Entropy of Kerr--Newman--AdS black holes with torsion
arXiv:2203.14696 · doi:10.1103/PhysRevD.105.104014
Abstract
The canonical approach to black hole entropy in Poincaré gauge theory without matter is extended to include Maxwell field as a matter source. The new formalism is used to calculate asymptotic charges and entropy of Kerr--Newmann--AdS black holes with torsion. The result implies that the first law, with a nontrivial contribution of the Maxwell field, takes the same form as in general relativity.
LaTex, 17 pages
References in corpus (6)
- Exact Solutions in Poincaré Gauge Gravity Theory
- Entropy in Poincaré gauge theory: Hamiltonian approach
- Entropy of Reissner-Nordström-like black holes
- Entropy in general relativity: Kerr-AdS black hole
- Entropy in Poincaré gauge theory: Kerr-AdS solution
- Thermodynamics of Riemannian Kerr-AdS black holes in Poincaré gauge theory