arXiv · hep-th/0507266
A model of radiating black hole in noncommutative geometry
Abstract
The phenomenology of a radiating Schwarzschild black hole is analyzed in a noncommutative spacetime. It is shown that noncommutativity does not depend on the intensity of the curvature. Thus we legitimately introduce noncommutativity in the weak field limit by a coordinate coherent state approach. The new interesting results are the following: 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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Piero Nicolini. 2005-07-27. A model of radiating black hole in noncommutative geometry. https://doi.org/10.1088/0305-4470%2F38%2F39%2Fl02
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