Black Holes in Magnetic Monopoles with a Dark Halo

Autores
Lugo, Adrián René; Pérez Ipiña, J. M.; Schaposnik, Fidel Arturo
Año de publicación
2019
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We study a spontaneously broken Einstein–Yang–Mills–Higgs model coupled via a Higgs portal to an uncharged scalar χ. We present a phase diagram of self-gravitating solutions showing that depending on the choice of parameters of the χ scalar potential and the Higgs portal coupling constant γ, one can identify different regions: If γ is sufficiently small, a χ halo is created around the monopole core which in turn surrounds a black hole. For larger values of γ, no halo exists and the solution is just a black hole monopole one. When the horizon radius grows and becomes larger than the monopole radius, solely a black hole solution exists. Because of the presence of the χ scalar, a bound for the Higgs potential coupling constant exists and when it is not satisfied, the vacuum is unstable and no nontrivial solution exists. We briefly comment on possible connections of our results with those found in recent dark matter axion models.
Instituto de Física La Plata
Materia
Ciencias Exactas
Física
Magnetic monopole
Higgs portal
Black hole
Nivel de accesibilidad
acceso abierto
Condiciones de uso
http://creativecommons.org/licenses/by/4.0/
Repositorio
SEDICI (UNLP)
Institución
Universidad Nacional de La Plata
OAI Identificador
oai:sedici.unlp.edu.ar:10915/124192

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network_name_str SEDICI (UNLP)
spelling Black Holes in Magnetic Monopoles with a Dark HaloLugo, Adrián RenéPérez Ipiña, J. M.Schaposnik, Fidel ArturoCiencias ExactasFísicaMagnetic monopoleHiggs portalBlack holeWe study a spontaneously broken Einstein–Yang–Mills–Higgs model coupled via a Higgs portal to an uncharged scalar χ. We present a phase diagram of self-gravitating solutions showing that depending on the choice of parameters of the χ scalar potential and the Higgs portal coupling constant γ, one can identify different regions: If γ is sufficiently small, a χ halo is created around the monopole core which in turn surrounds a black hole. For larger values of γ, no halo exists and the solution is just a black hole monopole one. When the horizon radius grows and becomes larger than the monopole radius, solely a black hole solution exists. Because of the presence of the χ scalar, a bound for the Higgs potential coupling constant exists and when it is not satisfied, the vacuum is unstable and no nontrivial solution exists. We briefly comment on possible connections of our results with those found in recent dark matter axion models.Instituto de Física La Plata2019-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionArticulohttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfhttp://sedici.unlp.edu.ar/handle/10915/124192enginfo:eu-repo/semantics/altIdentifier/issn/0217-751xinfo:eu-repo/semantics/altIdentifier/issn/1793-656xinfo:eu-repo/semantics/altIdentifier/arxiv/1808.07513info:eu-repo/semantics/altIdentifier/doi/10.1142/s0217751x19500027info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by/4.0/Creative Commons Attribution 4.0 International (CC BY 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2025-10-22T17:10:49Zoai:sedici.unlp.edu.ar:10915/124192Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292025-10-22 17:10:49.261SEDICI (UNLP) - Universidad Nacional de La Platafalse
dc.title.none.fl_str_mv Black Holes in Magnetic Monopoles with a Dark Halo
title Black Holes in Magnetic Monopoles with a Dark Halo
spellingShingle Black Holes in Magnetic Monopoles with a Dark Halo
Lugo, Adrián René
Ciencias Exactas
Física
Magnetic monopole
Higgs portal
Black hole
title_short Black Holes in Magnetic Monopoles with a Dark Halo
title_full Black Holes in Magnetic Monopoles with a Dark Halo
title_fullStr Black Holes in Magnetic Monopoles with a Dark Halo
title_full_unstemmed Black Holes in Magnetic Monopoles with a Dark Halo
title_sort Black Holes in Magnetic Monopoles with a Dark Halo
dc.creator.none.fl_str_mv Lugo, Adrián René
Pérez Ipiña, J. M.
Schaposnik, Fidel Arturo
author Lugo, Adrián René
author_facet Lugo, Adrián René
Pérez Ipiña, J. M.
Schaposnik, Fidel Arturo
author_role author
author2 Pérez Ipiña, J. M.
Schaposnik, Fidel Arturo
author2_role author
author
dc.subject.none.fl_str_mv Ciencias Exactas
Física
Magnetic monopole
Higgs portal
Black hole
topic Ciencias Exactas
Física
Magnetic monopole
Higgs portal
Black hole
dc.description.none.fl_txt_mv We study a spontaneously broken Einstein–Yang–Mills–Higgs model coupled via a Higgs portal to an uncharged scalar χ. We present a phase diagram of self-gravitating solutions showing that depending on the choice of parameters of the χ scalar potential and the Higgs portal coupling constant γ, one can identify different regions: If γ is sufficiently small, a χ halo is created around the monopole core which in turn surrounds a black hole. For larger values of γ, no halo exists and the solution is just a black hole monopole one. When the horizon radius grows and becomes larger than the monopole radius, solely a black hole solution exists. Because of the presence of the χ scalar, a bound for the Higgs potential coupling constant exists and when it is not satisfied, the vacuum is unstable and no nontrivial solution exists. We briefly comment on possible connections of our results with those found in recent dark matter axion models.
Instituto de Física La Plata
description We study a spontaneously broken Einstein–Yang–Mills–Higgs model coupled via a Higgs portal to an uncharged scalar χ. We present a phase diagram of self-gravitating solutions showing that depending on the choice of parameters of the χ scalar potential and the Higgs portal coupling constant γ, one can identify different regions: If γ is sufficiently small, a χ halo is created around the monopole core which in turn surrounds a black hole. For larger values of γ, no halo exists and the solution is just a black hole monopole one. When the horizon radius grows and becomes larger than the monopole radius, solely a black hole solution exists. Because of the presence of the χ scalar, a bound for the Higgs potential coupling constant exists and when it is not satisfied, the vacuum is unstable and no nontrivial solution exists. We briefly comment on possible connections of our results with those found in recent dark matter axion models.
publishDate 2019
dc.date.none.fl_str_mv 2019-01
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
Articulo
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://sedici.unlp.edu.ar/handle/10915/124192
url http://sedici.unlp.edu.ar/handle/10915/124192
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/issn/0217-751x
info:eu-repo/semantics/altIdentifier/issn/1793-656x
info:eu-repo/semantics/altIdentifier/arxiv/1808.07513
info:eu-repo/semantics/altIdentifier/doi/10.1142/s0217751x19500027
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
http://creativecommons.org/licenses/by/4.0/
Creative Commons Attribution 4.0 International (CC BY 4.0)
eu_rights_str_mv openAccess
rights_invalid_str_mv http://creativecommons.org/licenses/by/4.0/
Creative Commons Attribution 4.0 International (CC BY 4.0)
dc.format.none.fl_str_mv application/pdf
dc.source.none.fl_str_mv reponame:SEDICI (UNLP)
instname:Universidad Nacional de La Plata
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collection SEDICI (UNLP)
instname_str Universidad Nacional de La Plata
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repository.name.fl_str_mv SEDICI (UNLP) - Universidad Nacional de La Plata
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