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Supersymmetric black holes in N=8 supergravity
We study the embedding of extreme (multi-) dilaton black hole solutions for the values of the parameter a=\sqrt{3},1,1/\sqrt{3},0 in N=4 and N=8 four-dimensional supergravity. For each black hole solution we find different embeddings in N=4 supergravity which have different numbers of unbroken super...
Autores principales: | , |
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Lenguaje: | eng |
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1995
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Acceso en línea: | https://dx.doi.org/10.1016/0550-3213(96)00112-5 http://cds.cern.ch/record/294819 |
_version_ | 1780888881473781760 |
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author | Khuri, Ramzi R. Ortin, Tomas |
author_facet | Khuri, Ramzi R. Ortin, Tomas |
author_sort | Khuri, Ramzi R. |
collection | CERN |
description | We study the embedding of extreme (multi-) dilaton black hole solutions for the values of the parameter a=\sqrt{3},1,1/\sqrt{3},0 in N=4 and N=8 four-dimensional supergravity. For each black hole solution we find different embeddings in N=4 supergravity which have different numbers of unbroken supersymmetries. When embedded in N=8 supergravity, all different embeddings of the same solution have the same number of unbroken supersymmetries. Thus, there is a relation between the value of the parameter a and the number of unbroken supersymmetries in N=8 supergravity, but not in N=4, and the different embeddings must be related by dualities of the N=8 theory which are not dualities of the N=4 theory. The only exception in this scheme is a {\it dyonic} embedding of the a=0 black-hole solution which seems to break all supersymmetries both in the N=4 and in the N=8 theories. |
id | cern-294819 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1995 |
record_format | invenio |
spelling | cern-2948192023-03-14T19:55:48Zdoi:10.1016/0550-3213(96)00112-5http://cds.cern.ch/record/294819engKhuri, Ramzi R.Ortin, TomasSupersymmetric black holes in N=8 supergravityParticle Physics - TheoryWe study the embedding of extreme (multi-) dilaton black hole solutions for the values of the parameter a=\sqrt{3},1,1/\sqrt{3},0 in N=4 and N=8 four-dimensional supergravity. For each black hole solution we find different embeddings in N=4 supergravity which have different numbers of unbroken supersymmetries. When embedded in N=8 supergravity, all different embeddings of the same solution have the same number of unbroken supersymmetries. Thus, there is a relation between the value of the parameter a and the number of unbroken supersymmetries in N=8 supergravity, but not in N=4, and the different embeddings must be related by dualities of the N=8 theory which are not dualities of the N=4 theory. The only exception in this scheme is a {\it dyonic} embedding of the a=0 black-hole solution which seems to break all supersymmetries both in the N=4 and in the N=8 theories.We study the embedding of extreme (multi-) dilaton black hole solutions for the values of the parameter $a=\sqrt{3},1,1/\sqrt{3},0$ in $N=4$ and $N=8$ four-dimensional supergravity. For each black hole solution we find different embeddings in $N=4$ supergravity which have different numbers of unbroken supersymmetries. When embedded in $N=8$ supergravity, all different embeddings of the same solution have the same number of unbroken supersymmetries. Thus, there is a relation between the value of the parameter $a$ and the number of unbroken supersymmetries in $N=8$ supergravity, but not in $N=4$, and the different embeddings must be related by dualities of the $N=8$ theory which are not dualities of the $N=4$ theory. The only exception in this scheme is a {\it dyonic} embedding of the $a=0$ black-hole solution which seems to break all supersymmetries both in the $N=4$ and in the $N=8$ theories.We study the embedding of extreme (multi-) dilaton black hole solutions for the values of the parameter a = √3, 1, 1/√3, 0 in N = 4 and N = 8 four-dimensional supergravity. For each black hole solution we find different embeddings in N = 4 supergravity which have different numbers of unbroken supersymmetries. When embedded in N = 8 supergravity, all different embeddings of the same solution have the same number of unbroken supersymmetries. Thus, there is a relation between the value of the parameter a and the number of unbroken supersymmetries in N = 8 supergravity, but not in N = 4, and the different embeddings must be related by dualities of the N = 8 theory which are not dualities of the N = 4 theory. The only exception in this scheme is a dyonic embedding of the a = 0 black-hole solution which seems to break all supersymmetries both in the N = 4 and in the N = 8 theories.hep-th/9512177CERN-TH-95-348MCGILL-95-62CERN-TH-95-348MCGILL-95-62oai:cds.cern.ch:2948191995-12-21 |
spellingShingle | Particle Physics - Theory Khuri, Ramzi R. Ortin, Tomas Supersymmetric black holes in N=8 supergravity |
title | Supersymmetric black holes in N=8 supergravity |
title_full | Supersymmetric black holes in N=8 supergravity |
title_fullStr | Supersymmetric black holes in N=8 supergravity |
title_full_unstemmed | Supersymmetric black holes in N=8 supergravity |
title_short | Supersymmetric black holes in N=8 supergravity |
title_sort | supersymmetric black holes in n=8 supergravity |
topic | Particle Physics - Theory |
url | https://dx.doi.org/10.1016/0550-3213(96)00112-5 http://cds.cern.ch/record/294819 |
work_keys_str_mv | AT khuriramzir supersymmetricblackholesinn8supergravity AT ortintomas supersymmetricblackholesinn8supergravity |