A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes (2017)
- Autores:
- Autor USP: QIAN, WEILIANG - EEL
- Unidade: EEL
- DOI: 10.1088/1361-6382/aa6643
- Assunto: BURACOS NEGROS
- Idioma: Inglês
- Imprenta:
- Local: Bristol, U.K.
- Data de publicação: 2017
- Fonte:
- Título do periódico: Classical and Quantum Gravity
- ISSN: 1361-6382
- Volume/Número/Paginação/Ano: v. 34, 095004,2017. (13pp)
- Este periódico é de assinatura
- Este artigo é de acesso aberto
- URL de acesso aberto
- Cor do Acesso Aberto: green
- Licença: other-oa
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ABNT
LIN, K. e QIAN, W.-L. A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes. Classical and Quantum Gravity, v. 34, 2017Tradução . . Disponível em: https://doi.org/10.1088/1361-6382/aa6643. Acesso em: 24 abr. 2024. -
APA
Lin, K., & Qian, W. -L. (2017). A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes. Classical and Quantum Gravity, 34. doi:10.1088/1361-6382/aa6643 -
NLM
Lin K, Qian W-L. A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes [Internet]. Classical and Quantum Gravity. 2017 ; 34[citado 2024 abr. 24 ] Available from: https://doi.org/10.1088/1361-6382/aa6643 -
Vancouver
Lin K, Qian W-L. A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes [Internet]. Classical and Quantum Gravity. 2017 ; 34[citado 2024 abr. 24 ] Available from: https://doi.org/10.1088/1361-6382/aa6643 - Onset of chaotic gravitational lensing in non-Kerr rotating black holes with quadrupole mass moment
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Informações sobre o DOI: 10.1088/1361-6382/aa6643 (Fonte: oaDOI API)
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