Asymptotically flat, spherical, self-interacting scalar, Dirac and Proca stars

Detalhes bibliográficos
Autor(a) principal: Herdeiro, Carlos A. R.
Data de Publicação: 2020
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/10773/30089
Resumo: We present a comparative analysis of the self-gravitating solitons that arise in the Einstein–Klein–Gordon, Einstein–Dirac, and Einstein–Proca models, for the particular case of static, spherically symmetric spacetimes. Differently from the previous study by Herdeiro, Pombo and Radu in 2017, the matter fields possess suitable self-interacting terms in the Lagrangians, which allow for the existence of Q-ball-type solutions for these models in the flat spacetime limit. In spite of this important difference, our analysis shows that the high degree of universality that was observed by Herdeiro, Pombo and Radu remains, and various spin-independent common patterns are observed.
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spelling Asymptotically flat, spherical, self-interacting scalar, Dirac and Proca starsSolitonsBoson starsDirac starsWe present a comparative analysis of the self-gravitating solitons that arise in the Einstein–Klein–Gordon, Einstein–Dirac, and Einstein–Proca models, for the particular case of static, spherically symmetric spacetimes. Differently from the previous study by Herdeiro, Pombo and Radu in 2017, the matter fields possess suitable self-interacting terms in the Lagrangians, which allow for the existence of Q-ball-type solutions for these models in the flat spacetime limit. In spite of this important difference, our analysis shows that the high degree of universality that was observed by Herdeiro, Pombo and Radu remains, and various spin-independent common patterns are observed.MDPI2020-12-15T19:52:20Z2020-12-01T00:00:00Z2020-12info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/10773/30089eng2073-899410.3390/sym12122032Herdeiro, 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:RCAAP2024-02-22T11:58:02Zoai:ria.ua.pt:10773/30089Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireopendoar:71602024-03-20T03:02:13.936955Repositório 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 Asymptotically flat, spherical, self-interacting scalar, Dirac and Proca stars
title Asymptotically flat, spherical, self-interacting scalar, Dirac and Proca stars
spellingShingle Asymptotically flat, spherical, self-interacting scalar, Dirac and Proca stars
Herdeiro, Carlos A. R.
Solitons
Boson stars
Dirac stars
title_short Asymptotically flat, spherical, self-interacting scalar, Dirac and Proca stars
title_full Asymptotically flat, spherical, self-interacting scalar, Dirac and Proca stars
title_fullStr Asymptotically flat, spherical, self-interacting scalar, Dirac and Proca stars
title_full_unstemmed Asymptotically flat, spherical, self-interacting scalar, Dirac and Proca stars
title_sort Asymptotically flat, spherical, self-interacting scalar, Dirac and Proca 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 Solitons
Boson stars
Dirac stars
topic Solitons
Boson stars
Dirac stars
description We present a comparative analysis of the self-gravitating solitons that arise in the Einstein–Klein–Gordon, Einstein–Dirac, and Einstein–Proca models, for the particular case of static, spherically symmetric spacetimes. Differently from the previous study by Herdeiro, Pombo and Radu in 2017, the matter fields possess suitable self-interacting terms in the Lagrangians, which allow for the existence of Q-ball-type solutions for these models in the flat spacetime limit. In spite of this important difference, our analysis shows that the high degree of universality that was observed by Herdeiro, Pombo and Radu remains, and various spin-independent common patterns are observed.
publishDate 2020
dc.date.none.fl_str_mv 2020-12-15T19:52:20Z
2020-12-01T00:00:00Z
2020-12
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/10773/30089
url http://hdl.handle.net/10773/30089
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 2073-8994
10.3390/sym12122032
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
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