Publication:526323
From MaRDI portal
Publication:526323
{{DISPLAYTITLE:Extremal Kerr-Newman black holes with extremely short charged scalar hair
DOI10.1016/j.physletb.2015.10.039zbMath1360.83033arXiv1707.06246OpenAlexW2100425610MaRDI QIDQ526323
Publication date: 10 May 2017
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1707.06246
Related Items
The superradiant instability regime of the spinning Kerr black hole, Kerr-Newman black holes with scalar hair, On instabilities of scalar hairy regular compact reflecting stars, Relaxation rate of RNdS black hole, Spinning Kerr black holes with stationary massive scalar clouds: the large-coupling regime, On instabilities of stationary scalar field configurations supported by reflecting compact stars, The fastest relaxation rate of higher-dimensional Reissner-Nordström black hole, Hair distributions in noncommutative Einstein-Born-Infeld black holes, Stationary scalar clouds around a BTZ black hole, Onset of superradiant instabilities in rotating spacetimes of exotic compact objects, The charged black-hole bomb: a lower bound on the charge-to-mass ratio of the explosive scalar field, The extreme orbital period in scalar hairy Kerr black holes, Kerr black holes with synchronised scalar hair and boson stars in the Einstein-Friedberg-Lee-Sirlin model, The fastest relaxation rate of Born-Infeld black hole, Analytic and asymptotically flat hairy (ultra-compact) black-hole solutions and their axial perturbations
Cites Work
- Unnamed Item
- Unnamed Item
- Eigenvalue spectrum of the spheroidal harmonics: a uniform asymptotic analysis
- Regular and black hole solutions of Einstein-Yang-Mills dilaton theory
- Rotating black holes can have short bristles
- Spherically symmetric static SU(2) Einstein–Yang–Mills fields
- Classes of exact solutions to the Teukolsky master equation
- Gravitational Field of a Spinning Mass as an Example of Algebraically Special Metrics
- Do collapsed boson stars result in new types of black holes?
- A simple proof of a no-hair theorem in Einstein-Higgs theory