Dynamic generation or removal of a scalar hair
Autor(a) principal: | |
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Data de Publicação: | 2023 |
Outros Autores: | , , , |
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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Repositório Institucional da UNESP |
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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 |
|
_version_ |
1808128342101065728 |