Matrix method for perturbed black hole metric with discontinuity

Detalhes bibliográficos
Autor(a) principal: Shen, Shui-Fa
Data de Publicação: 2022
Outros Autores: Qian, Wei-Liang [UNESP], Lin, Kai, Shao, Cheng-Gang, Pan, Yu
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1088/1361-6382/ac95f1
http://hdl.handle.net/11449/246308
Resumo: Recent studies based on the notion of black hole pseudospectrum indicated substantial instability of the fundamental and high-overtone quasinormal modes (QNMs). Besides its theoretical novelty, the details about the migration of the QNM spectrum due to specific perturbations may furnish valuable information on the properties of associated gravitational waves in a more realistic context. This work generalizes the matrix method for black hole QNMs to cope with a specific class of perturbations to the metric featured by discontinuity, which is known to be intimately connected with the QNM structural instability. In practice, the presence of discontinuity poses a difficulty so that many well-known approaches for QNMs cannot be straightforwardly applied. By comparing with other methods, we show that the modified matrix method is efficient, which can be used to solve for the low-lying modes with reasonable precision. Therefore, it might serve as an alternative gadget for relevant studies.
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spelling Matrix method for perturbed black hole metric with discontinuityblack holediscontinuitymatrix methodperturbationpseudospectrumquasinormal modesRecent studies based on the notion of black hole pseudospectrum indicated substantial instability of the fundamental and high-overtone quasinormal modes (QNMs). Besides its theoretical novelty, the details about the migration of the QNM spectrum due to specific perturbations may furnish valuable information on the properties of associated gravitational waves in a more realistic context. This work generalizes the matrix method for black hole QNMs to cope with a specific class of perturbations to the metric featured by discontinuity, which is known to be intimately connected with the QNM structural instability. In practice, the presence of discontinuity poses a difficulty so that many well-known approaches for QNMs cannot be straightforwardly applied. By comparing with other methods, we show that the modified matrix method is efficient, which can be used to solve for the low-lying modes with reasonable precision. Therefore, it might serve as an alternative gadget for relevant studies.School of intelligent manufacturing Zhejiang Guangsha Vocational and Technical University of Construction, ZhejiangSchool of Electronic Electrical Engineering and Physics Fujian University of Technology, FujianEscola de Engenharia de Lorena Universidade de São Paulo, SPFaculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista, SPCenter for Gravitation and Cosmology School of Physical Science and Technology Yangzhou University, JiangsuHubei Subsurface Multi-scale Imaging Key Laboratory Institute of Geophysics and Geomatics China University of Geosciences, HubeiMOE Key Laboratory of Fundamental Physical Quantities Measurement Hubei Key Laboratory of Gravitation and Quantum Physics PGMF School of Physics Huazhong University of Science and Technology, HubeiCollege of Science Chongqing University of Posts and TelecommunicationsFaculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista, SPZhejiang Guangsha Vocational and Technical University of ConstructionFujian University of TechnologyUniversidade de São Paulo (USP)Universidade Estadual Paulista (UNESP)Yangzhou UniversityChina University of GeosciencesHuazhong University of Science and TechnologyChongqing University of Posts and TelecommunicationsShen, Shui-FaQian, Wei-Liang [UNESP]Lin, KaiShao, Cheng-GangPan, Yu2023-07-29T12:37:22Z2023-07-29T12:37:22Z2022-11-17info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1088/1361-6382/ac95f1Classical and Quantum Gravity, v. 39, n. 22, 2022.1361-63820264-9381http://hdl.handle.net/11449/24630810.1088/1361-6382/ac95f12-s2.0-85141954161Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengClassical and Quantum Gravityinfo:eu-repo/semantics/openAccess2023-07-29T12:37:22Zoai:repositorio.unesp.br:11449/246308Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462023-07-29T12:37:22Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Matrix method for perturbed black hole metric with discontinuity
title Matrix method for perturbed black hole metric with discontinuity
spellingShingle Matrix method for perturbed black hole metric with discontinuity
Shen, Shui-Fa
black hole
discontinuity
matrix method
perturbation
pseudospectrum
quasinormal modes
title_short Matrix method for perturbed black hole metric with discontinuity
title_full Matrix method for perturbed black hole metric with discontinuity
title_fullStr Matrix method for perturbed black hole metric with discontinuity
title_full_unstemmed Matrix method for perturbed black hole metric with discontinuity
title_sort Matrix method for perturbed black hole metric with discontinuity
author Shen, Shui-Fa
author_facet Shen, Shui-Fa
Qian, Wei-Liang [UNESP]
Lin, Kai
Shao, Cheng-Gang
Pan, Yu
author_role author
author2 Qian, Wei-Liang [UNESP]
Lin, Kai
Shao, Cheng-Gang
Pan, Yu
author2_role author
author
author
author
dc.contributor.none.fl_str_mv Zhejiang Guangsha Vocational and Technical University of Construction
Fujian University of Technology
Universidade de São Paulo (USP)
Universidade Estadual Paulista (UNESP)
Yangzhou University
China University of Geosciences
Huazhong University of Science and Technology
Chongqing University of Posts and Telecommunications
dc.contributor.author.fl_str_mv Shen, Shui-Fa
Qian, Wei-Liang [UNESP]
Lin, Kai
Shao, Cheng-Gang
Pan, Yu
dc.subject.por.fl_str_mv black hole
discontinuity
matrix method
perturbation
pseudospectrum
quasinormal modes
topic black hole
discontinuity
matrix method
perturbation
pseudospectrum
quasinormal modes
description Recent studies based on the notion of black hole pseudospectrum indicated substantial instability of the fundamental and high-overtone quasinormal modes (QNMs). Besides its theoretical novelty, the details about the migration of the QNM spectrum due to specific perturbations may furnish valuable information on the properties of associated gravitational waves in a more realistic context. This work generalizes the matrix method for black hole QNMs to cope with a specific class of perturbations to the metric featured by discontinuity, which is known to be intimately connected with the QNM structural instability. In practice, the presence of discontinuity poses a difficulty so that many well-known approaches for QNMs cannot be straightforwardly applied. By comparing with other methods, we show that the modified matrix method is efficient, which can be used to solve for the low-lying modes with reasonable precision. Therefore, it might serve as an alternative gadget for relevant studies.
publishDate 2022
dc.date.none.fl_str_mv 2022-11-17
2023-07-29T12:37:22Z
2023-07-29T12:37:22Z
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/10.1088/1361-6382/ac95f1
Classical and Quantum Gravity, v. 39, n. 22, 2022.
1361-6382
0264-9381
http://hdl.handle.net/11449/246308
10.1088/1361-6382/ac95f1
2-s2.0-85141954161
url http://dx.doi.org/10.1088/1361-6382/ac95f1
http://hdl.handle.net/11449/246308
identifier_str_mv Classical and Quantum Gravity, v. 39, n. 22, 2022.
1361-6382
0264-9381
10.1088/1361-6382/ac95f1
2-s2.0-85141954161
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Classical and Quantum Gravity
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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