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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...
Autores principales: | , , |
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Lenguaje: | eng |
Publicado: |
1995
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.52.R5412 http://cds.cern.ch/record/286302 |
_version_ | 1780888301364838400 |
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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. |
id | cern-286302 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1995 |
record_format | invenio |
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 |