High-order matrix method with delimited expansion domain

Detalhes bibliográficos
Autor(a) principal: Lin, Kai
Data de Publicação: 2023
Outros Autores: Qian, Wei-Liang [UNESP]
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://dx.doi.org/10.1088/1361-6382/acc50f
http://hdl.handle.net/11449/247105
Resumo: Motivated by the substantial instability of the fundamental and high-overtone quasinormal modes (QNMs), recent developments regarding the notion of black hole pseudospectrum call for numerical results with unprecedented precision. This work generalizes and improves the matrix method for black hole QNMs to higher orders, specifically aiming at a class of perturbations to the metric featured by discontinuity intimately associated with the QNM structural instability. The approach is based on the mock-Chebyshev grid, which guarantees its convergence in the degree of the interpolant. In practice, solving for black hole QNMs is a formidable task. The presence of discontinuity poses a further difficulty so that many well-known approaches cannot be employed straightforwardly. Compared with other viable methods, the modified matrix method is competent in speed and accuracy. Therefore, the method serves as a helpful gadget for relevant studies.
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spelling High-order matrix method with delimited expansion domainblack holematrix methodquasinormal modeMotivated by the substantial instability of the fundamental and high-overtone quasinormal modes (QNMs), recent developments regarding the notion of black hole pseudospectrum call for numerical results with unprecedented precision. This work generalizes and improves the matrix method for black hole QNMs to higher orders, specifically aiming at a class of perturbations to the metric featured by discontinuity intimately associated with the QNM structural instability. The approach is based on the mock-Chebyshev grid, which guarantees its convergence in the degree of the interpolant. In practice, solving for black hole QNMs is a formidable task. The presence of discontinuity poses a further difficulty so that many well-known approaches cannot be employed straightforwardly. Compared with other viable methods, the modified matrix method is competent in speed and accuracy. Therefore, the method serves as a helpful gadget for relevant studies.Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Fundação de Amparo à Pesquisa do Estado de GoiásFundação de Amparo à Pesquisa do Estado do PiauíFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)National Natural Science Foundation of ChinaHubei Subsurface Multi-scale Imaging Key Laboratory Institute of Geophysics and Geomatics China University of Geosciences, HubeiEscola de Engenharia de Lorena Universidade de São PauloFaculdade de Engenharia de Guaratinguetá Universidade Estadual PaulistaCenter for Gravitation and Cosmology School of Physical Science and Technology Yangzhou University, JiangsuFaculdade de Engenharia de Guaratinguetá Universidade Estadual PaulistaChina University of GeosciencesUniversidade de São Paulo (USP)Universidade Estadual Paulista (UNESP)Yangzhou UniversityLin, KaiQian, Wei-Liang [UNESP]2023-07-29T13:06:25Z2023-07-29T13:06:25Z2023-04-20info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articlehttp://dx.doi.org/10.1088/1361-6382/acc50fClassical and Quantum Gravity, v. 40, n. 8, 2023.1361-63820264-9381http://hdl.handle.net/11449/24710510.1088/1361-6382/acc50f2-s2.0-85151503331Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengClassical and Quantum Gravityinfo:eu-repo/semantics/openAccess2023-07-29T13:06:25Zoai:repositorio.unesp.br:11449/247105Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462024-08-05T20:36:52.799834Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv High-order matrix method with delimited expansion domain
title High-order matrix method with delimited expansion domain
spellingShingle High-order matrix method with delimited expansion domain
Lin, Kai
black hole
matrix method
quasinormal mode
title_short High-order matrix method with delimited expansion domain
title_full High-order matrix method with delimited expansion domain
title_fullStr High-order matrix method with delimited expansion domain
title_full_unstemmed High-order matrix method with delimited expansion domain
title_sort High-order matrix method with delimited expansion domain
author Lin, Kai
author_facet Lin, Kai
Qian, Wei-Liang [UNESP]
author_role author
author2 Qian, Wei-Liang [UNESP]
author2_role author
dc.contributor.none.fl_str_mv China University of Geosciences
Universidade de São Paulo (USP)
Universidade Estadual Paulista (UNESP)
Yangzhou University
dc.contributor.author.fl_str_mv Lin, Kai
Qian, Wei-Liang [UNESP]
dc.subject.por.fl_str_mv black hole
matrix method
quasinormal mode
topic black hole
matrix method
quasinormal mode
description Motivated by the substantial instability of the fundamental and high-overtone quasinormal modes (QNMs), recent developments regarding the notion of black hole pseudospectrum call for numerical results with unprecedented precision. This work generalizes and improves the matrix method for black hole QNMs to higher orders, specifically aiming at a class of perturbations to the metric featured by discontinuity intimately associated with the QNM structural instability. The approach is based on the mock-Chebyshev grid, which guarantees its convergence in the degree of the interpolant. In practice, solving for black hole QNMs is a formidable task. The presence of discontinuity poses a further difficulty so that many well-known approaches cannot be employed straightforwardly. Compared with other viable methods, the modified matrix method is competent in speed and accuracy. Therefore, the method serves as a helpful gadget for relevant studies.
publishDate 2023
dc.date.none.fl_str_mv 2023-07-29T13:06:25Z
2023-07-29T13:06:25Z
2023-04-20
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/acc50f
Classical and Quantum Gravity, v. 40, n. 8, 2023.
1361-6382
0264-9381
http://hdl.handle.net/11449/247105
10.1088/1361-6382/acc50f
2-s2.0-85151503331
url http://dx.doi.org/10.1088/1361-6382/acc50f
http://hdl.handle.net/11449/247105
identifier_str_mv Classical and Quantum Gravity, v. 40, n. 8, 2023.
1361-6382
0264-9381
10.1088/1361-6382/acc50f
2-s2.0-85151503331
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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