A matrix method for quasinormal modes: Kerr and Kerr–Sen black holes (2017)
Source: Modern Physics Letters A. Unidades: EEL, IF
Subjects: COSMOLOGIA, BURACOS NEGROS
ABNT
LIN, Kai et al. A matrix method for quasinormal modes: Kerr and Kerr–Sen black holes. Modern Physics Letters A, v. 32, n. 25, p. 1750134/1-1750134/9, 2017Tradução . . Disponível em: https://doi.org/10.1142/S0217732317501346. Acesso em: 18 ago. 2024.APA
Lin, K., Qian, W. -L., Pavan, A. B., & Abdalla, É. (2017). A matrix method for quasinormal modes: Kerr and Kerr–Sen black holes. Modern Physics Letters A, 32( 25), 1750134/1-1750134/9. doi:10.1142/S0217732317501346NLM
Lin K, Qian W-L, Pavan AB, Abdalla É. A matrix method for quasinormal modes: Kerr and Kerr–Sen black holes [Internet]. Modern Physics Letters A. 2017 ; 32( 25): 1750134/1-1750134/9.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1142/S0217732317501346Vancouver
Lin K, Qian W-L, Pavan AB, Abdalla É. A matrix method for quasinormal modes: Kerr and Kerr–Sen black holes [Internet]. Modern Physics Letters A. 2017 ; 32( 25): 1750134/1-1750134/9.[citado 2024 ago. 18 ] Available from: https://doi.org/10.1142/S0217732317501346