Stable p-branes in Chern-Simons AdS supergravities
- Autores
- Edelstein, Jose Daniel; Garbarz, Alan Nicolás; Mišković, Olivera; Zanelli, Jorge
- Año de publicación
- 2010
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We construct static codimension-two branes in any odd dimension D, with a negative cosmological constant, and show that they are exact solutions of Chern-Simons (super)gravity theory for (super)AdSD coupled to external sources. The stability of these solutions is analyzed by counting the number of preserved supersymmetries. It is shown that static massive (D 3)-branes are unstable unless some suitable gauge fields are added and the brane is extremal. In particular, in three dimensions, a 0-brane is recognized as the negative mass counterpart of the Ban˜ados-Teitelboim-Zanelli black hole. For these 0- branes, we write explicitly magnetically charged Bogomol’nyi-Prasad-Sommerfield states with various numbers of preserved supersymmetries within the OSpðp j 2Þ OSpðq j 2Þ supergroups. In five dimensions, we prove that stable 2-branes with magnetic charge always exist for the generic supergroup SUð2; 4 j NÞ, where N 4. For the special case N ¼ 4, in which Chern-Simons supergravity requires the addition of a nontrivial gauge field configuration in order to preserve the maximal number of degrees of freedom, we show for two different static 2-branes that they are Bogomol’nyi-Prasad-Sommerfield states (one of which is the ground state), and from the corresponding algebra of charges we show that the energy is bounded from below. In higher dimensions, our results admit a straightforward generalization, although there are presumably more solutions corresponding to different intersections of the elementary objects.
Fil: Edelstein, Jose Daniel. Universidad de Santiago de Compostela; España. Centro de Estudios Científicos; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Garbarz, Alan Nicolás. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Mišković, Olivera. Pontificia Universidad Catolica de Valparaiso; Chile. Max-Planck-Institut für Gravitationsphysik; Alemania
Fil: Zanelli, Jorge. Centro de Estudios Científicos; Chile - Materia
-
Chern-Simons
Branes - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/16538
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Stable p-branes in Chern-Simons AdS supergravitiesEdelstein, Jose DanielGarbarz, Alan NicolásMišković, OliveraZanelli, JorgeChern-SimonsBraneshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We construct static codimension-two branes in any odd dimension D, with a negative cosmological constant, and show that they are exact solutions of Chern-Simons (super)gravity theory for (super)AdSD coupled to external sources. The stability of these solutions is analyzed by counting the number of preserved supersymmetries. It is shown that static massive (D 3)-branes are unstable unless some suitable gauge fields are added and the brane is extremal. In particular, in three dimensions, a 0-brane is recognized as the negative mass counterpart of the Ban˜ados-Teitelboim-Zanelli black hole. For these 0- branes, we write explicitly magnetically charged Bogomol’nyi-Prasad-Sommerfield states with various numbers of preserved supersymmetries within the OSpðp j 2Þ OSpðq j 2Þ supergroups. In five dimensions, we prove that stable 2-branes with magnetic charge always exist for the generic supergroup SUð2; 4 j NÞ, where N 4. For the special case N ¼ 4, in which Chern-Simons supergravity requires the addition of a nontrivial gauge field configuration in order to preserve the maximal number of degrees of freedom, we show for two different static 2-branes that they are Bogomol’nyi-Prasad-Sommerfield states (one of which is the ground state), and from the corresponding algebra of charges we show that the energy is bounded from below. In higher dimensions, our results admit a straightforward generalization, although there are presumably more solutions corresponding to different intersections of the elementary objects.Fil: Edelstein, Jose Daniel. Universidad de Santiago de Compostela; España. Centro de Estudios Científicos; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Garbarz, Alan Nicolás. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Mišković, Olivera. Pontificia Universidad Catolica de Valparaiso; Chile. Max-Planck-Institut für Gravitationsphysik; AlemaniaFil: Zanelli, Jorge. Centro de Estudios Científicos; ChileAmerican Physical Society2010-08info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/16538Edelstein, Jose Daniel; Garbarz, Alan Nicolás; Mišković, Olivera; Zanelli, Jorge; Stable p-branes in Chern-Simons AdS supergravities; American Physical Society; Physical Review D: Particles, Fields, Gravitation And Cosmology; 82; 4; 8-2010; 1-24; 0440531550-7998enginfo:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.82.044053info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.82.044053info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1006.3753info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-03T09:51:46Zoai:ri.conicet.gov.ar:11336/16538instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-03 09:51:46.74CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Stable p-branes in Chern-Simons AdS supergravities |
title |
Stable p-branes in Chern-Simons AdS supergravities |
spellingShingle |
Stable p-branes in Chern-Simons AdS supergravities Edelstein, Jose Daniel Chern-Simons Branes |
title_short |
Stable p-branes in Chern-Simons AdS supergravities |
title_full |
Stable p-branes in Chern-Simons AdS supergravities |
title_fullStr |
Stable p-branes in Chern-Simons AdS supergravities |
title_full_unstemmed |
Stable p-branes in Chern-Simons AdS supergravities |
title_sort |
Stable p-branes in Chern-Simons AdS supergravities |
dc.creator.none.fl_str_mv |
Edelstein, Jose Daniel Garbarz, Alan Nicolás Mišković, Olivera Zanelli, Jorge |
author |
Edelstein, Jose Daniel |
author_facet |
Edelstein, Jose Daniel Garbarz, Alan Nicolás Mišković, Olivera Zanelli, Jorge |
author_role |
author |
author2 |
Garbarz, Alan Nicolás Mišković, Olivera Zanelli, Jorge |
author2_role |
author author author |
dc.subject.none.fl_str_mv |
Chern-Simons Branes |
topic |
Chern-Simons Branes |
purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
dc.description.none.fl_txt_mv |
We construct static codimension-two branes in any odd dimension D, with a negative cosmological constant, and show that they are exact solutions of Chern-Simons (super)gravity theory for (super)AdSD coupled to external sources. The stability of these solutions is analyzed by counting the number of preserved supersymmetries. It is shown that static massive (D 3)-branes are unstable unless some suitable gauge fields are added and the brane is extremal. In particular, in three dimensions, a 0-brane is recognized as the negative mass counterpart of the Ban˜ados-Teitelboim-Zanelli black hole. For these 0- branes, we write explicitly magnetically charged Bogomol’nyi-Prasad-Sommerfield states with various numbers of preserved supersymmetries within the OSpðp j 2Þ OSpðq j 2Þ supergroups. In five dimensions, we prove that stable 2-branes with magnetic charge always exist for the generic supergroup SUð2; 4 j NÞ, where N 4. For the special case N ¼ 4, in which Chern-Simons supergravity requires the addition of a nontrivial gauge field configuration in order to preserve the maximal number of degrees of freedom, we show for two different static 2-branes that they are Bogomol’nyi-Prasad-Sommerfield states (one of which is the ground state), and from the corresponding algebra of charges we show that the energy is bounded from below. In higher dimensions, our results admit a straightforward generalization, although there are presumably more solutions corresponding to different intersections of the elementary objects. Fil: Edelstein, Jose Daniel. Universidad de Santiago de Compostela; España. Centro de Estudios Científicos; Chile. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Garbarz, Alan Nicolás. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina Fil: Mišković, Olivera. Pontificia Universidad Catolica de Valparaiso; Chile. Max-Planck-Institut für Gravitationsphysik; Alemania Fil: Zanelli, Jorge. Centro de Estudios Científicos; Chile |
description |
We construct static codimension-two branes in any odd dimension D, with a negative cosmological constant, and show that they are exact solutions of Chern-Simons (super)gravity theory for (super)AdSD coupled to external sources. The stability of these solutions is analyzed by counting the number of preserved supersymmetries. It is shown that static massive (D 3)-branes are unstable unless some suitable gauge fields are added and the brane is extremal. In particular, in three dimensions, a 0-brane is recognized as the negative mass counterpart of the Ban˜ados-Teitelboim-Zanelli black hole. For these 0- branes, we write explicitly magnetically charged Bogomol’nyi-Prasad-Sommerfield states with various numbers of preserved supersymmetries within the OSpðp j 2Þ OSpðq j 2Þ supergroups. In five dimensions, we prove that stable 2-branes with magnetic charge always exist for the generic supergroup SUð2; 4 j NÞ, where N 4. For the special case N ¼ 4, in which Chern-Simons supergravity requires the addition of a nontrivial gauge field configuration in order to preserve the maximal number of degrees of freedom, we show for two different static 2-branes that they are Bogomol’nyi-Prasad-Sommerfield states (one of which is the ground state), and from the corresponding algebra of charges we show that the energy is bounded from below. In higher dimensions, our results admit a straightforward generalization, although there are presumably more solutions corresponding to different intersections of the elementary objects. |
publishDate |
2010 |
dc.date.none.fl_str_mv |
2010-08 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/16538 Edelstein, Jose Daniel; Garbarz, Alan Nicolás; Mišković, Olivera; Zanelli, Jorge; Stable p-branes in Chern-Simons AdS supergravities; American Physical Society; Physical Review D: Particles, Fields, Gravitation And Cosmology; 82; 4; 8-2010; 1-24; 044053 1550-7998 |
url |
http://hdl.handle.net/11336/16538 |
identifier_str_mv |
Edelstein, Jose Daniel; Garbarz, Alan Nicolás; Mišković, Olivera; Zanelli, Jorge; Stable p-branes in Chern-Simons AdS supergravities; American Physical Society; Physical Review D: Particles, Fields, Gravitation And Cosmology; 82; 4; 8-2010; 1-24; 044053 1550-7998 |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.82.044053 info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.82.044053 info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1006.3753 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
American Physical Society |
publisher.none.fl_str_mv |
American Physical Society |
dc.source.none.fl_str_mv |
reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
reponame_str |
CONICET Digital (CONICET) |
collection |
CONICET Digital (CONICET) |
instname_str |
Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.name.fl_str_mv |
CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
repository.mail.fl_str_mv |
dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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13.13397 |