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The cosmological constant and black-hole thermodynamic potentials
Classical and Quantum Gravity · 2011 · Vol. 28(12) · pp. 125020–125020
Brian P. Dolan✉(Dublin Institute For Advanced Studies)
Abstract
Abstract\nThe thermodynamics of black holes in various dimensions are described in the presence of a negative cosmological constant which is treated as a thermodynamic variable, interpreted as a pressure in the equation of state. The black hole mass is then identified with the enthalpy, rather than the internal energy, and heat capacities are calculated at constant pressure not at constant volume. The Euclidean action is associated with a bridge equation for the Gibbs free energy and not the Helmholtz free energy. Quantum corrections to the enthalpy and the equation of state of the BTZ black hole are studied.
Black Holes and Theoretical PhysicsCosmology and Gravitation TheoriesAstrophysical Phenomena and ObservationsPhysicsCosmological constantHelmholtz free energyEquation of stateThermodynamicsGibbs free energyThermodynamic free energyGibbs–Helmholtz equationInternal energyEnthalpy
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