Hawking radiation - quasi-normal modes correspondence and effective states for nonextremal Reissner-Nordström black holes

Abstract

It is known that the nonstrictly thermal character of the Hawking radiation spectrum harmonizes Hawking radiation with black hole (BH) quasi-normal modes (QNM). This paramount issue has been recently analyzed in the framework of both Schwarzschild BHs (SBH) and Kerr BHs (KBH). In this assignment, we generalize the analysis to the framework of nonextremal Reissner-Nordström BHs (RNBH). Such a generalization is important because in both SBHs and KBHs an absorbed (or emitted) particle has only mass. Instead, in RNBHs the particle has charge as well as mass. In doing so, we expose that for the RNBH, QNMs can be naturally interpreted in terms of quantum levels for both particle emission and absorption. Conjointly, we generalize some concepts concerning the RNBH's "effective states".

16 pages, accepted for publication in Advances in High Energy Physics

References in corpus (6)

• The physical interpretation of the spectrum of black hole quasinormal modes
• Quantum Tunneling and Trace Anomaly
• Effective temperature, Hawking radiation and quasinormal modes
• Area spectrum of the d-dimensional Reissner-Nordstrom black hole in the small charge limit
• Noncommutative information is revealed from Hawking radiation as tunneling
• Comment on "What the information loss is {\it not}"

Cited by in corpus (10)

• Quasinormal modes of nonlinear electromagnetic black holes from unstable null geodesics
• Nonlinear Electromagnetic Quasinormal Modes and Hawking Radiation of A Regular Black Hole with Magnetic Charge
• Quasi-normal modes: the "electrons" of black holes as "gravitational atoms"? Implications for the black hole information puzzle
• Gravitational Quasinormal Modes of Regular Phantom Black Hole
• Hawking radiation-quasinormal modes correspondence for large AdS black holes
• Quantum Tunnelling for Hawking Radiation from Both Static and Dynamic Black Holes
• The information loss problem and Hawking radiation as tunneling
• On quasi-normal modes, area quantization and Bohr correspondence principle
• Quantum corrected non-thermal radiation spectrum from the tunnelling mechanism
• Initiating the effective unification of black hole horizon area and entropy quantization with quasi-normal modes