Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity

Autores
Argüelles, Carlos Raúl; Grandi, Nicolás Esteban; Park, Mu In
Año de publicación
2015
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
Hořava gravity has been proposed as a renormalizable, higher-derivative gravity without ghost problems, by considering different scaling dimensions for space and time. In the non-relativistic higher-derivative generalization of Einstein gravity, the meaning and physical properties of black hole and membrane space-times are quite different from the conventional ones. Here, we study the singularity and horizon structures of such geometries in IR-modified Hořava gravity, where the so-called “detailed balance” condition is softly broken in IR. We classify all the viable static solutions without naked singularities and study its close connection to non-singular cosmology solutions. We find that, in addition to the usual point-like singularity at r = 0, there exists a “surface-like” curvature singularity at finite r = rS whichisthecuttingedgeofthereal-valuedspace-time. Thedegreeofdivergenceof such singularities is milder than those of general relativity, and the Hawking temperature of the horizons diverges when they coincide with the singularities. As a byproduct we find that, in addition to the usual “asymptotic limit”, a consistent flow of coupling constants, that we called “GR flow limit”, is needed in order to recover general relativity in the IR.
Fil: Argüelles, Carlos Raúl. Università degli studi di Roma "La Sapienza"; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Grandi, Nicolás Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Park, Mu In. Sogang University; Corea del Sur
Materia
BLACK HOLES
MODELS OF QUANTUM GRAVITY
SPACETIME SINGULARITIES
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:11336/181459
Acceder
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network_name_str CONICET Digital (CONICET)
spelling Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava GravityArgüelles, Carlos RaúlGrandi, Nicolás EstebanPark, Mu InBLACK HOLESMODELS OF QUANTUM GRAVITYSPACETIME SINGULARITIEShttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Hořava gravity has been proposed as a renormalizable, higher-derivative gravity without ghost problems, by considering different scaling dimensions for space and time. In the non-relativistic higher-derivative generalization of Einstein gravity, the meaning and physical properties of black hole and membrane space-times are quite different from the conventional ones. Here, we study the singularity and horizon structures of such geometries in IR-modified Hořava gravity, where the so-called “detailed balance” condition is softly broken in IR. We classify all the viable static solutions without naked singularities and study its close connection to non-singular cosmology solutions. We find that, in addition to the usual point-like singularity at r = 0, there exists a “surface-like” curvature singularity at finite r = rS whichisthecuttingedgeofthereal-valuedspace-time. Thedegreeofdivergenceof such singularities is milder than those of general relativity, and the Hawking temperature of the horizons diverges when they coincide with the singularities. As a byproduct we find that, in addition to the usual “asymptotic limit”, a consistent flow of coupling constants, that we called “GR flow limit”, is needed in order to recover general relativity in the IR.Fil: Argüelles, Carlos Raúl. Università degli studi di Roma "La Sapienza"; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas; ArgentinaFil: Grandi, Nicolás Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Park, Mu In. Sogang University; Corea del SurSpringer2015-09info: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/11336/181459Argüelles, Carlos Raúl; Grandi, Nicolás Esteban; Park, Mu In; Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity; Springer; Journal of High Energy Physics; 5; 100; 9-2015; 1-221029-8479CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://arxiv.org/pdf/1508.04380v2info:eu-repo/semantics/altIdentifier/doi/10.1007/JHEP10(2015)100info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-10-15T15:34:41Zoai:ri.conicet.gov.ar:11336/181459instacron: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 15:34:42.126CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity
title Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity
spellingShingle Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity
Argüelles, Carlos Raúl
BLACK HOLES
MODELS OF QUANTUM GRAVITY
SPACETIME SINGULARITIES
title_short Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity
title_full Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity
title_fullStr Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity
title_full_unstemmed Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity
title_sort Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity
dc.creator.none.fl_str_mv Argüelles, Carlos Raúl
Grandi, Nicolás Esteban
Park, Mu In
author Argüelles, Carlos Raúl
author_facet Argüelles, Carlos Raúl
Grandi, Nicolás Esteban
Park, Mu In
author_role author
author2 Grandi, Nicolás Esteban
Park, Mu In
author2_role author
author
dc.subject.none.fl_str_mv BLACK HOLES
MODELS OF QUANTUM GRAVITY
SPACETIME SINGULARITIES
topic BLACK HOLES
MODELS OF QUANTUM GRAVITY
SPACETIME SINGULARITIES
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv Hořava gravity has been proposed as a renormalizable, higher-derivative gravity without ghost problems, by considering different scaling dimensions for space and time. In the non-relativistic higher-derivative generalization of Einstein gravity, the meaning and physical properties of black hole and membrane space-times are quite different from the conventional ones. Here, we study the singularity and horizon structures of such geometries in IR-modified Hořava gravity, where the so-called “detailed balance” condition is softly broken in IR. We classify all the viable static solutions without naked singularities and study its close connection to non-singular cosmology solutions. We find that, in addition to the usual point-like singularity at r = 0, there exists a “surface-like” curvature singularity at finite r = rS whichisthecuttingedgeofthereal-valuedspace-time. Thedegreeofdivergenceof such singularities is milder than those of general relativity, and the Hawking temperature of the horizons diverges when they coincide with the singularities. As a byproduct we find that, in addition to the usual “asymptotic limit”, a consistent flow of coupling constants, that we called “GR flow limit”, is needed in order to recover general relativity in the IR.
Fil: Argüelles, Carlos Raúl. Università degli studi di Roma "La Sapienza"; Italia. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina
Fil: Grandi, Nicolás Esteban. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Park, Mu In. Sogang University; Corea del Sur
description Hořava gravity has been proposed as a renormalizable, higher-derivative gravity without ghost problems, by considering different scaling dimensions for space and time. In the non-relativistic higher-derivative generalization of Einstein gravity, the meaning and physical properties of black hole and membrane space-times are quite different from the conventional ones. Here, we study the singularity and horizon structures of such geometries in IR-modified Hořava gravity, where the so-called “detailed balance” condition is softly broken in IR. We classify all the viable static solutions without naked singularities and study its close connection to non-singular cosmology solutions. We find that, in addition to the usual point-like singularity at r = 0, there exists a “surface-like” curvature singularity at finite r = rS whichisthecuttingedgeofthereal-valuedspace-time. Thedegreeofdivergenceof such singularities is milder than those of general relativity, and the Hawking temperature of the horizons diverges when they coincide with the singularities. As a byproduct we find that, in addition to the usual “asymptotic limit”, a consistent flow of coupling constants, that we called “GR flow limit”, is needed in order to recover general relativity in the IR.
publishDate 2015
dc.date.none.fl_str_mv 2015-09
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/11336/181459
Argüelles, Carlos Raúl; Grandi, Nicolás Esteban; Park, Mu In; Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity; Springer; Journal of High Energy Physics; 5; 100; 9-2015; 1-22
1029-8479
CONICET Digital
CONICET
url http://hdl.handle.net/11336/181459
identifier_str_mv Argüelles, Carlos Raúl; Grandi, Nicolás Esteban; Park, Mu In; Complete Classification of Four-Dimensional Black Hole and Membrane Solutions in IR-modified Hořava Gravity; Springer; Journal of High Energy Physics; 5; 100; 9-2015; 1-22
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/url/http://arxiv.org/pdf/1508.04380v2
info:eu-repo/semantics/altIdentifier/doi/10.1007/JHEP10(2015)100
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
application/pdf
dc.publisher.none.fl_str_mv Springer
publisher.none.fl_str_mv Springer
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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score 13.22299

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