2007
DOI: 10.1088/0264-9381/24/23/014
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Black hole thermodynamics to all orders in the Planck length in extra dimensions

Abstract: We investigate the effects to all orders in the Planck length, from a generalized uncertainty principle (GUP), on the thermodynamic parameters of radiating Schwarzschild black holes in a scenario with large extra dimensions. We show that black holes in this framework are hotter, have less degrees of freedom and decay faster compared to black holes in the Hawking picture and in the framework with GUP to leading order in the Planck length. Particularly, we show that the final stage of the evaporation process is … Show more

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Cited by 65 publications
(52 citation statements)
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References 94 publications
(120 reference statements)
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“…The black hole thermodynamical stability is related to the sign of its heat capacity C h . In the following, we analyze the thermal stability of the black hole solutions via the behaviour of their heat capacities [104,137,138]…”
Section: Thermodynamical Stability and Phase Transitionmentioning
confidence: 99%
“…The black hole thermodynamical stability is related to the sign of its heat capacity C h . In the following, we analyze the thermal stability of the black hole solutions via the behaviour of their heat capacities [104,137,138]…”
Section: Thermodynamical Stability and Phase Transitionmentioning
confidence: 99%
“…On the other hand, one can derive modified blackhole temperatures for m m p from the GUP [26][27][28][29][30][31][32][33]. In particular, we just recall that one obtains…”
Section: Quantum Black-hole Evaporationmentioning
confidence: 99%
“…Refs. [45][46][47][48][49]51,52,57]). From the standard Heisenberg uncertainty principle we find the green curve, representing the usual Hawking formula.…”
Section: Applications To Micro Black Holesmentioning
confidence: 99%