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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...

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Detalles Bibliográficos
Autores principales: Jensen, Bjorn, Soleng, Harald H.
Lenguaje:eng
Publicado: 1996
Materias:
Acceso en línea:https://dx.doi.org/10.1088/0264-9381/14/7/017
http://cds.cern.ch/record/309472
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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.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1996
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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