High-order matrix method with delimited expansion domain
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/10.1088/1361-6382/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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Repositório Institucional da UNESP |
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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 |
|
_version_ |
1808129227496620032 |