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Anisotropic domain walls
We find an anisotropic, non-supersymmetric generalization of the extreme supersymmetric domain walls of simple non-dilatonic supergravity theory. As opposed to the isotropic non- and ultra-extreme domain walls, the anisotropic non-extreme wall has the \emph{same} spatial topology as the extreme wall...
Autores principales: | , |
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Lenguaje: | eng |
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1996
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/0264-9381/14/7/017 http://cds.cern.ch/record/309472 |
_version_ | 1780889979181858816 |
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author | Jensen, Bjorn Soleng, Harald H. |
author_facet | Jensen, Bjorn Soleng, Harald H. |
author_sort | Jensen, Bjorn |
collection | CERN |
description | We find an anisotropic, non-supersymmetric generalization of the extreme supersymmetric domain walls of simple non-dilatonic supergravity theory. As opposed to the isotropic non- and ultra-extreme domain walls, the anisotropic non-extreme wall has the \emph{same} spatial topology as the extreme wall. The solution has naked singularities which vanish in the extreme limit. Since the Hawking temperature on the two sides is different, the generic solution is unstable to Hawking decay. |
id | cern-309472 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1996 |
record_format | invenio |
spelling | cern-3094722023-03-14T19:29:00Zdoi:10.1088/0264-9381/14/7/017http://cds.cern.ch/record/309472engJensen, BjornSoleng, Harald H.Anisotropic domain wallsGeneral Relativity and CosmologyWe find an anisotropic, non-supersymmetric generalization of the extreme supersymmetric domain walls of simple non-dilatonic supergravity theory. As opposed to the isotropic non- and ultra-extreme domain walls, the anisotropic non-extreme wall has the \emph{same} spatial topology as the extreme wall. The solution has naked singularities which vanish in the extreme limit. Since the Hawking temperature on the two sides is different, the generic solution is unstable to Hawking decay.We find an anisotropic, non-supersymmetric generalization of the extreme supersymmetric domain walls of simple non-dilatonic supergravity theory. As opposed to the isotropic non- and ultra-extreme domain walls, the anisotropic non-extreme wall has the \emph{same} spatial topology as the extreme wall. The solution has naked singularities which vanish in the extreme limit. Since the Hawking temperature on the two sides is different, the generic solution is unstable to Hawking decay.gr-qc/9608060CERN-TH-96-092CERN-TH-96-92CERN-TH-96-092oai:cds.cern.ch:3094721996-08-26 |
spellingShingle | General Relativity and Cosmology Jensen, Bjorn Soleng, Harald H. Anisotropic domain walls |
title | Anisotropic domain walls |
title_full | Anisotropic domain walls |
title_fullStr | Anisotropic domain walls |
title_full_unstemmed | Anisotropic domain walls |
title_short | Anisotropic domain walls |
title_sort | anisotropic domain walls |
topic | General Relativity and Cosmology |
url | https://dx.doi.org/10.1088/0264-9381/14/7/017 http://cds.cern.ch/record/309472 |
work_keys_str_mv | AT jensenbjorn anisotropicdomainwalls AT solengharaldh anisotropicdomainwalls |