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: 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 acesso aberto
- Este artigo NÃO é de acesso aberto
-
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: 10 fev. 2026. -
APA
Lin, K., Qian, W. -L., Pavan, A. B., & Abdalla, E. (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 E. 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 2026 fev. 10 ] Available from: https://doi.org/10.1142/S0217732317501346 -
Vancouver
Lin K, Qian W-L, Pavan AB, Abdalla E. 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 2026 fev. 10 ] Available from: https://doi.org/10.1142/S0217732317501346 - (Anti-) de Sitter electrically charged black-hole solutions in higher-derivative gravity
- Hawking radiation received at infinity in higher dimensional Reissner-Nordström black hole spacetimes
- Quasinormal modes for the Vaidya metric in asymptotically anti–de sitter spacetime
- The matrix method for black hole quasinormal modes
- Scalar quasinormal modes of nonlinear charged black holes in Rastall gravity
- Quasinormal modes in two-photon autocorrelation and the geometric-optics approximation
- Cuspy and fractured black hole shadows in a toy model with axisymmetry
- Shadows of magnetically charged rotating black holes surrounded by quintessence
- Cosmological-model-independent tests of cosmic distance duality relation with Type Ia supernovae and radio quasars
- Detection of scalar fields by extreme mass ratio inspirals with a Kerr black hole
Informações sobre o DOI: 10.1142/S0217732317501346 (Fonte: oaDOI API)
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