Gravitational Quasinormal Modes of Regular Phantom Black Hole (2017)
- Authors:
- Autor USP: QIAN, WEILIANG - EEL
- Unidade: EEL
- DOI: 10.1155/2017/5234214
- Assunto: BURACOS NEGROS
- Language: Inglês
- Imprenta:
- Publisher place: New York, US
- Date published: 2017
- Source:
- Título: Advances in High Energy Physics
- ISSN: 1687-7365
- Volume/Número/Paginação/Ano: v.2017, Article ID 5234214,2017
- Este periódico é de acesso aberto
- Este artigo NÃO é de acesso aberto
-
ABNT
LI, J. et al. Gravitational Quasinormal Modes of Regular Phantom Black Hole. Advances in High Energy Physics, v. 2017, 2017Tradução . . Disponível em: https://doi.org/10.1155/2017/5234214. Acesso em: 13 fev. 2026. -
APA
Li, J., Ka, L., Wen, H., & Qian, W. -L. (2017). Gravitational Quasinormal Modes of Regular Phantom Black Hole. Advances in High Energy Physics, 2017. doi:10.1155/2017/5234214 -
NLM
Li J, Ka L, Wen H, Qian W-L. Gravitational Quasinormal Modes of Regular Phantom Black Hole [Internet]. Advances in High Energy Physics. 2017 ;2017[citado 2026 fev. 13 ] Available from: https://doi.org/10.1155/2017/5234214 -
Vancouver
Li J, Ka L, Wen H, Qian W-L. Gravitational Quasinormal Modes of Regular Phantom Black Hole [Internet]. Advances in High Energy Physics. 2017 ;2017[citado 2026 fev. 13 ] Available from: https://doi.org/10.1155/2017/5234214 - 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
- Combinatorial algebraic approach for modified second-generation time-delay interferometry
- Scalar quasinormal modes of anti–de Sitter static spacetime in Horava-Lifshitz gravity with U ( 1 ) symmetry
- A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes
Informações sobre o DOI: 10.1155/2017/5234214 (Fonte: oaDOI API)
How to cite
A citação é gerada automaticamente e pode não estar totalmente de acordo com as normas
