arXiv · 1104.4120
Aspects of noncommutative (1+1)-dimensional black holes
Abstract
We present a comprehensive analysis of the spacetime structure and thermodynamics of $(1+1)-$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 $\sqrtθ$ 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 $M$, cosmological constant $Λ$, 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.
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Jonas R. Mureika, Piero Nicolini. 2011-08-05. Aspects of noncommutative (1+1)-dimensional black holes. https://doi.org/10.1103/physrevd.84.044020
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