116 research outputs found

    Positive mass theorem in extended supergravities

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    Following the Witten-Nester formalism, we present a useful prescription using Weyl spinors towards the positivity of mass. As a generalization of arXiv:1310.1663, we show that some "positivity conditions" must be imposed upon the gauge connections appearing in the supercovariant derivative acting on spinors. A complete classification of the connection fulfilling the positivity conditions is given. It turns out that these positivity conditions are indeed satisfied for a number of extended supergravity theories. It is shown that the positivity property holds for the Einstein-complex scalar system, provided that the target space is Hodge-Kahler and the potential is expressed in terms of the superpotential. In the Einstein-Maxwell-dilaton theory with a dilaton potential, the dilaton coupling function and the superpotential are fixed by the positive mass property. We also explore the N=8N=8 gauged supergravity and demonstrate that the positivity of the mass holds independently of the gaugings and the deformation parameters.Comment: v2: 22 pages, typos fixed and refs added, a section discussing the Einstein-Maxwell-dilaton theory added, an appendix classifies the connection satisfying positivity conditions, accepted for publication in NP

    Black holes in an expanding universe and supersymmetry

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    This paper analyzes the supersymmetric solutions to five and six-dimensional minimal (un)gauged supergravities for which the bilinear Killing vector constructed from the Killing spinor is null. We focus on the spacetimes which admit an additional SO(1,1){\rm SO}(1,1) boost symmetry. Upon the toroidal dimensional reduction along the Killing vector corresponding to the boost, we show that the solution in the ungauged case describes a charged, nonextremal black hole in a Friedmann-Lema\^itre-Robertson-Walker (FLRW) universe with an expansion driven by a massless scalar field. For the gauged case, the solution corresponds to a charged, nonextremal black hole embedded conformally into a Kantowski-Sachs universe. It turns out that these dimensional reductions break supersymmetry since the bilinear Killing vector and the Killing vector corresponding to the boost fail to commute. This represents a new mechanism of supersymmetry breaking that has not been considered in the literature before.Comment: 9 pages, 1 figure; v2: minor modifications, published version in PL

    Geometry of Killing spinors in neutral signature

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    We classify the supersymmetric solutions of minimal N=2N=2 gauged supergravity in four dimensions with neutral signature. They are distinguished according to the sign of the cosmological constant and whether the vector field constructed as a bilinear of the Killing spinor is null or non-null. In neutral signature the bilinear vector field can be spacelike, which is a new feature not arising in Lorentzian signature. In the Λ<0\Lambda<0 non-null case, the canonical form of the metric is described by a fibration over a three-dimensional base space that has U(1)\text{U}(1) holonomy with torsion. We find that a generalized monopole equation determines the twist of the bilinear Killing field, which is reminiscent of an Einstein-Weyl structure. If, moreover, the electromagnetic field strength is self-dual, one gets the Kleinian signature analogue of the Przanowski-Tod class of metrics, namely a pseudo-hermitian spacetime determined by solutions of the continuous Toda equation, conformal to a scalar-flat pseudo-K\"ahler manifold, and admitting in addition a charged conformal Killing spinor. In the Λ<0\Lambda<0 null case, the supersymmetric solutions define an integrable null K\"ahler structure. In the Λ>0\Lambda>0 non-null case, the manifold is a fibration over a Lorentzian Gauduchon-Tod base space. Finally, in the Λ>0\Lambda>0 null class, the metric is contained in the Kundt family, and it turns out that the holonomy is reduced to Sim(1)×Sim(1){\rm Sim}(1)\times{\rm Sim}(1). There appear no self-dual solutions in the null class for either sign of the cosmological constant.Comment: 40 pages, uses JHEP3.cls. v2: Appendix and ref. added. v3: Published versio
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