Aspects of noncommutative (1+1)-dimensional black holes

Jonas R. Mureika and Piero Nicolini
Phys. Rev. D 84, 044020 – Published 4 August 2011

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 θ 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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  • Received 29 May 2011

DOI:https://doi.org/10.1103/PhysRevD.84.044020

© 2011 American Physical Society

Authors & Affiliations

Jonas R. Mureika*

  • Department of Physics, Loyola Marymount University, Los Angeles, California 90045-2659, USA

Piero Nicolini

  • Frankfurt Institute for Advandced Studies (FIAS), Goethe-Universität, Frankfurt am Main, Germany and Institut für Theoretische Physik, Goethe-Universität, Frankfurt am Main, Germany

  • *jmureika@lmu.edu
  • nicolini@th.physik.uni-frankfurt.de

See Also

Charged rotating noncommutative black holes

Leonardo Modesto and Piero Nicolini
Phys. Rev. D 82, 104035 (2010)

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Vol. 84, Iss. 4 — 15 August 2011

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