Publication Date:
2016-08-24
Description:
Author(s): Shahar Hod Charged rotating Kerr-Newman black holes are known to be superradiantly unstable to perturbations of charged massive bosonic fields whose proper frequencies lie in the bounded regime 0 〈 ω 〈 min { ω c ≡ m Ω H + q Φ H , μ } , where { Ω H , Φ H } are, respectively, the angular velocity and electric potential of the Kerr… [Phys. Rev. D 94, 044036] Published Mon Aug 22, 2016
Keywords:
General relativity, alternative theories of gravity
Print ISSN:
0556-2821
Electronic ISSN:
1089-4918
Topics:
Physics
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