PV criticality of higher dimensional charged topological dilaton de Sitter black holes

Hui-Hua Zhao, Li-Chun Zhang, Meng-Sen Ma, and Ren Zhao
Phys. Rev. D 90, 064018 – Published 11 September 2014

Abstract

There are both the black hole horizon and the cosmological horizon for the charged topological dilaton de Sitter spacetime. The thermodynamic quantities on both horizons satisfy the first law of black hole thermodynamics. Because all of these thermodynamic quantities depend on the mass M, the electric charge Q, and the cosmological constant l, the two horizons are not independent. Considering the connection between the black hole horizon and the cosmological horizon, we derive the effective thermodynamic quantities of the (n+1)-dimensional charged topological dilaton de Sitter spacetime. We find that the charged topological dilaton black hole in de Sitter spacetime has a similar phase transition and critical behavior to that in anti–de Sitter spacetime.

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  • Received 15 May 2014

DOI:https://doi.org/10.1103/PhysRevD.90.064018

© 2014 American Physical Society

Authors & Affiliations

Hui-Hua Zhao1,2, Li-Chun Zhang1,2, Meng-Sen Ma1,2, and Ren Zhao1,2

  • 1Institute of theoretical physics, Shanxi Datong University, 037009 Datong, China
  • 2Department of Physics, Shanxi Datong University, 037009 Datong, China

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Issue

Vol. 90, Iss. 6 — 15 September 2014

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