The matrix method for black hole quasinormal modes (2019)
- Authors:
- Autor USP: QIAN, WEILIANG - EEL
- Unidade: EEL
- DOI: 10.1088/1674-1137/43/3/035105
- Assunto: BURACOS NEGROS
- Keywords: quasinormal modes; black hole spacetime; matrix method; quasinormal frequency
- Agências de fomento:
- Language: Inglês
- Abstract: We provide a comprehensive survey of possible applications of the matrix method for black hole quasinormal modes. The proposed algorithm can generally be applied to various background metrics, and in particular, it accommodates both analytic and numerical forms of the tortoise coordinates, as well as black hole spacetimes. We give a detailed account of different types of black hole metrics, master equations, and corresponding boundary conditions. Besides, we argue that the method can readily be applied to cases where the master equation is a system of coupled equations. By adjusting the number of interpolation points, the present method provides a desirable degree of precision, in reasonable balance with its efficiency. The method is flexible and can easily be adopted to various distinct physical scenarios.
- Imprenta:
- Source:
- Título do periódico: Chinese Physics C
- ISSN: 16741137
- Volume/Número/Paginação/Ano: v.43, n.3, p.035105-, 2019
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
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ABNT
LIN, Kai e QIAN, Wei-Liang. The matrix method for black hole quasinormal modes. Chinese Physics C, v. 43, n. 3, p. 035105-, 2019Tradução . . Disponível em: https://doi.org/10.1088/1674-1137/43/3/035105. Acesso em: 23 abr. 2024. -
APA
Lin, K., & Qian, W. -L. (2019). The matrix method for black hole quasinormal modes. Chinese Physics C, 43( 3), 035105-. doi:10.1088/1674-1137/43/3/035105 -
NLM
Lin K, Qian W-L. The matrix method for black hole quasinormal modes [Internet]. Chinese Physics C. 2019 ;43( 3): 035105-.[citado 2024 abr. 23 ] Available from: https://doi.org/10.1088/1674-1137/43/3/035105 -
Vancouver
Lin K, Qian W-L. The matrix method for black hole quasinormal modes [Internet]. Chinese Physics C. 2019 ;43( 3): 035105-.[citado 2024 abr. 23 ] Available from: https://doi.org/10.1088/1674-1137/43/3/035105 - Onset of chaotic gravitational lensing in non-Kerr rotating black holes with quadrupole mass moment
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Informações sobre o DOI: 10.1088/1674-1137/43/3/035105 (Fonte: oaDOI API)
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