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Paper   IPM / P / 14258
School of Physics
  Title:   Conserved charges and first law of thermodynamics for Kerr-de Sitter black holes
  Author(s):  K. Hajian
  Status:   Published
  Journal: General Relativity and Gravitation
  No.:  8
  Vol.:  48
  Year:  2016
  Pages:   114
  Supported by:  IPM
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.

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