Thermodynamic Volume of Kerr-bolt-AdS Spacetime
arXiv:1406.1257
Abstract
In theories of gravity where the cosmological constant defines a thermodynamic variable, the pressure, it has been shown that solutions of Einstein's equations have a corresponding thermodynamic volume. In general, the expression for the volume is not the same as the one arising from naive geometrical considerations. Both rotation and nut charge are properties known in the literature to give non-geometric thermodynamic volumes, and so we combine the two in a single example and compute the volume for the Kerr-bolt-AdS spacetime, presenting a new expression that generalizes the previously known non-geometric cases.
11 pages, 4 figures; v2: some references added
References in corpus (7)
- Black Hole Enthalpy and an Entropy Inequality for the Thermodynamic Volume
- Thermodynamics of de Sitter Black Holes: Thermal Cosmological Constant
- Extended phase space thermodynamics for third order Lovelock black holes in diverse dimensions
- Critical phenomena of static charged AdS black holes in conformal gravity
- The first laws of thermodynamics of the (2+1)-dimensional BTZ black holes and Kerr-de Sitter spacetimes
- Stringy Generalization of the First Law of Thermodynamics for Rotating BTZ Black Hole with a Cosmological Constant as State Parameter
- Thermodynamics Of A Class Of Kerr-Bolt-Ads Spacetime
Cited by in corpus (4)
- Multiple Reentrant Phase Transitions and Triple Points in Lovelock Thermodynamics
- Black holes and Boyle's law -- the thermodynamics of the cosmological constant
- The Extended Thermodynamic Properties of Taub-NUT/Bolt-AdS spaces
- The correspondence between thermodynamic curvature and isoperimetric theorem from ultraspinning black hole