On the late-time tails of massive perturbations in spherically symmetric black holes

Registro completo de metadados
MetadadosDescriçãoIdioma
Autor(es): dc.contributorYangzhou University-
Autor(es): dc.contributorUniversidade de São Paulo (USP)-
Autor(es): dc.contributorUniversidade Estadual Paulista (UNESP)-
Autor(es): dc.contributorChina University of Geosciences-
Autor(es): dc.contributorHuazhong University of Science and Technology-
Autor(es): dc.contributorShanghai Jiao Tong University-
Autor(es): dc.creatorQian, Wei-Liang-
Autor(es): dc.creatorLin, Kai-
Autor(es): dc.creatorShao, Cai-Ying-
Autor(es): dc.creatorWang, Bin-
Autor(es): dc.creatorYue, Rui-Hong-
Data de aceite: dc.date.accessioned2025-08-21T23:28:36Z-
Data de disponibilização: dc.date.available2025-08-21T23:28:36Z-
Data de envio: dc.date.issued2023-07-29-
Data de envio: dc.date.issued2023-07-29-
Data de envio: dc.date.issued2022-10-01-
Fonte completa do material: dc.identifierhttp://dx.doi.org/10.1140/epjc/s10052-022-10910-z-
Fonte completa do material: dc.identifierhttp://hdl.handle.net/11449/246114-
Fonte: dc.identifier.urihttp://educapes.capes.gov.br/handle/11449/246114-
Descrição: dc.descriptionIt was first pointed out by Koyama and Tomimatsu that, under reasonable assumptions, the asymptotic late-time tails of massive scalar perturbations in the far zone of spherically symmetric black hole spacetimes decay universally as t- 5 / 6. The late-time tail is furnished by the contribution from the branch cut of the frequency-domain Green’s function, which is constructed in terms of two appropriate solutions of the corresponding homogeneous equation. The present study focuses on some particular forms of the in-going wave that were not explicitly considered in the original derivations but nonetheless have been taken into account in the literature by other authors. In this regard, we reassess the authors’ arguments and provide a detailed complimentary analysis that covers a few specific aspects. For some particular cases, the tail is found to possess the form t- 1. We also discuss the possible implications of the present findings.-
Descrição: dc.descriptionCoordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)-
Descrição: dc.descriptionConselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)-
Descrição: dc.descriptionFundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)-
Descrição: dc.descriptionNational Natural Science Foundation of China-
Descrição: dc.descriptionCenter for Gravitation and Cosmology School of Physical Science and Technology Yangzhou University, Jiangsu-
Descrição: dc.descriptionEscola de Engenharia de Lorena Universidade de São Paulo, SP-
Descrição: dc.descriptionFaculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista, SP-
Descrição: dc.descriptionHubei Subsurface Multi-scale Imaging Key Laboratory Institute of Geophysics and Geomatics China University of Geosciences, Hubei-
Descrição: dc.descriptionMOE Key Laboratory of Fundamental Physical Quantities Measurement Hubei Key Laboratory of Gravitation and Quantum Physics PGMF and School of Physics Huazhong University of Science and Technology, Hubei-
Descrição: dc.descriptionSchool of Aeronautics and Astronautics Shanghai Jiao Tong University-
Descrição: dc.descriptionFaculdade de Engenharia de Guaratinguetá Universidade Estadual Paulista, SP-
Idioma: dc.languageen-
Relação: dc.relationEuropean Physical Journal C-
???dc.source???: dc.sourceScopus-
Título: dc.titleOn the late-time tails of massive perturbations in spherically symmetric black holes-
Tipo de arquivo: dc.typelivro digital-
Aparece nas coleções:Repositório Institucional - Unesp

Não existem arquivos associados a este item.