Source: Classical and Quantum Gravity. Unidade: EEL
Assunto: BURACOS NEGROS
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: 08 maio 2024.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/aa6643NLM
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 2024 maio 08 ] Available from: https://doi.org/10.1088/1361-6382/aa6643Vancouver
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 2024 maio 08 ] Available from: https://doi.org/10.1088/1361-6382/aa6643