Kerr black holes with synchronised scalar hair and higher azimuthal harmonic index

Detalhes bibliográficos
Autor(a) principal: Delgado, Jorge F. M.
Data de Publicação: 2019
Outros Autores: Herdeiro, Carlos A. R., Radu, Eugen
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/10773/25990
Resumo: Kerr black holes with synchronised scalar hair and azimuthal harmonic index m>1 are constructed and studied. The corresponding domain of existence has a broader frequency range than the fundamental m=1 family; moreover, larger ADM masses, M and angular momenta J are allowed. Amongst other salient features, non-uniqueness of solutions for fixed global quantities is observed: solutions with the same M and J co-exist, for consecutive values of m, and the ones with larger m are always entropically favoured. Our analysis demonstrates, moreover, the qualitative universality of various features observed for m=1 solutions, such as the shape of the domain of existence, the typology of ergo-regions, and the horizon geometry, which is studied through its isometric embedding in Euclidean 3-space.
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spelling Kerr black holes with synchronised scalar hair and higher azimuthal harmonic indexKerr black holes with synchronised scalar hair and azimuthal harmonic index m>1 are constructed and studied. The corresponding domain of existence has a broader frequency range than the fundamental m=1 family; moreover, larger ADM masses, M and angular momenta J are allowed. Amongst other salient features, non-uniqueness of solutions for fixed global quantities is observed: solutions with the same M and J co-exist, for consecutive values of m, and the ones with larger m are always entropically favoured. Our analysis demonstrates, moreover, the qualitative universality of various features observed for m=1 solutions, such as the shape of the domain of existence, the typology of ergo-regions, and the horizon geometry, which is studied through its isometric embedding in Euclidean 3-space.Elsevier2019-05-09T11:10:44Z2019-05-10T00:00:00Z2019-05-10info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10773/25990eng0370-269310.1016/j.physletb.2019.04.009Delgado, Jorge F. M.Herdeiro, Carlos A. R.Radu, Eugeninfo:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2024-02-22T11:50:16Zoai:ria.ua.pt:10773/25990Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-20T02:59:04.382881Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãofalse
dc.title.none.fl_str_mv Kerr black holes with synchronised scalar hair and higher azimuthal harmonic index
title Kerr black holes with synchronised scalar hair and higher azimuthal harmonic index
spellingShingle Kerr black holes with synchronised scalar hair and higher azimuthal harmonic index
Delgado, Jorge F. M.
title_short Kerr black holes with synchronised scalar hair and higher azimuthal harmonic index
title_full Kerr black holes with synchronised scalar hair and higher azimuthal harmonic index
title_fullStr Kerr black holes with synchronised scalar hair and higher azimuthal harmonic index
title_full_unstemmed Kerr black holes with synchronised scalar hair and higher azimuthal harmonic index
title_sort Kerr black holes with synchronised scalar hair and higher azimuthal harmonic index
author Delgado, Jorge F. M.
author_facet Delgado, Jorge F. M.
Herdeiro, Carlos A. R.
Radu, Eugen
author_role author
author2 Herdeiro, Carlos A. R.
Radu, Eugen
author2_role author
author
dc.contributor.author.fl_str_mv Delgado, Jorge F. M.
Herdeiro, Carlos A. R.
Radu, Eugen
description Kerr black holes with synchronised scalar hair and azimuthal harmonic index m>1 are constructed and studied. The corresponding domain of existence has a broader frequency range than the fundamental m=1 family; moreover, larger ADM masses, M and angular momenta J are allowed. Amongst other salient features, non-uniqueness of solutions for fixed global quantities is observed: solutions with the same M and J co-exist, for consecutive values of m, and the ones with larger m are always entropically favoured. Our analysis demonstrates, moreover, the qualitative universality of various features observed for m=1 solutions, such as the shape of the domain of existence, the typology of ergo-regions, and the horizon geometry, which is studied through its isometric embedding in Euclidean 3-space.
publishDate 2019
dc.date.none.fl_str_mv 2019-05-09T11:10:44Z
2019-05-10T00:00:00Z
2019-05-10
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
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status_str publishedVersion
dc.identifier.uri.fl_str_mv http://hdl.handle.net/10773/25990
url http://hdl.handle.net/10773/25990
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 0370-2693
10.1016/j.physletb.2019.04.009
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
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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:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
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