2016/02/29 by Kamal Hajian · 1 citation
Physics and Astronomy · #gr-qc #hep-th
paper · pdf · doi:10.1007/s10714-016-2108-4
published as Gen Relativ Gravit (2016) 48: 114 · 20 pages, synchronized with the published version in General Relativity and Gravitation, volume 48, number 8, (2016)
arxiv created 2016/07/28 · arxiv updated 2016/08/02
Recently, a general method for calculating conserved charges for (black hole) solutions to generally covariant gravitational theories, in any dimensions and with arbitrary asymptotic behaviors has been introduced. Equipped with this method, which can be dubbed as "solution phase space method," we calculate mass and angular momentum for the Kerr-dS black holes. Furthermore, for any choice of horizons, associated entropy and the first law of thermodynamics are derived. Interestingly, according to insensitivity of the analysis to the chosen cosmological constant, the analysis unifies the thermodynamics of rotating stationary black holes in 4 (and other) dimensions with either AdS, flat or dS asymptotics. We extend the analysis to include electric charge, i.e. to the Kerr-Newman-dS black holes.