Supersymmetric multi-charge<i>AdS</i><sub>5</sub>black holes

Kunduri, Hari K.; Lucietti, James; Reall, Harvey S.

doi:10.1088/1126-6708/2006/04/036

Cited by 218 publications

(409 citation statements)

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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%

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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%

“…These solutions can be embedded in the numerical solutions constructed in [29] for the N = 2 theory, whose potential reduce to the 4 + potential after identifying the two scalars λ 1 = λ 2 = λ. 16 15 The corresponding projections for full black string solutions in the N = 8 language are:…”

Section: Holographic Rg Flowsmentioning

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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“…This restriction remains in generalizations involving two different angular momenta [8,9]. This situation is in contrast with the asymptotically flat 5D space-time, where BPS solutions exist for arbitrary values of the angular momenta and charges within certain…”

Section: Introductionmentioning

confidence: 97%

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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“…These solutions have been further generalised in [3,4,5,6]. When lifted to 10-dimensional solutions of type IIB, these geometries asymptote to the maximally supersymmetric AdS 5 × S 5 solution and preserve just two of the 32 supersymmetries [7].…”

Section: Introductionmentioning

confidence: 99%

At the horizon of a supersymmetricAdS₅black hole: Isometries and half-BPS giants

Sinha¹,

Sonner²,

Suryanarayana³

2007

J. High Energy Phys.

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The near-horizon geometry of an asymptotically AdS 5 supersymmetric black hole discovered by Gutowski and Reall is analysed. After lifting the solution to 10 dimensions, we explicitly solve the Killing spinor equations in both Poincaré and global coordinates. It is found that exactly four supersymmetries are preserved which is twice the number for the full black hole. The full set of isometries is constructed and the isometry supergroup is shown to be SU (1, 1|1) × SU (2) × U (3). We further study half-BPS configurations of D3-branes in the near-horizon geometry in Poincaré and global coordinates. Both giant graviton probes and dual giant graviton probes are found.

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Supersymmetric multi-chargeAdS₅black holes

Cited by 218 publications

References 18 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

At the horizon of a supersymmetricAdS₅black hole: Isometries and half-BPS giants

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Supersymmetric multi-chargeAdS5black holes

Cited by 218 publications

References 18 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

At the horizon of a supersymmetricAdS5black hole: Isometries and half-BPS giants

Contact Info

Product

Resources

About

Supersymmetric multi-chargeAdS₅black holes

At the horizon of a supersymmetricAdS₅black hole: Isometries and half-BPS giants