Hawking radiation as tunneling from the Kerr and Kerr-Newman black holes
Abstract
Recent work, which treats the Hawking radiation as a semiclassical tunneling process at the horizon of the Schwarzschild and Reissner-Nordstroem spacetimes, indicates that the exact radiant spectrum is no longer pure thermal after considering the black hole background as dynamical and the conservation of energy. In this paper, we extend the method to investigate Hawking radiation as massless particles tunneling across the event horizon of the Kerr black hole and that of charged particles from the Kerr-Newman black hole by taking into account the energy conservation, the angular momentum conservation, and the electric charge conservation. Our results show that when self-gravitation is considered, the tunneling rate is related to the change of Bekenstein-Hawking entropy and the derived emission spectrum deviates from the pure thermal spectrum, but is consistent with an underlying unitary theory.
- Authors:
-
- College of Physical Science and Technology, Central China Normal University, Wuhan, Hubei 430079 (China)
- Publication Date:
- OSTI Identifier:
- 20782637
- Resource Type:
- Journal Article
- Journal Name:
- Physical Review. D, Particles Fields
- Additional Journal Information:
- Journal Volume: 73; Journal Issue: 6; Other Information: DOI: 10.1103/PhysRevD.73.064003; (c) 2006 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0556-2821
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; ANGULAR MOMENTUM; BLACK HOLES; CHARGED PARTICLES; ELECTRIC CHARGES; EMISSION SPECTRA; ENERGY CONSERVATION; ENTROPY; GRAVITATION; MASSLESS PARTICLES; SCHWARZSCHILD METRIC; SEMICLASSICAL APPROXIMATION; SPACE-TIME; TUNNEL EFFECT
Citation Formats
Qingqan, Jiang, Shuangqing, Wu, Xu, Cai, Institute of Theoretical Physics, China West Normal University, Nanchong, Sichuan 637002, College of Physical Science and Technology, Central China Normal University, Wuhan, Hubei 430079, and Institute of Particle Physics, Central China Normal University, Wuhan, Hubei 430079. Hawking radiation as tunneling from the Kerr and Kerr-Newman black holes. United States: N. p., 2006.
Web. doi:10.1103/PHYSREVD.73.064003.
Qingqan, Jiang, Shuangqing, Wu, Xu, Cai, Institute of Theoretical Physics, China West Normal University, Nanchong, Sichuan 637002, College of Physical Science and Technology, Central China Normal University, Wuhan, Hubei 430079, & Institute of Particle Physics, Central China Normal University, Wuhan, Hubei 430079. Hawking radiation as tunneling from the Kerr and Kerr-Newman black holes. United States. https://doi.org/10.1103/PHYSREVD.73.064003
Qingqan, Jiang, Shuangqing, Wu, Xu, Cai, Institute of Theoretical Physics, China West Normal University, Nanchong, Sichuan 637002, College of Physical Science and Technology, Central China Normal University, Wuhan, Hubei 430079, and Institute of Particle Physics, Central China Normal University, Wuhan, Hubei 430079. 2006.
"Hawking radiation as tunneling from the Kerr and Kerr-Newman black holes". United States. https://doi.org/10.1103/PHYSREVD.73.064003.
@article{osti_20782637,
title = {Hawking radiation as tunneling from the Kerr and Kerr-Newman black holes},
author = {Qingqan, Jiang and Shuangqing, Wu and Xu, Cai and Institute of Theoretical Physics, China West Normal University, Nanchong, Sichuan 637002 and College of Physical Science and Technology, Central China Normal University, Wuhan, Hubei 430079 and Institute of Particle Physics, Central China Normal University, Wuhan, Hubei 430079},
abstractNote = {Recent work, which treats the Hawking radiation as a semiclassical tunneling process at the horizon of the Schwarzschild and Reissner-Nordstroem spacetimes, indicates that the exact radiant spectrum is no longer pure thermal after considering the black hole background as dynamical and the conservation of energy. In this paper, we extend the method to investigate Hawking radiation as massless particles tunneling across the event horizon of the Kerr black hole and that of charged particles from the Kerr-Newman black hole by taking into account the energy conservation, the angular momentum conservation, and the electric charge conservation. Our results show that when self-gravitation is considered, the tunneling rate is related to the change of Bekenstein-Hawking entropy and the derived emission spectrum deviates from the pure thermal spectrum, but is consistent with an underlying unitary theory.},
doi = {10.1103/PHYSREVD.73.064003},
url = {https://www.osti.gov/biblio/20782637},
journal = {Physical Review. D, Particles Fields},
issn = {0556-2821},
number = 6,
volume = 73,
place = {United States},
year = {Wed Mar 15 00:00:00 EST 2006},
month = {Wed Mar 15 00:00:00 EST 2006}
}