Three dimensional charged black holes in Gauss-Bonnet gravity
Kimet Jusufi, Mubasher Jamil, Ahmad Sheykhi

TL;DR
This paper introduces a new class of three-dimensional charged black hole solutions in Gauss-Bonnet gravity incorporating zero-point length effects, analyzing their regularity, thermodynamics, and spinning variants.
Contribution
It constructs regular charged black hole solutions in 3D Gauss-Bonnet gravity with zero-point length effects, including thermodynamic analysis and spinning black hole solutions.
Findings
Potentials are finite and regular everywhere.
Entropy decreases due to stringy effects.
First law of thermodynamics is verified.
Abstract
By using the zero-point length effect, we construct a new class of charged black hole solutions in the framework of three dimensional Gauss-Bonnet (GB) gravity with Maxwell electrodynamics. The gravitational and electromagnetic potentials are finite and regular everywhere, however, the computation of scalar curvature invariants suggest the presence of a singularity at the origin. We also explore thermodynamics of the obtained solutions and reveal that the entropy of the black hole decreases due to the stringy effects. The thermodynamic and conserved quantities are computed and also the validity of the first law of thermodynamics on the black hole horizon is verified. Finally, the spinning black hole solution is also reported.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Astrophysical Phenomena and Observations
