Corrected Hawking Radiation of Dirac Particles from a General Static Riemann Black Hole
Author(s) -
Ge-Rui Chen,
Yong-Chang Huang
Publication year - 2013
Publication title -
advances in high energy physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.59
H-Index - 49
eISSN - 1687-7365
pISSN - 1687-7357
DOI - 10.1155/2013/982146
Subject(s) - physics , hawking radiation , black hole information paradox , black hole (networking) , unitarity , micro black hole , dirac (video compression format) , extremal black hole , black hole thermodynamics , negative energy , white hole , quantum field theory in curved spacetime , quantum electrodynamics , quantum mechanics , mathematical physics , quantum gravity , quantum , gravitational wave , computer network , routing protocol , routing (electronic design automation) , entropy (arrow of time) , planck , computer science , neutrino , link state routing protocol
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
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