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
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/124192
Ver los metadatos del registro completo
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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 |
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2019-01 |
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eng |
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eng |
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