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Observing remnants by fermions' tunneling

The standard Hawking formula predicts the complete evaporation of black holes. In this paper, we introduce effects of quantum gravity into fermions' tunneling from Reissner-Nordstrom and Kerr black holes. The quantum gravity effects slow down the increase of Hawking temperatures. This property naturally leads to a residue mass in black hole evaporation. The corrected temperatures are affected by the quantum numbers of emitted fermions. Meanwhile, the temperature of the Kerr black hole is a function of $θ$ due to the rotation.

preprint2014arXivOpen access
Deyou ChenHouwen WuHaitang Yang
gr-qchep-th
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Open access3 authors2 topics
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Deyou ChenHouwen WuHaitang Yang

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