Abstract
We present a comprehensive analysis of the spacetime structure and thermodynamics of ()-dimensional black holes in a noncommutative framework. It is shown that a wider variety of solutions are possible than the commutative case considered previously in the literature. As expected, the introduction of a minimal length cures singularity pathologies that plague the standard two-dimensional general relativistic case, where the latter solution is recovered at large length scales. Depending on the choice of input parameters (black hole mass , cosmological constant , etc.), black hole solutions with zero, up to six, horizons are possible. The associated thermodynamics allows for the either complete evaporation, or the production of black hole remnants.
5 More- Received 29 May 2011
DOI:https://doi.org/10.1103/PhysRevD.84.044020
© 2011 American Physical Society