Quasinormal modes and the correspondence with shadow in black holes with a deficit solid angle and quintessence-like matter
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Publication:2169473
DOI10.1016/j.nuclphysb.2022.115925OpenAlexW4290792904MaRDI QIDQ2169473
Chengye Yu, Chuanhong Gao, De-You Chen
Publication date: 2 September 2022
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2207.06796
Relativistic cosmology (83F05) Black holes (83C57) Quantum optics (81V80) Semiclassical techniques, including WKB and Maslov methods applied to problems in quantum theory (81Q20) Mono-, di- and multipole moments (EM and other), gyromagnetic relations (81V60)
Cites Work
- Unnamed Item
- Electromagnetic quasinormal modes of rotating black strings and the AdS/CFT correspondence
- A new approach to black hole quasinormal modes: a review of the asymptotic iteration method
- Quasinormal modes of Rarita-Schwinger field in Reissner-Nordström black hole spacetimes
- Analytical correspondence between shadow radius and black hole quasinormal frequencies
- Quasinormal modes of a black hole with quintessence-like matter and a deficit solid angle: Scalar and gravitational perturbations
- The large-\(N\) limit of superconformal field theories and supergravity
- Geodesics of Hayward black hole surrounded by quintessence
- Are eikonal quasinormal modes linked to the unstable circular null geodesics?
- Spectral decomposition of the perturbation response of the Schwarzschild geometry
- Black-hole normal modes: Phase-integral treatment
- Black hole quasinormal modes using the asymptotic iteration method
- Quintessence and black holes
- Higher order WKB formula for quasinormal modes and grey-body factors: recipes for quick and accurate calculations
- A matrix method for quasinormal modes: Schwarzschild black holes in asymptotically flat and (anti-) de Sitter spacetimes
- Quasinormal modes of Reissner-Nordström anti-de Sitter black holes
- Interplay between gravity and quintessence: a set of new GR solutions
