Analytic treatment of the system of a Kerr-Newman black hole and a charged massive scalar field
arXiv:1609.07146 · doi:10.1103/PhysRevD.94.044036
Abstract
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 [here are respectively the angular velocity and electric potential of the Kerr-Newman black hole, and are respectively the azimuthal harmonic index, the charge coupling constant, and the proper mass of the field]. In this paper we study analytically the complex resonance spectrum which characterizes the dynamics of linearized charged massive scalar fields in a near-extremal Kerr-Newman black-hole spacetime. Interestingly, it is shown that near the critical frequency for superradiant amplification and in the eikonal large-mass regime, the superradiant instability growth rates of the explosive scalar fields are characterized by a non-trivial (non-monotonic) dependence on the dimensionless charge-to-mass ratio . In particular, for given parameters of the central Kerr-Newman black hole, we determine analytically the optimal charge-to-mass ratio of the explosive scalar field which {\it maximizes} the growth rate of the superradiant instabilities in the composed Kerr-Newman-black-hole-charged-massive-scalar-field system.
arXiv comment11 pages
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