Angular momentum – area – proportionality of extremal charged black holes in odd dimensions

Extremal rotating cohomogeneity-1 black holes in Einstein-Maxwell theory feature two branches. On the branch emerging from the Myers-Perry solutions their angular momentum is proportional to their horizon area, while on the branch emerging from the Tangherlini solutions their angular momentum is pro...

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Detalles Bibliográficos
Autores: Blázquez Salcedo, José Luis, Kunz, Jutta, Navarro Lerida, Francisco
Tipo de recurso: artículo
Fecha de publicación:2013
País:España
Institución:Universidad Complutense de Madrid (UCM)
Repositorio:Docta Complutense
Idioma:inglés
OAI Identifier:oai:docta.ucm.es:20.500.14352/98615
Acceso en línea:https://hdl.handle.net/20.500.14352/98615
Access Level:acceso abierto
Palabra clave:53
Physics
Astronomy & astrophysics
Física (Física)
22 Física
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spelling Angular momentum – area – proportionality of extremal charged black holes in odd dimensionsBlázquez Salcedo, José LuisKunz, JuttaNavarro Lerida, Francisco53PhysicsAstronomy & astrophysicsFísica (Física)22 FísicaExtremal rotating cohomogeneity-1 black holes in Einstein-Maxwell theory feature two branches. On the branch emerging from the Myers-Perry solutions their angular momentum is proportional to their horizon area, while on the branch emerging from the Tangherlini solutions their angular momentum is proportional to their horizon angular momentum. The transition between these branches occurs at a critical value of the charge, which depends on the value of the angular momentum. However, when a dilaton is included, the angular momentum is always proportional to the horizon area.ElsevierUniversidad Complutense de Madrid20132013-01-0120132013-01-01journal articlehttp://purl.org/coar/resource_type/c_6501VoRhttp://purl.org/coar/version/c_970fb48d4fbd8a85info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/20.500.14352/98615reponame:Docta Complutenseinstname:Universidad Complutense de Madrid (UCM)InglésengFIS2011-28013 Not available Not available1620 Not available Not availableopen accesshttp://purl.org/coar/access_right/c_abf2Attribution 4.0 Internationalhttps://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccessoai:docta.ucm.es:20.500.14352/986152026-06-02T12:44:21Z
dc.title.none.fl_str_mv Angular momentum – area – proportionality of extremal charged black holes in odd dimensions
title Angular momentum – area – proportionality of extremal charged black holes in odd dimensions
spellingShingle Angular momentum – area – proportionality of extremal charged black holes in odd dimensions
Blázquez Salcedo, José Luis
53
Physics
Astronomy & astrophysics
Física (Física)
22 Física
title_short Angular momentum – area – proportionality of extremal charged black holes in odd dimensions
title_full Angular momentum – area – proportionality of extremal charged black holes in odd dimensions
title_fullStr Angular momentum – area – proportionality of extremal charged black holes in odd dimensions
title_full_unstemmed Angular momentum – area – proportionality of extremal charged black holes in odd dimensions
title_sort Angular momentum – area – proportionality of extremal charged black holes in odd dimensions
dc.creator.none.fl_str_mv Blázquez Salcedo, José Luis
Kunz, Jutta
Navarro Lerida, Francisco
author Blázquez Salcedo, José Luis
author_facet Blázquez Salcedo, José Luis
Kunz, Jutta
Navarro Lerida, Francisco
author_role author
author2 Kunz, Jutta
Navarro Lerida, Francisco
author2_role author
author
dc.contributor.none.fl_str_mv Universidad Complutense de Madrid
dc.subject.none.fl_str_mv 53
Physics
Astronomy & astrophysics
Física (Física)
22 Física
topic 53
Physics
Astronomy & astrophysics
Física (Física)
22 Física
description Extremal rotating cohomogeneity-1 black holes in Einstein-Maxwell theory feature two branches. On the branch emerging from the Myers-Perry solutions their angular momentum is proportional to their horizon area, while on the branch emerging from the Tangherlini solutions their angular momentum is proportional to their horizon angular momentum. The transition between these branches occurs at a critical value of the charge, which depends on the value of the angular momentum. However, when a dilaton is included, the angular momentum is always proportional to the horizon area.
publishDate 2013
dc.date.none.fl_str_mv 2013
2013-01-01
2013
2013-01-01
dc.type.none.fl_str_mv journal article
http://purl.org/coar/resource_type/c_6501
VoR
http://purl.org/coar/version/c_970fb48d4fbd8a85
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv https://hdl.handle.net/20.500.14352/98615
url https://hdl.handle.net/20.500.14352/98615
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.relation.none.fl_str_mv FIS2011-28013 Not available Not available
1620 Not available Not available
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Elsevier
publisher.none.fl_str_mv Elsevier
dc.source.none.fl_str_mv reponame:Docta Complutense
instname:Universidad Complutense de Madrid (UCM)
instname_str Universidad Complutense de Madrid (UCM)
reponame_str Docta Complutense
collection Docta Complutense
repository.name.fl_str_mv
repository.mail.fl_str_mv
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score 15.300724

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