantities and Scalar Asymptoticsmentioning

confidence: 99%

“…We consider the rotating purely magnetic AdS black holes of [24] arising from N = 2 abelian FI (electrically) gauged supergravity with prepotential F = −iX 0 X 1 . This model is a truncation of N = 4 SO(4) gauged fourdimensional supergravity, which was obtained by KaluzaKlein reduction of D = 11 supergravity on S 7 in [20,21].…”

Section: Rotating Black Hole Solution Of Thementioning

confidence: 99%

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Thermodynamics of spinningAdS4black holes in gauged supergravity

Toldo

2016

Phys. Rev. D

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In this paper we study the thermodynamics of rotating black hole solutions arising from fourdimensional gauged N = 2 supergravity. We analyze two different supergravity models, characterized by prepotentials F = −iX 0 X 1 and F = −2i X 0 (X 1 ) 3 . The black hole configurations are supported by electromagnetic charges and scalar fields with different kinds of boundary conditions. We perform our analysis in the canonical ensemble, where we find a first order phase transition for a suitable range of charges and angular momentum. We perform the thermodynamic stability check on the configurations. Using the holographic dictionary we interpret the phase transition in terms of expectation values of operators in the dual field theory, which pertains to the class of ABJM theories living on a rotating Einstein universe. We extend the analysis to dyonic configurations as well. Lastly, we show the computation of the on shell action and mass via holographic renormalization techniques.

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“…Due to the anticipated S-duality symmetry, this solution has the same metric form as the one with two independent electric-charges only, obtained in [32]. We also need to mention the solution containing one charge parameter less than the one in [31], but having general Fayet-Iliopoulos parameters [33].…”

Section: Introductionmentioning

confidence: 99%

An analysis of the wave equation for theU(1)²gauged supergravity black hole

Birkandan¹,

Cvetič²

2015

Class. Quantum Grav.

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Abstract. We study the massless Klein-Gordon equation in the background of the most general rotating dyonic AdS black hole in gauged N = 2, U (1) 2 gauged supergravity in D = 4, given by Chow and Compère [Phys. Rev. D89 (2014) 065003]. The angular part of the separable wave equation is of the Heun type, while the radial part is a Fuchsian equation with five regular singularities. The radial equation is further analyzed and written in a specific form, that reveals the pole structure of the horizon equation, whose residua are expressed in terms of the surface gravities and angular velocities associated with respective horizons. The near-horizon (near-)extremal limits of the solution are also studied, where the expected hidden conformal symmetry is revealed. Furthermore, we present the retarded Green's functions for these limiting cases. We also comment on the generality of the charge-dependent parts of the metric parameters and address some further examples of limiting cases.

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Rotating black holes in 4d gauged supergravity

Cited by 101 publications

References 88 publications

Static BPS black holes in U(1) gauged supergravity

Static BPS black holes in U(1) gauged supergravity

Thermodynamics of spinningAdS4black holes in gauged supergravity

An analysis of the wave equation for theU(1)²gauged supergravity black hole

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Rotating black holes in 4d gauged supergravity

Cited by 101 publications

References 88 publications

Static BPS black holes in U(1) gauged supergravity

Static BPS black holes in U(1) gauged supergravity

Thermodynamics of spinningAdS4black holes in gauged supergravity

An analysis of the wave equation for theU(1)2gauged supergravity black hole

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An analysis of the wave equation for theU(1)²gauged supergravity black hole