Superradiance and quasinormal modes of the gravitational perturbation around rotating hairy black hole
The No Hair theorem in classical general relativity predicts that rotating black holes are specified by the Kerr metric, which is uniquely identified by the mass and spin. However, as a pioneering study beyond general relativity, the rotating hairy black hole has been proposed, which encompasses the...
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| Format: | Article |
| Language: | English |
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Elsevier
2023-06-01
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| Series: | Physics Letters B |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269323002368 |