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
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/74232

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spelling 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)
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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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