Hawking Radiation-Quasi-Normal Modes Correspondence and Effective States for Nonextremal Reissner-Nordström Black Holes
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...
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| Main Authors: | , , , |
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| Format: | Article |
| Language: | English |
| Published: |
Wiley
2014-01-01
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| Series: | Advances in High Energy Physics |
| Online Access: | http://dx.doi.org/10.1155/2014/527874 |
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| Summary: | 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.” |
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| ISSN: | 1687-7357 1687-7365 |