Corrected Hawking Radiation of Dirac Particles from a General Static Riemann Black Hole

Considering energy conservation and the back reaction of radiating particles to the spacetime, we investigate the massive Dirac particles' Hawking radiation from a general static Riemann black hole using improved Damour-Ruffini method. A direct consequence is that the radiation spectrum is not...

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Main Authors: Ge-Rui Chen, Yong-Chang Huang
Format: Article
Language:English
Published: Hindawi Limited 2013-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2013/982146
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spelling doaj-a70722841d8341e5ba03ca97cb43f5272020-11-24T22:33:33ZengHindawi LimitedAdvances in High Energy Physics1687-73571687-73652013-01-01201310.1155/2013/982146982146Corrected Hawking Radiation of Dirac Particles from a General Static Riemann Black HoleGe-Rui Chen0Yong-Chang Huang1Institute of Theoretical Physics, Beijing University of Technology, Beijing 100124, ChinaInstitute of Theoretical Physics, Beijing University of Technology, Beijing 100124, ChinaConsidering energy conservation and the back reaction of radiating particles to the spacetime, we investigate the massive Dirac particles' Hawking radiation from a general static Riemann black hole using improved Damour-Ruffini method. A direct consequence is that the radiation spectrum is not strictly thermal. The correction to the thermal spectrum is consistent with an underlying unitary quantum theory and this may have profound implications for the black hole information loss paradox.http://dx.doi.org/10.1155/2013/982146
collection DOAJ
language English
format Article
sources DOAJ
author Ge-Rui Chen
Yong-Chang Huang
spellingShingle Ge-Rui Chen
Yong-Chang Huang
Corrected Hawking Radiation of Dirac Particles from a General Static Riemann Black Hole
Advances in High Energy Physics
author_facet Ge-Rui Chen
Yong-Chang Huang
author_sort Ge-Rui Chen
title Corrected Hawking Radiation of Dirac Particles from a General Static Riemann Black Hole
title_short Corrected Hawking Radiation of Dirac Particles from a General Static Riemann Black Hole
title_full Corrected Hawking Radiation of Dirac Particles from a General Static Riemann Black Hole
title_fullStr Corrected Hawking Radiation of Dirac Particles from a General Static Riemann Black Hole
title_full_unstemmed Corrected Hawking Radiation of Dirac Particles from a General Static Riemann Black Hole
title_sort corrected hawking radiation of dirac particles from a general static riemann black hole
publisher Hindawi Limited
series Advances in High Energy Physics
issn 1687-7357
1687-7365
publishDate 2013-01-01
description Considering energy conservation and the back reaction of radiating particles to the spacetime, we investigate the massive Dirac particles' Hawking radiation from a general static Riemann black hole using improved Damour-Ruffini method. A direct consequence is that the radiation spectrum is not strictly thermal. The correction to the thermal spectrum is consistent with an underlying unitary quantum theory and this may have profound implications for the black hole information loss paradox.
url http://dx.doi.org/10.1155/2013/982146
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AT yongchanghuang correctedhawkingradiationofdiracparticlesfromageneralstaticriemannblackhole
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