Simple compactifications and black p-branes in Gauss-Bonnet and Lovelock theories
- Autores
- Giribet, Gaston Enrique; Oliva, Julio; Ricardo Troncoso
- Año de publicación
- 2006
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- We look for the existence of asymptotically flat simple compactifications of the form D-p × Tp in D-dimensional gravity theories with higher powers of the curvature. Assuming the manifold D-p to be spherically symmetric, it is shown that the Einstein-Gauss-Bonnet theory admits this class of solutions only for the pure Einstein-Hilbert or Gauss-Bonnet Lagrangians, but not for an arbitrary linear combination of them. Once these special cases have been selected, the requirement of spherical symmetry is no longer relevant since actually any solution of the pure Einstein or pure Gauss-Bonnet theories can then be toroidally extended to higher dimensions. Depending on p and the spacetime dimension, the metric on D-p may describe a black hole or a spacetime with a conical singularity, so that the whole spacetime describes a black or a cosmic p-brane, respectively. For the purely Gauss-Bonnet theory it is shown that, if D-p is four-dimensional, a new exotic class of black hole solutions exists, for which spherical symmetry can be relaxed. Under the same assumptions, it is also shown that simple compactifications acquire a similar structure for a wide class of theories among the Lovelock family which accepts this toroidal extension. The thermodynamics of black p-branes is also discussed, and it is shown that a thermodynamical analogue of the Gregory-Laflamme transition always occurs regardless the spacetime dimension or the theory considered, hence not only for General Relativity. Relaxing the asymptotically flat behavior, it is also shown that exact black brane solutions exist within a very special class of Lovelock theories. © SISSA 2006.
Fil: Giribet, Gaston Enrique. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina
Fil: Oliva, Julio. Universidad de Concepción; Chile
Fil: Ricardo Troncoso. Centro de Estudios Fisicos; Chile - Materia
-
BLACK HOLES
CLASSICAL THEORIES OF GRAVITY
P-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:11336/74232
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Simple compactifications and black p-branes in Gauss-Bonnet and Lovelock theoriesGiribet, Gaston EnriqueOliva, JulioRicardo TroncosoBLACK HOLESCLASSICAL THEORIES OF GRAVITYP-BRANEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We look for the existence of asymptotically flat simple compactifications of the form D-p × Tp in D-dimensional gravity theories with higher powers of the curvature. Assuming the manifold D-p to be spherically symmetric, it is shown that the Einstein-Gauss-Bonnet theory admits this class of solutions only for the pure Einstein-Hilbert or Gauss-Bonnet Lagrangians, but not for an arbitrary linear combination of them. Once these special cases have been selected, the requirement of spherical symmetry is no longer relevant since actually any solution of the pure Einstein or pure Gauss-Bonnet theories can then be toroidally extended to higher dimensions. Depending on p and the spacetime dimension, the metric on D-p may describe a black hole or a spacetime with a conical singularity, so that the whole spacetime describes a black or a cosmic p-brane, respectively. For the purely Gauss-Bonnet theory it is shown that, if D-p is four-dimensional, a new exotic class of black hole solutions exists, for which spherical symmetry can be relaxed. Under the same assumptions, it is also shown that simple compactifications acquire a similar structure for a wide class of theories among the Lovelock family which accepts this toroidal extension. The thermodynamics of black p-branes is also discussed, and it is shown that a thermodynamical analogue of the Gregory-Laflamme transition always occurs regardless the spacetime dimension or the theory considered, hence not only for General Relativity. Relaxing the asymptotically flat behavior, it is also shown that exact black brane solutions exist within a very special class of Lovelock theories. © SISSA 2006.Fil: Giribet, Gaston Enrique. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; ArgentinaFil: Oliva, Julio. Universidad de Concepción; ChileFil: Ricardo Troncoso. Centro de Estudios Fisicos; ChileIOP Publishing2006-12info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/74232Giribet, Gaston Enrique; Oliva, Julio; Ricardo Troncoso; Simple compactifications and black p-branes in Gauss-Bonnet and Lovelock theories; IOP Publishing; Journal of High Energy Physics; 2006; 5; 12-2006; 1-191029-8479CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1088/1126-6708/2006/05/007info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:36:03Zoai:ri.conicet.gov.ar:11336/74232instacron: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:34982025-09-29 09:36:04.121CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Simple compactifications and black p-branes in Gauss-Bonnet and Lovelock theories |
title |
Simple compactifications and black p-branes in Gauss-Bonnet and Lovelock theories |
spellingShingle |
Simple compactifications and black p-branes in Gauss-Bonnet and Lovelock theories Giribet, Gaston Enrique BLACK HOLES CLASSICAL THEORIES OF GRAVITY P-BRANES |
title_short |
Simple compactifications and black p-branes in Gauss-Bonnet and Lovelock theories |
title_full |
Simple compactifications and black p-branes in Gauss-Bonnet and Lovelock theories |
title_fullStr |
Simple compactifications and black p-branes in Gauss-Bonnet and Lovelock theories |
title_full_unstemmed |
Simple compactifications and black p-branes in Gauss-Bonnet and Lovelock theories |
title_sort |
Simple compactifications and black p-branes in Gauss-Bonnet and Lovelock theories |
dc.creator.none.fl_str_mv |
Giribet, Gaston Enrique Oliva, Julio Ricardo Troncoso |
author |
Giribet, Gaston Enrique |
author_facet |
Giribet, Gaston Enrique Oliva, Julio Ricardo Troncoso |
author_role |
author |
author2 |
Oliva, Julio Ricardo Troncoso |
author2_role |
author author |
dc.subject.none.fl_str_mv |
BLACK HOLES CLASSICAL THEORIES OF GRAVITY P-BRANES |
topic |
BLACK HOLES CLASSICAL THEORIES OF GRAVITY P-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 look for the existence of asymptotically flat simple compactifications of the form D-p × Tp in D-dimensional gravity theories with higher powers of the curvature. Assuming the manifold D-p to be spherically symmetric, it is shown that the Einstein-Gauss-Bonnet theory admits this class of solutions only for the pure Einstein-Hilbert or Gauss-Bonnet Lagrangians, but not for an arbitrary linear combination of them. Once these special cases have been selected, the requirement of spherical symmetry is no longer relevant since actually any solution of the pure Einstein or pure Gauss-Bonnet theories can then be toroidally extended to higher dimensions. Depending on p and the spacetime dimension, the metric on D-p may describe a black hole or a spacetime with a conical singularity, so that the whole spacetime describes a black or a cosmic p-brane, respectively. For the purely Gauss-Bonnet theory it is shown that, if D-p is four-dimensional, a new exotic class of black hole solutions exists, for which spherical symmetry can be relaxed. Under the same assumptions, it is also shown that simple compactifications acquire a similar structure for a wide class of theories among the Lovelock family which accepts this toroidal extension. The thermodynamics of black p-branes is also discussed, and it is shown that a thermodynamical analogue of the Gregory-Laflamme transition always occurs regardless the spacetime dimension or the theory considered, hence not only for General Relativity. Relaxing the asymptotically flat behavior, it is also shown that exact black brane solutions exist within a very special class of Lovelock theories. © SISSA 2006. Fil: Giribet, Gaston Enrique. Consejo Nacional de Investigaciones Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Física de Buenos Aires. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Física de Buenos Aires; Argentina Fil: Oliva, Julio. Universidad de Concepción; Chile Fil: Ricardo Troncoso. Centro de Estudios Fisicos; Chile |
description |
We look for the existence of asymptotically flat simple compactifications of the form D-p × Tp in D-dimensional gravity theories with higher powers of the curvature. Assuming the manifold D-p to be spherically symmetric, it is shown that the Einstein-Gauss-Bonnet theory admits this class of solutions only for the pure Einstein-Hilbert or Gauss-Bonnet Lagrangians, but not for an arbitrary linear combination of them. Once these special cases have been selected, the requirement of spherical symmetry is no longer relevant since actually any solution of the pure Einstein or pure Gauss-Bonnet theories can then be toroidally extended to higher dimensions. Depending on p and the spacetime dimension, the metric on D-p may describe a black hole or a spacetime with a conical singularity, so that the whole spacetime describes a black or a cosmic p-brane, respectively. For the purely Gauss-Bonnet theory it is shown that, if D-p is four-dimensional, a new exotic class of black hole solutions exists, for which spherical symmetry can be relaxed. Under the same assumptions, it is also shown that simple compactifications acquire a similar structure for a wide class of theories among the Lovelock family which accepts this toroidal extension. The thermodynamics of black p-branes is also discussed, and it is shown that a thermodynamical analogue of the Gregory-Laflamme transition always occurs regardless the spacetime dimension or the theory considered, hence not only for General Relativity. Relaxing the asymptotically flat behavior, it is also shown that exact black brane solutions exist within a very special class of Lovelock theories. © SISSA 2006. |
publishDate |
2006 |
dc.date.none.fl_str_mv |
2006-12 |
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/11336/74232 Giribet, Gaston Enrique; Oliva, Julio; Ricardo Troncoso; Simple compactifications and black p-branes in Gauss-Bonnet and Lovelock theories; IOP Publishing; Journal of High Energy Physics; 2006; 5; 12-2006; 1-19 1029-8479 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/74232 |
identifier_str_mv |
Giribet, Gaston Enrique; Oliva, Julio; Ricardo Troncoso; Simple compactifications and black p-branes in Gauss-Bonnet and Lovelock theories; IOP Publishing; Journal of High Energy Physics; 2006; 5; 12-2006; 1-19 1029-8479 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1088/1126-6708/2006/05/007 |
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 |
IOP Publishing |
publisher.none.fl_str_mv |
IOP Publishing |
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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