On the classicality of bosonic stars

Detalhes bibliográficos
Autor(a) principal: Herdeiro, Carlos A. R.
Data de Publicação: 2022
Outros Autores: 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/10773/35217
Resumo: Because the Klein–Gordon and Proca equations involve ℏ, they describe quantum fields. Their solutions, however, may be treated as classical if their typical action obeys typical≫ℏ. This is possible due to their bosonic nature, allowing states with many particles. We show, by generic arguments, that the typical action for such bosonic stars is typical/ℏ≳(max/Pl)2∼1076(max/⊙)2, where max is the maximal bosonic star mass of the particular model and Pl is the Planck mass. Thus, for models allowing max≫Pl and for solutions with mass ∼max, the classical treatment is legitimate, which includes masses in the astrophysical interesting range ≳⊙.
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spelling On the classicality of bosonic starsBoson starsGeneral relativityQuantum field theoryBecause the Klein–Gordon and Proca equations involve ℏ, they describe quantum fields. Their solutions, however, may be treated as classical if their typical action obeys typical≫ℏ. This is possible due to their bosonic nature, allowing states with many particles. We show, by generic arguments, that the typical action for such bosonic stars is typical/ℏ≳(max/Pl)2∼1076(max/⊙)2, where max is the maximal bosonic star mass of the particular model and Pl is the Planck mass. Thus, for models allowing max≫Pl and for solutions with mass ∼max, the classical treatment is legitimate, which includes masses in the astrophysical interesting range ≳⊙.World Scientific Publishing2022-11-18T15:51:03Z2022-01-01T00:00:00Z2022info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10773/35217eng0218-271810.1142/S0218271822420226Herdeiro, 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:RCAAP2024-02-22T12:07:41Zoai:ria.ua.pt:10773/35217Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-20T03:06:14.465037Repositório 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 On the classicality of bosonic stars
title On the classicality of bosonic stars
spellingShingle On the classicality of bosonic stars
Herdeiro, Carlos A. R.
Boson stars
General relativity
Quantum field theory
title_short On the classicality of bosonic stars
title_full On the classicality of bosonic stars
title_fullStr On the classicality of bosonic stars
title_full_unstemmed On the classicality of bosonic stars
title_sort On the classicality of bosonic stars
author Herdeiro, Carlos A. R.
author_facet Herdeiro, Carlos A. R.
Radu, Eugen
author_role author
author2 Radu, Eugen
author2_role author
dc.contributor.author.fl_str_mv Herdeiro, Carlos A. R.
Radu, Eugen
dc.subject.por.fl_str_mv Boson stars
General relativity
Quantum field theory
topic Boson stars
General relativity
Quantum field theory
description Because the Klein–Gordon and Proca equations involve ℏ, they describe quantum fields. Their solutions, however, may be treated as classical if their typical action obeys typical≫ℏ. This is possible due to their bosonic nature, allowing states with many particles. We show, by generic arguments, that the typical action for such bosonic stars is typical/ℏ≳(max/Pl)2∼1076(max/⊙)2, where max is the maximal bosonic star mass of the particular model and Pl is the Planck mass. Thus, for models allowing max≫Pl and for solutions with mass ∼max, the classical treatment is legitimate, which includes masses in the astrophysical interesting range ≳⊙.
publishDate 2022
dc.date.none.fl_str_mv 2022-11-18T15:51:03Z
2022-01-01T00:00:00Z
2022
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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/10773/35217
url http://hdl.handle.net/10773/35217
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 0218-2718
10.1142/S0218271822420226
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dc.publisher.none.fl_str_mv World Scientific Publishing
publisher.none.fl_str_mv World Scientific Publishing
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