Khireddine Nouicer 2007 Class. Quantum Grav. 24 5917 doi:10.1088/0264-9381/24/23/014
Khireddine Nouicer1
Show affiliationsWe 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 fewer 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 a black hole remnant with zero entropy, zero heat capacity and nonzero finite temperature. We finally compare our results with those obtained in the standard Hawking picture and with the GUP to leading order in the Planck length.
04.70.Dy Quantum aspects of black holes, evaporation, thermodynamics
04.50.-h Higher-dimensional gravity and other theories of gravity
83C45 Quantization of the gravitational field
Issue 23 (7 December 2007)
Received 20 July 2007, in final form 9 October 2007
Published 21 November 2007
A Corrigendum for this article has been published in 2007 Class. Quantum Grav. 24 6435
Khireddine Nouicer 2007 Class. Quantum Grav. 24 5917
Lev Vaidman 2007 J. Phys. A: Math. Theor. 40 3275
C L Lu et al 2006 J. Phys.: Condens. Matter 18 5849
John P Killingbeck et al 2005 J. Phys. A: Math. Gen. 38 L695
Péter Csizmadia 2007 Class. Quantum Grav. 24 S369
L. Verde et al. 2003 ApJS 148 195
John J. Feldmeier et al 1996 ApJ 461 L25
Eli Waxman 2004 ApJ 602 886
A Berko et al 2009 J. Phys.: Conf. Ser. 190 012147
Benjamin Bahr and Bianca Dittrich 2009 Class. Quantum Grav. 26 225011