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N = 2 extremal black holes

It is shown that extremal magnetic black hole solutions of N = 2 supergravity coupled to vector multiplets X^\Lambda with a generic holomorphic prepotential F(X^\Lambda) can be described as supersymmetric solitons which interpolate between maximally symmetric limiting solutions at spatial infinity a...

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Detalles Bibliográficos
Autores principales: Ferrara, Sergio, Kallosh, Renata, Strominger, Andrew
Lenguaje:eng
Publicado: 1995
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.52.R5412
http://cds.cern.ch/record/286302
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author Ferrara, Sergio
Kallosh, Renata
Strominger, Andrew
author_facet Ferrara, Sergio
Kallosh, Renata
Strominger, Andrew
author_sort Ferrara, Sergio
collection CERN
description It is shown that extremal magnetic black hole solutions of N = 2 supergravity coupled to vector multiplets X^\Lambda with a generic holomorphic prepotential F(X^\Lambda) can be described as supersymmetric solitons which interpolate between maximally symmetric limiting solutions at spatial infinity and the horizon. A simple exact solution is found for the special case that the ratios of the X^\Lambda are real (imaginary), and it is seen that the logarithm of the conformal factor of the spatial metric equals the K\"{a}hler potential on the vector multiplet moduli space. Several examples are discussed in detail.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1995
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spelling cern-2863022019-09-30T06:29:59Zdoi:10.1103/PhysRevD.52.R5412http://cds.cern.ch/record/286302engFerrara, SergioKallosh, RenataStrominger, AndrewN = 2 extremal black holesParticle Physics - TheoryIt is shown that extremal magnetic black hole solutions of N = 2 supergravity coupled to vector multiplets X^\Lambda with a generic holomorphic prepotential F(X^\Lambda) can be described as supersymmetric solitons which interpolate between maximally symmetric limiting solutions at spatial infinity and the horizon. A simple exact solution is found for the special case that the ratios of the X^\Lambda are real (imaginary), and it is seen that the logarithm of the conformal factor of the spatial metric equals the K\"{a}hler potential on the vector multiplet moduli space. Several examples are discussed in detail.hep-th/9508072CERN-TH-95-211SU-ITP-95-16oai:cds.cern.ch:2863021995-08-15
spellingShingle Particle Physics - Theory
Ferrara, Sergio
Kallosh, Renata
Strominger, Andrew
N = 2 extremal black holes
title N = 2 extremal black holes
title_full N = 2 extremal black holes
title_fullStr N = 2 extremal black holes
title_full_unstemmed N = 2 extremal black holes
title_short N = 2 extremal black holes
title_sort n = 2 extremal black holes
topic Particle Physics - Theory
url https://dx.doi.org/10.1103/PhysRevD.52.R5412
http://cds.cern.ch/record/286302
work_keys_str_mv AT ferrarasergio n2extremalblackholes
AT kalloshrenata n2extremalblackholes
AT stromingerandrew n2extremalblackholes