Dynamic generation or removal of a scalar hair

Detalhes bibliográficos
Autor(a) principal: Liu, Yunqi
Data de Publicação: 2023
Outros Autores: Zhang, Cheng-Yong, Qian, Wei-Liang [UNESP], Lin, Kai, Wang, Bin
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1007/JHEP01(2023)074
http://hdl.handle.net/11449/246676
Resumo: We study dynamic processes through which the scalar hair of black holes is generated or detached in a theory with a scalar field non-minimally coupled to Gauss-Bonnet and Ricci scalar invariants. We concentrate on the nonlinear temporal evolution of a far-from-equilibrium gravitational system. In our simulations, we choose the initial spacetime to be either a bald Schwarzschild or a scalarized spherically symmetric black hole. Succeeding continuous accretion of the scalar field onto the original black hole, the final fate of the system displays intriguing features, which depend on the initial configurations, strengths of the perturbation, and specific metric parameters. In addition to the scalarization process through which the bald black hole addresses scalar hair, we observe the dynamical descalarization, which removes scalar hair from an original hairy hole after continuous scalar field accretion. We examine the temporal evolution of the scalar field, the metrics, and the Misner-Sharp mass of the spacetime and exhibit rich phase structures through nonlinear dynamical processes.
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spelling Dynamic generation or removal of a scalar hairBlack HolesSpacetime SingularitiesWe study dynamic processes through which the scalar hair of black holes is generated or detached in a theory with a scalar field non-minimally coupled to Gauss-Bonnet and Ricci scalar invariants. We concentrate on the nonlinear temporal evolution of a far-from-equilibrium gravitational system. In our simulations, we choose the initial spacetime to be either a bald Schwarzschild or a scalarized spherically symmetric black hole. Succeeding continuous accretion of the scalar field onto the original black hole, the final fate of the system displays intriguing features, which depend on the initial configurations, strengths of the perturbation, and specific metric parameters. In addition to the scalarization process through which the bald black hole addresses scalar hair, we observe the dynamical descalarization, which removes scalar hair from an original hairy hole after continuous scalar field accretion. We examine the temporal evolution of the scalar field, the metrics, and the Misner-Sharp mass of the spacetime and exhibit rich phase structures through nonlinear dynamical processes.Center for Gravitation and Cosmology College of Physical Science and Technology Yangzhou UniversitySchool of Aeronautics and Astronautics Shanghai Jiao Tong UniversityDepartment of Physics and Siyuan Laboratory Jinan UniversityEscola de Engenharia de Lorena Universidade de São Paulo, SPFaculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista, SPHubei Subsurface Multi-scale Imaging Key Laboratory Institute of Geophysics and Geomatics China University of Geosciences, HubeiShanghai Frontier Science Center for Gravitational Wave Detection Shanghai Jiao Tong UniversityFaculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista, SPYangzhou UniversityShanghai Jiao Tong UniversityJinan UniversityUniversidade de São Paulo (USP)Universidade Estadual Paulista (UNESP)China University of GeosciencesLiu, YunqiZhang, Cheng-YongQian, Wei-Liang [UNESP]Lin, KaiWang, Bin2023-07-29T12:47:27Z2023-07-29T12:47:27Z2023-01-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1007/JHEP01(2023)074Journal of High Energy Physics, v. 2023, n. 1, 2023.1029-8479http://hdl.handle.net/11449/24667610.1007/JHEP01(2023)0742-s2.0-85146527687Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengJournal of High Energy Physicsinfo:eu-repo/semantics/openAccess2023-07-29T12:47:27Zoai:repositorio.unesp.br:11449/246676Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T14:17:43.441209Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Dynamic generation or removal of a scalar hair
title Dynamic generation or removal of a scalar hair
spellingShingle Dynamic generation or removal of a scalar hair
Liu, Yunqi
Black Holes
Spacetime Singularities
title_short Dynamic generation or removal of a scalar hair
title_full Dynamic generation or removal of a scalar hair
title_fullStr Dynamic generation or removal of a scalar hair
title_full_unstemmed Dynamic generation or removal of a scalar hair
title_sort Dynamic generation or removal of a scalar hair
author Liu, Yunqi
author_facet Liu, Yunqi
Zhang, Cheng-Yong
Qian, Wei-Liang [UNESP]
Lin, Kai
Wang, Bin
author_role author
author2 Zhang, Cheng-Yong
Qian, Wei-Liang [UNESP]
Lin, Kai
Wang, Bin
author2_role author
author
author
author
dc.contributor.none.fl_str_mv Yangzhou University
Shanghai Jiao Tong University
Jinan University
Universidade de São Paulo (USP)
Universidade Estadual Paulista (UNESP)
China University of Geosciences
dc.contributor.author.fl_str_mv Liu, Yunqi
Zhang, Cheng-Yong
Qian, Wei-Liang [UNESP]
Lin, Kai
Wang, Bin
dc.subject.por.fl_str_mv Black Holes
Spacetime Singularities
topic Black Holes
Spacetime Singularities
description We study dynamic processes through which the scalar hair of black holes is generated or detached in a theory with a scalar field non-minimally coupled to Gauss-Bonnet and Ricci scalar invariants. We concentrate on the nonlinear temporal evolution of a far-from-equilibrium gravitational system. In our simulations, we choose the initial spacetime to be either a bald Schwarzschild or a scalarized spherically symmetric black hole. Succeeding continuous accretion of the scalar field onto the original black hole, the final fate of the system displays intriguing features, which depend on the initial configurations, strengths of the perturbation, and specific metric parameters. In addition to the scalarization process through which the bald black hole addresses scalar hair, we observe the dynamical descalarization, which removes scalar hair from an original hairy hole after continuous scalar field accretion. We examine the temporal evolution of the scalar field, the metrics, and the Misner-Sharp mass of the spacetime and exhibit rich phase structures through nonlinear dynamical processes.
publishDate 2023
dc.date.none.fl_str_mv 2023-07-29T12:47:27Z
2023-07-29T12:47:27Z
2023-01-01
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://dx.doi.org/10.1007/JHEP01(2023)074
Journal of High Energy Physics, v. 2023, n. 1, 2023.
1029-8479
http://hdl.handle.net/11449/246676
10.1007/JHEP01(2023)074
2-s2.0-85146527687
url http://dx.doi.org/10.1007/JHEP01(2023)074
http://hdl.handle.net/11449/246676
identifier_str_mv Journal of High Energy Physics, v. 2023, n. 1, 2023.
1029-8479
10.1007/JHEP01(2023)074
2-s2.0-85146527687
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Journal of High Energy Physics
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
repository.mail.fl_str_mv
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