Black hole entropy in 3D gravity with torsion
M. Blagojevic, B. Cvetkovic
TL;DR
This paper explores how torsion affects black hole entropy in 3D quantum gravity, showing deviations from the standard formula but maintaining thermodynamic consistency.
Contribution
It introduces the impact of torsion in 3D gravity on black hole entropy and demonstrates its compatibility with thermodynamic laws.
Findings
Black hole entropy with torsion differs from Bekenstein-Hawking formula.
Entropy remains consistent with the first law of thermodynamics.
Torsion influences quantum properties of 3D black holes.
Abstract
The role of torsion in quantum three-dimensional gravity is investigated by studying the partition function of the Euclidean theory in Riemann-Cartan spacetime. The entropy of the black hole with torsion is found to differ from the standard Bekenstein-Hawking result, but its form is in complete agreement with the first law of black hole thermodynamics.
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