Dirac quasinormal modes of power-Maxwell charged black holes in Rastall gravity

DOI10.1142/S021773232050193XzbMath1443.83053arXiv2005.00674OpenAlexW3105674240MaRDI QIDQ4971731

Cheng-Gang Shao, YuJie Tan, Yu Hu, Wei-Liang Qian, Kai Lin, Cai-Ying Shao

Publication date: 12 October 2020

Published in: Modern Physics Letters A (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2005.00674

zbMATH Keywords

black holeDirac fieldquasinormal modesRastall gravitylate-time tail

Mathematics Subject Classification ID

Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Spinor and twistor methods in general relativity and gravitational theory; Newman-Penrose formalism (83C60)

Related Items (3)

High-order matrix method with delimited expansion domain ⋮ Thermal stability and tunneling radiation in van der Waals black hole ⋮ Gravitational lensing for power-Maxwell charged quintessence black hole in Rastall gravity

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