A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes (2017)
- Authors:
- Autor USP: QIAN, WEILIANG - EEL
- Unidade: EEL
- DOI: 10.1088/1361-6382/aa6643
- Assunto: BURACOS NEGROS
- Language: Inglês
- Imprenta:
- Publisher place: Bristol, U. K.
- Date published: 2017
- Source:
- Título: Classical and Quantum Gravity
- ISSN: 1361-6382
- Volume/Número/Paginação/Ano: v.34, n. 9, p.095004, 2017
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
- Licença: other-oa
-
ABNT
LIN, Kai e QIAN, Wei-liang. A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes. Classical and Quantum Gravity, v. 34, n. 9, p. 095004, 2017Tradução . . Disponível em: https://doi.org/10.1088/1361-6382/aa6643. Acesso em: 10 jan. 2026. -
APA
Lin, K., & Qian, W. -liang. (2017). A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes. Classical and Quantum Gravity, 34( 9), 095004. doi:10.1088/1361-6382/aa6643 -
NLM
Lin K, Qian W-liang. A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes [Internet]. Classical and Quantum Gravity. 2017 ;34( 9): 095004.[citado 2026 jan. 10 ] Available from: https://doi.org/10.1088/1361-6382/aa6643 -
Vancouver
Lin K, Qian W-liang. A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes [Internet]. Classical and Quantum Gravity. 2017 ;34( 9): 095004.[citado 2026 jan. 10 ] Available from: https://doi.org/10.1088/1361-6382/aa6643 - A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes
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Informações sobre o DOI: 10.1088/1361-6382/aa6643 (Fonte: oaDOI API)
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