Entropy in three-dimensional general relativity: Kerr-AdS black hole
arXiv:1911.11261 · doi:10.1016/j.physletb.2019.135180
Abstract
Black hole thermodynamics of the Kerr-AdS spacetime in three-dimensional general relativity is analyzed using a Hamiltonian approach. The values of the conserved charges and entropy, obtained by a proper treatment of the AdS asymptotic conditions, are shown to satisfy the first law of black hole dynamics.
arXiv commentLaTeX, 9 pages; v2 minor changes
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