More on vacua of exotic massive 3D gravity

Autores
Giribet, Gaston Enrique; Oliva, Julio
Año de publicación
2019
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
In a recent paper [M. Chernicoff et al., J. High Energy Phys. 08 (2018) 087JHEPFG1029-847910.1007/JHEP08(2018)087], we explored the space of solutions of the exotic massive 3D gravity theory proposed in [M. Özkan et al., J. High Energy Phys. 08 (2018) 035JHEPFG1029-847910.1007/JHEP08(2018)035]. We showed that the theory admits a rich space of vacua, including asymptotically anti de-Sitter (AdS) geometries obeying different types of boundary conditions. The examples include black holes dressed with low decaying gravitons. Based on what happens in other theories of massive gravity, we conjectured that such geometries appear on a curve of the parameter space (chiral curve) where the exotic massive gravity on AdS with sufficiently strong boundary conditions results dual to a 2D chiral conformal field theory. Here, we show that this expectation is consistent with the conserved charges and thermodynamical properties of the black holes of the theory, which have recently been computed [Mann et al.,Energy of asymptotically AdS black holes in exotic massive gravity and its log-extension, arXiv:1812.09525.]. When the boundary conditions are relaxed relative to the standard Brown-Henneaux boundary conditions, the theory exhibits solutions consistent with the definition of the so-called log-gravity. The asymptotic behavior of these solutions presents a logarithmic term in the Fefferman-Graham expansion that, nonetheless, is compatible with the AdS asymptotic symmetries. This long range interaction is due to a mode of the massive gravity that becomes massless precisely on the chiral curve. We construct exact solutions exhibiting this behavior, which admit to be interpreted as fully backreacting gravitational waves propagating on an extremal black hole, and carrying nonvanishing gravitational energy. We also discuss other vacua of the theory, such as warped-AdS3 black holes, gravitational waves on such backgrounds, AdS2×S1 spaces, and black holes in dS3 space.
Fil: Giribet, Gaston Enrique. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. 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
Materia
Black holes
3D gravity
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/147855

id CONICETDig_a89cbfd2fbe3ef3242f5cfb2e3df5e0a
oai_identifier_str oai:ri.conicet.gov.ar:11336/147855
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling More on vacua of exotic massive 3D gravityGiribet, Gaston EnriqueOliva, JulioBlack holes3D gravityhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1In a recent paper [M. Chernicoff et al., J. High Energy Phys. 08 (2018) 087JHEPFG1029-847910.1007/JHEP08(2018)087], we explored the space of solutions of the exotic massive 3D gravity theory proposed in [M. Özkan et al., J. High Energy Phys. 08 (2018) 035JHEPFG1029-847910.1007/JHEP08(2018)035]. We showed that the theory admits a rich space of vacua, including asymptotically anti de-Sitter (AdS) geometries obeying different types of boundary conditions. The examples include black holes dressed with low decaying gravitons. Based on what happens in other theories of massive gravity, we conjectured that such geometries appear on a curve of the parameter space (chiral curve) where the exotic massive gravity on AdS with sufficiently strong boundary conditions results dual to a 2D chiral conformal field theory. Here, we show that this expectation is consistent with the conserved charges and thermodynamical properties of the black holes of the theory, which have recently been computed [Mann et al.,Energy of asymptotically AdS black holes in exotic massive gravity and its log-extension, arXiv:1812.09525.]. When the boundary conditions are relaxed relative to the standard Brown-Henneaux boundary conditions, the theory exhibits solutions consistent with the definition of the so-called log-gravity. The asymptotic behavior of these solutions presents a logarithmic term in the Fefferman-Graham expansion that, nonetheless, is compatible with the AdS asymptotic symmetries. This long range interaction is due to a mode of the massive gravity that becomes massless precisely on the chiral curve. We construct exact solutions exhibiting this behavior, which admit to be interpreted as fully backreacting gravitational waves propagating on an extremal black hole, and carrying nonvanishing gravitational energy. We also discuss other vacua of the theory, such as warped-AdS3 black holes, gravitational waves on such backgrounds, AdS2×S1 spaces, and black holes in dS3 space.Fil: Giribet, Gaston Enrique. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. 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; ChileAmerican Physical Society2019-03-18info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/147855Giribet, Gaston Enrique; Oliva, Julio; More on vacua of exotic massive 3D gravity; American Physical Society; Physical Review D; 99; 6; 18-3-2019; 1-92470-00102470-0029CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.99.064021info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.99.064021info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1901.08457info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:55:24Zoai:ri.conicet.gov.ar:11336/147855instacron: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 09:55:25.136CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv More on vacua of exotic massive 3D gravity
title More on vacua of exotic massive 3D gravity
spellingShingle More on vacua of exotic massive 3D gravity
Giribet, Gaston Enrique
Black holes
3D gravity
title_short More on vacua of exotic massive 3D gravity
title_full More on vacua of exotic massive 3D gravity
title_fullStr More on vacua of exotic massive 3D gravity
title_full_unstemmed More on vacua of exotic massive 3D gravity
title_sort More on vacua of exotic massive 3D gravity
dc.creator.none.fl_str_mv Giribet, Gaston Enrique
Oliva, Julio
author Giribet, Gaston Enrique
author_facet Giribet, Gaston Enrique
Oliva, Julio
author_role author
author2 Oliva, Julio
author2_role author
dc.subject.none.fl_str_mv Black holes
3D gravity
topic Black holes
3D gravity
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv In a recent paper [M. Chernicoff et al., J. High Energy Phys. 08 (2018) 087JHEPFG1029-847910.1007/JHEP08(2018)087], we explored the space of solutions of the exotic massive 3D gravity theory proposed in [M. Özkan et al., J. High Energy Phys. 08 (2018) 035JHEPFG1029-847910.1007/JHEP08(2018)035]. We showed that the theory admits a rich space of vacua, including asymptotically anti de-Sitter (AdS) geometries obeying different types of boundary conditions. The examples include black holes dressed with low decaying gravitons. Based on what happens in other theories of massive gravity, we conjectured that such geometries appear on a curve of the parameter space (chiral curve) where the exotic massive gravity on AdS with sufficiently strong boundary conditions results dual to a 2D chiral conformal field theory. Here, we show that this expectation is consistent with the conserved charges and thermodynamical properties of the black holes of the theory, which have recently been computed [Mann et al.,Energy of asymptotically AdS black holes in exotic massive gravity and its log-extension, arXiv:1812.09525.]. When the boundary conditions are relaxed relative to the standard Brown-Henneaux boundary conditions, the theory exhibits solutions consistent with the definition of the so-called log-gravity. The asymptotic behavior of these solutions presents a logarithmic term in the Fefferman-Graham expansion that, nonetheless, is compatible with the AdS asymptotic symmetries. This long range interaction is due to a mode of the massive gravity that becomes massless precisely on the chiral curve. We construct exact solutions exhibiting this behavior, which admit to be interpreted as fully backreacting gravitational waves propagating on an extremal black hole, and carrying nonvanishing gravitational energy. We also discuss other vacua of the theory, such as warped-AdS3 black holes, gravitational waves on such backgrounds, AdS2×S1 spaces, and black holes in dS3 space.
Fil: Giribet, Gaston Enrique. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; Argentina. 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
description In a recent paper [M. Chernicoff et al., J. High Energy Phys. 08 (2018) 087JHEPFG1029-847910.1007/JHEP08(2018)087], we explored the space of solutions of the exotic massive 3D gravity theory proposed in [M. Özkan et al., J. High Energy Phys. 08 (2018) 035JHEPFG1029-847910.1007/JHEP08(2018)035]. We showed that the theory admits a rich space of vacua, including asymptotically anti de-Sitter (AdS) geometries obeying different types of boundary conditions. The examples include black holes dressed with low decaying gravitons. Based on what happens in other theories of massive gravity, we conjectured that such geometries appear on a curve of the parameter space (chiral curve) where the exotic massive gravity on AdS with sufficiently strong boundary conditions results dual to a 2D chiral conformal field theory. Here, we show that this expectation is consistent with the conserved charges and thermodynamical properties of the black holes of the theory, which have recently been computed [Mann et al.,Energy of asymptotically AdS black holes in exotic massive gravity and its log-extension, arXiv:1812.09525.]. When the boundary conditions are relaxed relative to the standard Brown-Henneaux boundary conditions, the theory exhibits solutions consistent with the definition of the so-called log-gravity. The asymptotic behavior of these solutions presents a logarithmic term in the Fefferman-Graham expansion that, nonetheless, is compatible with the AdS asymptotic symmetries. This long range interaction is due to a mode of the massive gravity that becomes massless precisely on the chiral curve. We construct exact solutions exhibiting this behavior, which admit to be interpreted as fully backreacting gravitational waves propagating on an extremal black hole, and carrying nonvanishing gravitational energy. We also discuss other vacua of the theory, such as warped-AdS3 black holes, gravitational waves on such backgrounds, AdS2×S1 spaces, and black holes in dS3 space.
publishDate 2019
dc.date.none.fl_str_mv 2019-03-18
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/11336/147855
Giribet, Gaston Enrique; Oliva, Julio; More on vacua of exotic massive 3D gravity; American Physical Society; Physical Review D; 99; 6; 18-3-2019; 1-9
2470-0010
2470-0029
CONICET Digital
CONICET
url http://hdl.handle.net/11336/147855
identifier_str_mv Giribet, Gaston Enrique; Oliva, Julio; More on vacua of exotic massive 3D gravity; American Physical Society; Physical Review D; 99; 6; 18-3-2019; 1-9
2470-0010
2470-0029
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1103/PhysRevD.99.064021
info:eu-repo/semantics/altIdentifier/url/https://journals.aps.org/prd/abstract/10.1103/PhysRevD.99.064021
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1901.08457
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/2.5/ar/
dc.format.none.fl_str_mv application/pdf
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_ 1844613670509740032
score 13.070432