The longlived charged massive scalar field in the higher-dimensional Reissner-Nordström spacetime
From MaRDI portal
Publication:1716694
DOI10.1016/j.physletb.2018.10.072zbMath1406.83013arXiv1811.04183OpenAlexW2899802625MaRDI QIDQ1716694
Jie Jiang, Zhen Zhong, Ming Zhang
Publication date: 5 February 2019
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1811.04183
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Cites Work
- Decay of massive scalar field in a Schwarzschild background
- Strong cosmic censorship for the massless Dirac field in the Reissner-Nordstrom-de Sitter spacetime
- Stationary scalar clouds around a BTZ black hole
- No hair for spherically symmetric neutral reflecting stars: nonminimally coupled massive scalar fields
- Gravitational spectrum of black holes in the Einstein-aether theory
- Stationary bound-state scalar configurations supported by rapidly-spinning exotic compact objects
- Spinning Kerr black holes with stationary massive scalar clouds: the large-coupling regime
- Regular and black hole solutions of Einstein-Yang-Mills dilaton theory
- 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
- Stationary scalar configurations around extremal charged black holes
- Asymptotically flat black holes with scalar hair: A review
- Spectral decomposition of the perturbation response of the Schwarzschild geometry
- Weak Cosmic Censorship: As Strong as Ever
- Quasinormal modes of Schwarzschild black holes: Defined and calculated via Laplace transformation
- Quasinormal modes of black holes and black branes
- Colored black holes
- Black Holes Have No Short Hair
- Bohr's Correspondence Principle and the Area Spectrum of Quantum Black Holes
- Master Equations for Perturbations of Generalised Static Black Holes with Charge in Higher Dimensions
- Stability of Higher-Dimensional Schwarzschild Black Holes
- Massive quasi-normal mode
- Quasinormal modes: the characteristic `sound' of black holes and neutron stars
- Quasi-normal modes of stars and black holes
