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: Chinese Physics C
- ISSN: 16741137
- Volume/Número/Paginação/Ano: v.43, n.3, p.035105-, 2019
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
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: 24 jan. 2026. -
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 2026 jan. 24 ] 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 2026 jan. 24 ] Available from: https://doi.org/10.1088/1674-1137/43/3/035105 - Echoes of axial gravitational perturbations in stars of uniform density*
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Informações sobre o DOI: 10.1088/1674-1137/43/3/035105 (Fonte: oaDOI API)
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