Einstein-Maxwell-scalar black holes: classes of solutions, dyons and extremality
Autor(a) principal: | |
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Data de Publicação: | 2019 |
Outros Autores: | , , |
Tipo de documento: | Artigo |
Idioma: | eng |
Título da fonte: | Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
Texto Completo: | http://hdl.handle.net/10773/27050 |
Resumo: | Spherical black hole (BH) solutions in Einstein-Maxwell-scalar (EMS) models wherein the scalar field is non-minimally coupled to the Maxwell invariant by some coupling function are discussed. We suggest a classification for these models into two classes, based on the properties of the coupling function, which, in particular, allow, or not, the ReissnerNordstr¨om (RN) BH solution of electrovacuum to solve a given model. Then, a comparative analysis of two illustrative families of solutions, one belonging to each class is performed: dilatonic versus scalarised BHs. By including magnetic charge, that is considering dyons, we show that scalarised BHs can have a smooth extremal limit, unlike purely electric or magnetic solutions. In particular, we study this extremal limit using the entropy function formalism, which provides insight on why both charges are necessary for extremal solutions to exist. |
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Einstein-Maxwell-scalar black holes: classes of solutions, dyons and extremalityBlack holesClassical theories of gravityScalarizationDyonsSpherical black hole (BH) solutions in Einstein-Maxwell-scalar (EMS) models wherein the scalar field is non-minimally coupled to the Maxwell invariant by some coupling function are discussed. We suggest a classification for these models into two classes, based on the properties of the coupling function, which, in particular, allow, or not, the ReissnerNordstr¨om (RN) BH solution of electrovacuum to solve a given model. Then, a comparative analysis of two illustrative families of solutions, one belonging to each class is performed: dilatonic versus scalarised BHs. By including magnetic charge, that is considering dyons, we show that scalarised BHs can have a smooth extremal limit, unlike purely electric or magnetic solutions. In particular, we study this extremal limit using the entropy function formalism, which provides insight on why both charges are necessary for extremal solutions to exist.Springer Verlag2019-11-27T11:08:16Z2019-10-07T00:00:00Z2019-10-07info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10773/27050eng1126-670810.1007/JHEP10(2019)078Astefanesei, D.Herdeiro, C.Pombo, A.Radu, E.info: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:RCAAP2024-02-22T11:52:24Zoai:ria.ua.pt:10773/27050Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-20T02:59:55.164211Repositório 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 |
Einstein-Maxwell-scalar black holes: classes of solutions, dyons and extremality |
title |
Einstein-Maxwell-scalar black holes: classes of solutions, dyons and extremality |
spellingShingle |
Einstein-Maxwell-scalar black holes: classes of solutions, dyons and extremality Astefanesei, D. Black holes Classical theories of gravity Scalarization Dyons |
title_short |
Einstein-Maxwell-scalar black holes: classes of solutions, dyons and extremality |
title_full |
Einstein-Maxwell-scalar black holes: classes of solutions, dyons and extremality |
title_fullStr |
Einstein-Maxwell-scalar black holes: classes of solutions, dyons and extremality |
title_full_unstemmed |
Einstein-Maxwell-scalar black holes: classes of solutions, dyons and extremality |
title_sort |
Einstein-Maxwell-scalar black holes: classes of solutions, dyons and extremality |
author |
Astefanesei, D. |
author_facet |
Astefanesei, D. Herdeiro, C. Pombo, A. Radu, E. |
author_role |
author |
author2 |
Herdeiro, C. Pombo, A. Radu, E. |
author2_role |
author author author |
dc.contributor.author.fl_str_mv |
Astefanesei, D. Herdeiro, C. Pombo, A. Radu, E. |
dc.subject.por.fl_str_mv |
Black holes Classical theories of gravity Scalarization Dyons |
topic |
Black holes Classical theories of gravity Scalarization Dyons |
description |
Spherical black hole (BH) solutions in Einstein-Maxwell-scalar (EMS) models wherein the scalar field is non-minimally coupled to the Maxwell invariant by some coupling function are discussed. We suggest a classification for these models into two classes, based on the properties of the coupling function, which, in particular, allow, or not, the ReissnerNordstr¨om (RN) BH solution of electrovacuum to solve a given model. Then, a comparative analysis of two illustrative families of solutions, one belonging to each class is performed: dilatonic versus scalarised BHs. By including magnetic charge, that is considering dyons, we show that scalarised BHs can have a smooth extremal limit, unlike purely electric or magnetic solutions. In particular, we study this extremal limit using the entropy function formalism, which provides insight on why both charges are necessary for extremal solutions to exist. |
publishDate |
2019 |
dc.date.none.fl_str_mv |
2019-11-27T11:08:16Z 2019-10-07T00:00:00Z 2019-10-07 |
dc.type.status.fl_str_mv |
info:eu-repo/semantics/publishedVersion |
dc.type.driver.fl_str_mv |
info:eu-repo/semantics/article |
format |
article |
status_str |
publishedVersion |
dc.identifier.uri.fl_str_mv |
http://hdl.handle.net/10773/27050 |
url |
http://hdl.handle.net/10773/27050 |
dc.language.iso.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
1126-6708 10.1007/JHEP10(2019)078 |
dc.rights.driver.fl_str_mv |
info:eu-repo/semantics/openAccess |
eu_rights_str_mv |
openAccess |
dc.format.none.fl_str_mv |
application/pdf |
dc.publisher.none.fl_str_mv |
Springer Verlag |
publisher.none.fl_str_mv |
Springer Verlag |
dc.source.none.fl_str_mv |
reponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação instacron:RCAAP |
instname_str |
Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação |
instacron_str |
RCAAP |
institution |
RCAAP |
reponame_str |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
collection |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) |
repository.name.fl_str_mv |
Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos) - Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informação |
repository.mail.fl_str_mv |
|
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1799137654202171392 |