The fate of radiating black holes in noncommutative geometry

Details The fate of radiating black holes in noncommutative geometry The fate of radiating black holes in noncommutative geometry

2005-07-22

arxiv.org/abs/hep-th/0507226v2

ESA Spec.Publ.637:11.1,2006

Physics

High Energy Physics

High Energy Physics - Theory

5 pages, 3 figures. Contributed to Proceedings of EPS 13 General Conference -"Beyond Einstein, Physics for the 21st Century" J

Scientific paper

We investigate the behavior of a radiating Schwarzschild black hole toy-model in a 2D noncommutative spacetime. It is shown that coordinate noncommutativity leads to: i) the existence of a minimal non-zero mass to which black hole can shrink; ii) a finite maximum temperature that the black hole can reach before cooling down to absolute zero; iii) the absence of any curvature singularity. The proposed scenario offers a possible solution to conventional difficulties when describing terminal phase of black hole evaporation.

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