Entropy in general relativity: Kerr-AdS black hole
arXiv:2002.05029 · doi:10.1103/PhysRevD.101.084023
Abstract
A general Hamiltonian approach to black hole thermodynamics is used to study entropy and conserved charges for Kerr-AdS solutions in general relativity. These thermodynamic variables are first consistently defined by choosing suitable boundary conditions, and then, they are shown to satisfy the first law of black hole dynamics
arXiv commentLaTeX, 12 pages
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