Hawking Radiation-Quasi-Normal Modes Correspondence and Effective States for Nonextremal Reissner-Nordström Black Holes

Corda, C. (Dipartimento di Fisica e Chimica, Università Santa Rita and Institute for Theoretical Physics and Advanced Mathematics Einstein-Galilei (IFM), 59100 Prato, Italy) (International Institute for Applicable Mathematics & Information Sciences (IIAMIS), Hyderabad, India) (International Institute for Applicable Mathematics & Information Sciences (IIAMIS), Udine, Italy) ; Hendi, S. H.  (Physics Department and Biruni Observatory, College of Sciences, Shiraz University, Shiraz 71454, Iran) (Research Institute for Astrophysics and Astronomy of Maragha (RIAAM), P.O. Box 55134-441, Maragha, Iran) ; Katebi, R. (Department of Physics, California State University Fullerton, 800 North State College Boulevard, Fullerton, CA 92831, USA) ; Schmidt, N. O. (Department of Mathematics, Boise State University, 1910 University Drive, Boise, ID 83725, USA)

11 February 2014

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 Schwarzschild and Kerr BHs an absorbed (emitted) particle has only mass. Instead, in RNBH 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.”

Published in: Advances in High Energy Physics 2014 (2014) 527874
Published by: Hindawi Publishing Corporation
DOI: 10.1155/2014/527874
License: CC-BY-3.0

Back to search

Download fulltextPDF Download fulltextXML Download fulltextPDF (PDFA)