Hawking radiation of charged Dirac particles from a Kerr-Newman black hole

2008 ◽  
Vol 77 (10) ◽  
Author(s):  
Shiwei Zhou ◽  
Wenbiao Liu
2007 ◽  
Vol 46 (12) ◽  
pp. 3067-3071 ◽  
Author(s):  
DeYou Chen ◽  
ShuZheng Yang

Author(s):  
Pu-Jian Mao ◽  
Ran Li ◽  
Lin-Yu Jia ◽  
Ji-Rong Ren

2013 ◽  
Vol 2013 ◽  
pp. 1-6 ◽  
Author(s):  
Ge-Rui Chen ◽  
Yong-Chang Huang

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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