Long-lived resonances of massive scalar fields in the Reissner-Nordstr"om black-hole spacetime: Analytic treatment in the large-mass regime
gr-qc, astro-ph.HE, hep-th
Submitted: 2025-11-13
Updated: 2025-11-13
Comments: 9 pages
Journal ref: Phys. Lett. B 874, 140228 (2026)
License: http://creativecommons.org/licenses/by/4.0/
The gist: The physical and mathematical properties of the composed Reissner-Nordström-black-hole-massive-scalar-field system are studied analytically in the dimensionless large-mass Mμ 1 regime [here M,μ
Terminology
Abstract
The physical and mathematical properties of the composed Reissner-Nordström-black-hole-massive-scalar-field system are studied analytically in the dimensionless large-mass Mμ 1 regime [here M,μ are respectively the mass of the central black hole and the proper mass of the scalar field]. It is proved that, for a given value Q Q/M of the dimensionless charge parameter of the central black hole, the system is characterized by the presence of quasi-resonances, linearized perturbation modes with arbitrarily long lifetimes. In particular, using analytical techniques, we determine the black-hole-field critical mass spectrum Mμ crit(Q) which characterizes the long-lived resonances of the composed physical system.
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