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