期刊
CLASSICAL AND QUANTUM GRAVITY
卷 26, 期 7, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/26/7/075010
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- Natural Science and Engineering Research Council of Canada
We give an approach for studying quantum gravity effects on black hole thermodynamics. This combines a quantum framework for gravitational collapse with quasi-local definitions of energy and surface gravity. Our arguments suggest that (i) the specific heat of a black hole becomes positive after a phase transition near the Planck scale,(ii) its entropy acquires a logarithmic correction and (iii) the mass loss rate is modified such that Hawking radiation stops near the Planck scale. These results are due essentially to a realization of fundamental discreteness in quantum gravity, and are in this sense potentially theory independent.
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