Relaxation rate of RNdS black hole
From MaRDI portal
Publication:2663445
DOI10.1016/J.PHYSLETB.2020.135523zbMath1458.83005arXiv2005.12722OpenAlexW3028732960MaRDI QIDQ2663445
Ming Zhang, Jie Jiang, Zhen Zhong
Publication date: 19 April 2021
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2005.12722
Related Items (1)
Uses Software
Cites Work
- Extremal Kerr-Newman black holes with extremely short charged scalar hair
- Gravitational spectrum of black holes in the Einstein-aether theory
- The instability spectra of near-extremal Reissner-Nordström-de Sitter black holes
- The longlived charged massive scalar field in the higher-dimensional Reissner-Nordström spacetime
- The fastest relaxation rate of higher-dimensional Reissner-Nordström black hole
- Slowly decaying resonances of charged massive scalar fields in the Reissner-Nordström black-hole spacetime
- Charged massive scalar field configurations supported by a spherically symmetric charged reflecting shell
- Strong cosmic censorship in higher-dimensional Reissner-Nordström-de Sitter spacetime
- Strong cosmic censorship in charged black-hole spacetimes: as strong as ever
- Quasinormal modes of black holes and black branes
- Bohr's Correspondence Principle and the Area Spectrum of Quantum Black Holes
- Scalar clouds around Kerr–Sen black holes
- Field propagation in de Sitter black holes
- Quasinormal modes: the characteristic `sound' of black holes and neutron stars
This page was built for publication: Relaxation rate of RNdS black hole
