All supersymmetric solutions of minimal supergravity in five- dimensions

By J. Gauntlett, J. Gutowski, C. Hull, Stathis Pakis, Harvey Reall. 2002

719 citations recorded by the source corpus.

All purely bosonic supersymmetric solutions of minimal supergravity in five dimensions are classified. The solutions preserve either one half or all of the supersymmetry. Explicit examples of new solutions are given, including a large family of plane-fronted waves and a maximally supersymmetric analogue of the Godel universe which lifts to a solution of 11-dimensional supergravity that preserves 20 supersymmetries.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/770e62f6a673f498b4c37bba6ba2e5ee5458bda1

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Citations in the corpus

General Concentric Black Rings (2004, methodology): “We use the classification of the most general supersymmetric solutions of D=5 gauged supergravity coupled to an arbitrary number of vector multiplets [21], generalising that of [22, 23].”
Black Saturn (2007, background): “The first order nature of the supersymmetry conditions [16, 17] makes the construction of multi-black hole solutions a fairly straightforward superposition of harmonic functions.”
Supersymmetric AdS5 solutions of type IIB supergravity (2005, methodology): “Once again, following [3, 4 , 5], we analyse the G-structure defined by the Killing spinors.”
Black holes as effective geometries (2008, background): “The latter require specifying a four-dimensional base metric that is restricted to be hyperkähler [76].”
Wormholes in AdS (2004, background): “solutions must have a timelike or null killing vector [ 17 ].”
G structures, fluxes and calibrations in M theory (2003, methodology): “Subsequent works have used this approach to analyse and classify supersymmetric backgrounds in various supergravity theories [2, 3, 4, 5, 6, 7, 8, 9, 10].”
Global structure of five-dimensional fuzzballs (2013, background): “2 BPS solutions The solutions of [88, 89, 10, 11, 13] are BPS, i.”
Holographic Protection of Chronology in Universes of the Godel Type (2002, background): “As remarked in [10], this solution is homogeneous, and in fact has a nine-dimensional group of bosonic isometries.”
Superstrings with intrinsic torsion (2003, background): “Similar ideas have been used to analyse other supergravity solutions in [12, 13, 14, 15, 16].”
Supersymmetric black rings and three-charge supertubes (2004, background): “t the roles of some coordinates, like ψ′ and z′, are exchanged relative to BMPV. We will revisit this issue in section 6.4. 9Formally, this is the same as the oxidation of BMPV: see equation (6.8) of [33] with u→ ψ′, ψ′ → 2z′′/q 3, φ→ χ. (Lens spaces do not arise from an asymptotically ﬂat BMPV blac”
Four-dimensional SCFTs from M5-branes (2012, background): “This has been shown for other supergravity theories in [55, 56, 57], but has not been shown for the maximal gauged supergravity in seven dimensions.”
Supersymmetric AdS5 solutions of M-theory (2004, background): “Essentially the same techniques have also proved very useful in determining the general form of supersymmetric solutions in various lower-dimensional supergravities [30]–[34].”
Habemus superstratum! A constructive proof of the existence of superstrata (2015, background): “ill describe later in this paper, we can then generalize this dictionary to the 1 8 -BPS (4-supercharge) D1-D5-P superstrata. Second, the equations that govern the superstrata solutions are wellknown [21,22], and can be organized in a linear fashion [23], and so this technique appears to 1In [2], do”
Supergravity microstates for BPS black holes and black rings (2005, background): “and K, generalizing the appendix in [13] patterned on [ 24 ].”
AdS 3 solutions of IIB supergravity from D3-branes (2005, neutral): “Contents”
Exotic Branes in String Theory (2012, neutral): “After such puffing up, the corresponding backreacted solution in supergravity is [91,94] ds(2)str = f −1 1 [ −(dt− A)(2) + (dx(4) − A)(2) + (f2 − 1)(dt− dx(4))(2) ] + dx(2) + dz(2), e = f−1 1 , B (2) = −(f−1 1 − 1)dt ∧ dx(4) + f−1 1 (dt− dx(4)) ∧ A, (5.”
Mergers and typical black hole microstates (2006, background): “The general BPS solutions with a positive-definite GH base were obtained in [4,7], and it is straightforward to adapt these solutions to generalized GH metrics that allow overall sign changes.”