The remnants in Reissner–Nordström–de Sitter quintessence black hole
Zhong-Wen FengSchool of Physical Electronics, University of Electronic Science and Technology of China, Chengdu 610054, P. R. ChinaLi ZhangSchool of Physical Electronics, University of Electronic Science and Technology of China, Chengdu 610054, P. R. ChinaXiaotao ZuSchool of Physical Electronics, University of Electronic Science and Technology of China, Chengdu 610054, P. R. China
2014en
ABI
Аннотация
According to the effects of quantum gravity, we investigated the fermion tunneling from the Reissner–Nordström–de Sitter quintessence (RN–dSQ) black hole. The corrected temperature is not only determined by the mass and charge of the black hole, but also depended on the quantum number of the emitted fermion and β, which is a small value representing the effects of quantum gravity. The effects of quantum gravity slowed down the increase of the temperature and led to the remnants of the black hole. We think it is a method to avoid the information loss paradox of black holes.
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