The quasi-normal modes of charged scalar fields in Kerr-Newman black hole and its geometric interpretation

DOI10.1007/JHEP11(2015)167zbMath1388.83511arXiv1506.08276MaRDI QIDQ2636175

Peng Zhao, Yu Tian, Zhao-Yong Sun, Xiao-Ning Wu

Publication date: 31 May 2018

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1506.08276

zbMATH Keywords

black holesclassical theories of gravity

Mathematics Subject Classification ID

Black holes (83C57) Quantum field theory on curved space or space-time backgrounds (81T20)

Related Items (2)

Scalar QNM Spectra of Kerr and Reissner-Nordström revealed by eigenvalue repulsions in Kerr-Newman ⋮ Holographic Einstein ring of a charged AdS black hole

Cites Work

• Unnamed Item
• Relaxation dynamics of charged gravitational collapse
• Quasinormal resonances of near-extremal Kerr-Newman black holes
• Quasi-normal modes and gravitational wave astronomy
• Universality in the relaxation dynamics of the composed black-hole-charged-massive-scalar-field system: the role of quantum Schwinger discharge
• Analytical Solutions for Geodesic Equation in Black Hole Spacetimes
• Quasinormal modes of black holes and black branes
• A note on circular geodesics in the equatorial plane of an extreme Kerr–Newman black hole
• Instability of Massive Scalar Fields in Kerr-Newman Spacetime
• Quasi-normal modes of stars and black holes

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