Quasinormal Modes of the Schwarzschild Black Hole Surrounded by the Quintessence Field in Rastall Gravity
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Publication:3387672
DOI10.1088/0253-6102/70/6/695zbMath1452.83015OpenAlexW2909802854WikidataQ128616335 ScholiaQ128616335MaRDI QIDQ3387672
Publication date: 13 January 2021
Published in: Communications in Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1088/0253-6102/70/6/695
WKB approximationquasinormal modesRastall gravitySchwarzschild black hole surrounded by the quintessence field
Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (7)
Quasinormal modes and Hawking radiation sparsity of GUP corrected black holes in bumblebee gravity with topological defects ⋮ Joule‐Thomson Expansion and Optical Behaviour of Reissner‐Nordström‐Anti‐de Sitter Black Holes in Rastall Gravity Surrounded by a Quintessence Field ⋮ Comparative analysis of Einstein gravity and Rastall gravity for the compact objects ⋮ Quasinormal modes of nonlinearly charged black holes surrounded by a cloud of strings in Rastall gravity ⋮ Models of non-static and inhomogeneous gravitating source in Rastall gravity ⋮ Dirac quasinormal modes of power-Maxwell charged black holes in Rastall gravity ⋮ Geodesic Structure of a Non-linear Magnetic Charged Black Hole Surrounded by Quintessence*
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