A matrix method for quasinormal modes: Kerr and Kerr–Sen black holes (2017)
- Authors:
- USP affiliated authors: QIAN, WEILIANG - EEL ; ABDALLA, ELCIO - IF
- Unidades: EEL; IF
- DOI: 10.1142/S0217732317501346
- Subjects: COSMOLOGIA; BURACOS NEGROS
- Language: Inglês
- Imprenta:
- Source:
- Título do periódico: Modern Physics Letters A
- ISSN: 0217-7323
- Volume/Número/Paginação/Ano: v. 32, n. 25, p. 1750134/1-1750134/9, 2017
- 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, 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: 19 set. 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/S0217732317501346 -
NLM
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 set. 19 ] Available from: https://doi.org/10.1142/S0217732317501346 -
Vancouver
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 set. 19 ] Available from: https://doi.org/10.1142/S0217732317501346 - Quasinormal modes for the Vaidya metric in asymptotically anti–de sitter spacetime
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Informações sobre o DOI: 10.1142/S0217732317501346 (Fonte: oaDOI API)
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