All the supersymmetric solutions of<i>N</i>= 1,<i>d</i>= 5 ungauged supergravity

Bellorín, Jorge; Meessen, Patrick; Ortı́n, Tomás

doi:10.1088/1126-6708/2007/01/020

Cited by 59 publications

(153 citation statements)

References 73 publications

(103 reference statements)

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“…[7] all the supersymmetric solutions of minimal supergravity in d = 5 dimensions were determined. These results were immediately extended to the Abelian gauged case [8] and later on to general matter contents and couplings [9] (always in the minimal N = 2 supergravity). The spinorbilinear method was subsequently applied to other 4-dimensional [10]- [21], 6-dimensional [22], 7-dimensional [23], 11-dimensional [24] and, recently, to 3-dimensional [25] supergravities.…”

Section: Introductionmentioning

confidence: 77%

All the timelike supersymmetric solutions of all ungauged d = 4 supergravities

Meessen

Ortı́n

Vaulá

2010

J. High Energ. Phys.

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We determine the form of all timelike supersymmetric solutions of all N ≥ 2, d = 4 ungauged supergravities, for N ≤ 4 coupled to vector supermultiplets, using the Usp(n,n)-symmetric formulation of Andrianopoli, D'Auria and Ferrara and the spinor-bilinears method, while preserving the global symmetries of the theories all the way.As previously conjectured in the literature, the supersymmetric solutions are always associated to a truncation to an N = 2 theory that may include hypermultiplets, although fields which are eliminated in the truncations can have non-trivial values, as is required by the preservation of the global symmetry of the theories.The solutions are determined by a number of independent functions, harmonic in transverse space, which is twice the number of vector fields of the theory (n). The transverse space is flat if an only if the would-be hyperscalars of the associated N = 2 truncation are trivial.

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Section: Introductionmentioning

confidence: 77%

All the timelike supersymmetric solutions of all ungauged d = 4 supergravities

Meessen

Ortı́n

Vaulá

2010

J. High Energ. Phys.

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“…The very fresh result of [31] attests that solutions preserving only 1/8 of supersymmetry exist already in ungauged supergravity with hypers. In contrast, without hypermultiplet coupled the supersymmetric configuration preserves at least two supercharges [62].…”

Section: Discussionmentioning

confidence: 99%

“…Nowadays there is a renew interest for a more systematical understanding of BPS solutions with hypermultiplets. The full classification in N = 2 ungauged supergravity has been achieved in four and five dimensions in [30,31]. Some steps towards this goal in the more complicated gauged case had been previously performed in five dimensions [32,33,34].…”

Section: Introductionmentioning

confidence: 99%

Null deformed domain wall

Celi

2007

J. High Energy Phys.

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We study null 1/4 BPS deformations of flat Domain Wall solutions (NDDW) in N = 2, d = 5 gauged supergravity with hypermultiplets and vector multiplets coupled. These are uncharged timedependent configurations and contain as special case, 1/2 supersymmetric flat domain walls (DW) and, as well, 1/2 BPS null solutions of the ungauged supergravity. Combining our analysis with the classification method initiated by Gauntlett et al., we prove that all the possible deformations of the DW have origin in the hypermultiplet sector or/and are null. Here, we classify all the null deformations: we show that they naturally organize in "gauging" (v-deformation) and "non gauging" (u-deformation). They have different properties: only in presence of v-deformation the solution is supported by a timedependent scalar potential. Furthermore we show that u-deformation forces the number of multiplets coupled to be different by one. We discuss the general procedure for constructing explicit solutions, stressing the crucial role taken by the integrability conditions of the scalars as spacetime functions. Two analytical solutions are presented. Finally, we comment on the holographic applications of NDDW, in relation with the recently proposed timedependent AdS/CFT.

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“…Let us consider the metric as written in (3.19). In the purely spatial part there are no singularities in these surfaces because the product f −1 H defines a finite positive quantity, 47) JHEP11 (2016)152 and I is also regular, as easily seen from its expression in terms of the seed functions (3.22). Of course, this is only possible because lim H→0 f ∼ 0 and this, in particular, means that the critical surfaces are determined by the vanishing of the norm of the Killing vector that generates time translations,…”

Section: Critical Surfacesmentioning

confidence: 91%

“…11 Those were first considered in [46], see [26,32,47,48] for more detailed expositions in our same conventions. 12 Here the index I is for labeling each one of these vectors.…”

Section: Jhep11(2016)152mentioning

confidence: 99%

Non-Abelian bubbles in microstate geometries

Ramírez

2016

J. High Energ. Phys.

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We find the first smooth bubbling microstate geometries with non-Abelian fields. The solutions constitute an extension of the BPS three-charge smooth microstates. These consist in general families of regular supersymmetric solutions with non-trivial topology, i.e. bubbles, of N = 1, d = 5 Super-Einstein-Yang-Mills theory, having the asymptotic charges of a black hole or black ring but with no horizon. The non-Abelian fields make their presence at the very heart of the microstate structure: the physical size of the bubbles is affected by the non-Abelian topological charge they carry, which combines with the Abelian flux threading the bubbles to hold them up. Interestingly the non-Abelian fields carry a set of adjustable continuous parameters that do not alter the asymptotics of the solutions but modify the local geometry. This feature can be used to obtain a classically infinite number of microstate solutions with the asymptotics of a single black hole or black ring.

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All the supersymmetric solutions ofN= 1,d= 5 ungauged supergravity

Cited by 59 publications

References 73 publications

All the timelike supersymmetric solutions of all ungauged d = 4 supergravities

All the timelike supersymmetric solutions of all ungauged d = 4 supergravities

Null deformed domain wall

Non-Abelian bubbles in microstate geometries

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