General supersymmetric<i>AdS</i><sub>5</sub>black holes

Gutowski, J.; Reall, Harvey S.

doi:10.1088/1126-6708/2004/04/048

Cited by 376 publications

(793 citation statements)

References 33 publications

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“…Although N = 8 was formulated back in 80's [1][2][3], very few analytic solutions have been constructed explicitely in this theory [4], since most of them are also solutions to the less supersymmetric truncations, which are more straightforward to approach [5][6][7][8][9][10][11][12][13][14][15][16][17][18][19].…”

Section: Jhep03(2014)057mentioning

confidence: 99%

“…Notice that we have a large variety of possible attractor geometries, and for each geometry we have a two dimensional moduli space. 12 As we already mentioned there are two interesting subsets of solutions in the moduli space, which we will analyze later on: those that can be connected to infinity with a full analytic solution and those that are BPS.…”

Section: Black String Attractorsmentioning

confidence: 99%

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Attractors, black objects and holographic RG flows in 5d maximal gauged supergravities

Hristov

Rota

2014

J. High Energ. Phys.

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We perform a systematic search for static solutions in different sectors of 5d N = 8 supergravities with compact and non-compact gauged R-symmetry groups, finding new and listing already known backgrounds. Due to the variety of possible gauge groups and resulting scalar potentials, the maximally symmetric vacua we encounter in these theories can be Minkowski, de Sitter, or anti-de Sitter. There exist BPS and non-BPS near-horizon geometries and full solutions with all these three types of asymptotics, corresponding to black holes, branes, strings, rings, and other black objects with more exotic horizon topologies, supported by U(1) and SU(2) charges. The asymptotically AdS 5 solutions also have a clear holographic interpretation as RG flows of field theories on D3 branes, wrapped on compact 2-and 3-manifolds.

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Section: Jhep03(2014)057mentioning

confidence: 99%

Section: Black String Attractorsmentioning

confidence: 99%

Attractors, black objects and holographic RG flows in 5d maximal gauged supergravities

Hristov

Rota

2014

J. High Energ. Phys.

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“…In terms of the SU(2) × U(1) symmetric ansatz used in [47,48,7], slightly generalized to include an arbitrary lapse function N (ρ) and Chern class k, In this section, we specialize to the case of minimal N = 1 supergravity in 5 dimensions, possibly gauged, and restrict to stationary solutions with SU(2) × U(1) group of isometries.…”

Section: Jhep05(2008)045mentioning

confidence: 99%

“…Supersymmetric rotating black holes in minimal D = 5 gauged supergravity were constructed in [6], and extended to general D = 5 gauged supergravity in [7]. In the case of minimal supergravity, the solution is given by…”

Section: Jhep05(2008)045mentioning

confidence: 99%

5D black holes and non-linear sigma models

Berkooz

Pioline

2008

J. High Energy Phys.

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Stationary solutions of 5D supergravity with U(1) isometry can be efficiently studied by dimensional reduction to three dimensions, where they reduce to solutions to a locally supersymmetric non-linear sigma model. We generalize this procedure to 5D gauged supergravity, and identify the corresponding gauging in 3D. We pay particular attention to the case where the Killing spinor is non constant along the fibration, which results, even for ungauged supergravity in 5D, in an additional gauging in 3D, without introducing any extra potential. We further study SU(2) × U(1) symmetric solutions, which correspond to geodesic motion on the sigma model (with potential in the gauged case). We identify and study the algebra of BPS constraints relevant for the Breckenridge-Myers-Peet-Vafa black hole, the Gutowski-Reall black hole and several other BPS solutions, and obtain the corresponding radial wave functions in the semi-classical approximation.

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“…For example, masses of rotating supersymmetric AdS 5 black holes [32,33] were recently considered in [27]. It may also be of interest to apply the above methods in examining the properties of the five-dimensional black ring solutions [34]- [37].…”

Section: Jhep05(2005)034mentioning

confidence: 99%

Black hole mass and Hamilton-Jacobi counterterms

Batrachenko¹,

Liu²,

McNees³

et al. 2005

J. High Energy Phys.

116

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Abstract:We apply the method of holographic renormalization to computing black hole masses in asymptotically anti-de Sitter spaces. In particular, we demonstrate that the Hamilton-Jacobi approach to obtaining the boundary action yields a set of counterterms sufficient to render the masses finite for four, five, six and seven-dimensional R-charged black holes in gauged supergravities. In addition, we prove that the familiar black hole thermodynamical expression Ω = E − T S − Φ I Q I continues to hold in general in the presence of arbitrary matter couplings to gravity.

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General supersymmetricAdS₅black holes

Cited by 376 publications

References 33 publications

Attractors, black objects and holographic RG flows in 5d maximal gauged supergravities

Attractors, black objects and holographic RG flows in 5d maximal gauged supergravities

5D black holes and non-linear sigma models

Black hole mass and Hamilton-Jacobi counterterms

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General supersymmetricAdS5black holes

Cited by 376 publications

References 33 publications

Attractors, black objects and holographic RG flows in 5d maximal gauged supergravities

Attractors, black objects and holographic RG flows in 5d maximal gauged supergravities

5D black holes and non-linear sigma models

Black hole mass and Hamilton-Jacobi counterterms

Contact Info

Product

Resources

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General supersymmetricAdS₅black holes