Evanescent gravitons in Warped Anti-de Sitter space

Autores
Giribet, Gaston Enrique; Yerko Vásquez
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Paste one version of a text here.Besides black holes, the phase space of three-dimensional massive gravity about Warped-Anti de Sitter (WAdS) space contains solutions that decay exponentially in time. They describe evanescent graviton configurations that, while governed by a wave equation with non-vanishing effective mass, do not carry net gravitational energy. Explicit examples of such solutions have been found in the case of Topologically Massive Gravity; here, we generalize them to a much more general ghost-free massive deformation, with the difference being that the decay rate gets corrected due to the presence of higher-order terms.
Fil: Giribet, Gaston Enrique. Universidad Libre de Bruselas; Bélgica. 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. Pontificia Universidad Católica de Valparaíso; Chile
Fil: Yerko Vásquez. Universidad de La Serena; Chile
Materia
Ads/Cft
Black Holes
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:11336/46652
Acceder
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spelling Evanescent gravitons in Warped Anti-de Sitter spaceGiribet, Gaston EnriqueYerko VásquezAds/CftBlack Holeshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Paste one version of a text here.Besides black holes, the phase space of three-dimensional massive gravity about Warped-Anti de Sitter (WAdS) space contains solutions that decay exponentially in time. They describe evanescent graviton configurations that, while governed by a wave equation with non-vanishing effective mass, do not carry net gravitational energy. Explicit examples of such solutions have been found in the case of Topologically Massive Gravity; here, we generalize them to a much more general ghost-free massive deformation, with the difference being that the decay rate gets corrected due to the presence of higher-order terms.Fil: Giribet, Gaston Enrique. Universidad Libre de Bruselas; Bélgica. 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. Pontificia Universidad Católica de Valparaíso; ChileFil: Yerko Vásquez. Universidad de La Serena; ChileAmerican Physical Society2016-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/46652Giribet, Gaston Enrique; Yerko Vásquez; Evanescent gravitons in Warped Anti-de Sitter space; American Physical Society; Physical Review D; 93; 2; 1-2016; 24001-240010556-2821CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.93.024001info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.93.024001info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T15:26:03Zoai:ri.conicet.gov.ar:11336/46652instacron: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:34982025-10-15 15:26:04.036CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Evanescent gravitons in Warped Anti-de Sitter space
title Evanescent gravitons in Warped Anti-de Sitter space
spellingShingle Evanescent gravitons in Warped Anti-de Sitter space
Giribet, Gaston Enrique
Ads/Cft
Black Holes
title_short Evanescent gravitons in Warped Anti-de Sitter space
title_full Evanescent gravitons in Warped Anti-de Sitter space
title_fullStr Evanescent gravitons in Warped Anti-de Sitter space
title_full_unstemmed Evanescent gravitons in Warped Anti-de Sitter space
title_sort Evanescent gravitons in Warped Anti-de Sitter space
dc.creator.none.fl_str_mv Giribet, Gaston Enrique
Yerko Vásquez
author Giribet, Gaston Enrique
author_facet Giribet, Gaston Enrique
Yerko Vásquez
author_role author
author2 Yerko Vásquez
author2_role author
dc.subject.none.fl_str_mv Ads/Cft
Black Holes
topic Ads/Cft
Black Holes
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Paste one version of a text here.Besides black holes, the phase space of three-dimensional massive gravity about Warped-Anti de Sitter (WAdS) space contains solutions that decay exponentially in time. They describe evanescent graviton configurations that, while governed by a wave equation with non-vanishing effective mass, do not carry net gravitational energy. Explicit examples of such solutions have been found in the case of Topologically Massive Gravity; here, we generalize them to a much more general ghost-free massive deformation, with the difference being that the decay rate gets corrected due to the presence of higher-order terms.
Fil: Giribet, Gaston Enrique. Universidad Libre de Bruselas; Bélgica. 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. Pontificia Universidad Católica de Valparaíso; Chile
Fil: Yerko Vásquez. Universidad de La Serena; Chile
description Paste one version of a text here.Besides black holes, the phase space of three-dimensional massive gravity about Warped-Anti de Sitter (WAdS) space contains solutions that decay exponentially in time. They describe evanescent graviton configurations that, while governed by a wave equation with non-vanishing effective mass, do not carry net gravitational energy. Explicit examples of such solutions have been found in the case of Topologically Massive Gravity; here, we generalize them to a much more general ghost-free massive deformation, with the difference being that the decay rate gets corrected due to the presence of higher-order terms.
publishDate 2016
dc.date.none.fl_str_mv 2016-01
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/11336/46652
Giribet, Gaston Enrique; Yerko Vásquez; Evanescent gravitons in Warped Anti-de Sitter space; American Physical Society; Physical Review D; 93; 2; 1-2016; 24001-24001
0556-2821
CONICET Digital
CONICET
url http://hdl.handle.net/11336/46652
identifier_str_mv Giribet, Gaston Enrique; Yerko Vásquez; Evanescent gravitons in Warped Anti-de Sitter space; American Physical Society; Physical Review D; 93; 2; 1-2016; 24001-24001
0556-2821
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.93.024001
info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.93.024001
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
_version_ 1846083404310773760
score 13.22299

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