Phase transition of the higher dimensional charged Gauss-Bonnet black hole in de Sitter spacetime
arXiv:1410.5950
Abstract
We study the phase transition of charged Gauss-Bonnet-de Sitter (GB-dS) black hole. For black holes in de Sitter spacetime, there is not only black hole horizon, but also the cosmological horizon. The thermodynamic quantities on the both horizons satisfy the first law of the black hole thermodynamics, respectively; moreover, there are additional connections between them. Using the effective temperature approach, we obtained the effective thermodynamic quantities of charged GB-dS black hole. According to Ehrenfest classification, we calculate some response functions and plot their figures, from which one can see that the spacetime undergoes a second-order phase transition at the critical point. It is shown that the critical values of effective temperature and pressure decrease with the increase of the value of GB parameter .
9 pages, 16 figures
References in corpus (8)
- Black Hole Enthalpy and an Entropy Inequality for the Thermodynamic Volume
- Critical phenomena and thermodynamic geometry of charged Gauss-Bonnet AdS black holes
- Thermodynamics of de Sitter Black Holes: Thermal Cosmological Constant
- Mechanical First Law of Black Hole Spacetimes with Cosmological Constant and Its Application to Schwarzschild-de Sitter Spacetime
- Thermodynamics of Schwarzschild-de Sitter black hole: thermal stability of Nariai black hole
- Phase transitions of hairy black holes in massive gravity and thermodynamic behavior of charged AdS black holes in an extended phase space
- On The Phase Structure and Thermodynamic Geometry of R-Charged Black Holes
- Vacuum energy and the latent heat of AdS-Kerr black holes