Criticality and surface tension in rotating horizon thermodynamics

DOI10.1088/0264-9381/33/16/165005zbMath1346.83039arXiv1604.06312OpenAlexW3104577700WikidataQ60720993 ScholiaQ60720993MaRDI QIDQ2822165

David Kubizňák, Robert B. Mann, Devin Hansen

Publication date: 27 September 2016

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1604.06312

zbMATH Keywords

criticalitythermodynamicsblack holes

Mathematics Subject Classification ID

Black holes (83C57) Dynamical systems in other branches of physics (quantum mechanics, general relativity, laser physics) (37N20) Gravitational energy and conservation laws; groups of motions (83C40) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Classical and relativistic thermodynamics (80A10)

Related Items (10)

Horizon thermodynamics from Einstein's equation of state ⋮ Universality of \(P - V\) criticality in horizon thermodynamics ⋮ Thermodynamics of two black holes ⋮ Thermodynamic properties of Schwarzschild black hole in non-commutative gauge theory of gravity ⋮ Quantum tunneling from Schwarzschild black hole in non-commutative gauge theory of gravity ⋮ Quasi-Local Masses of Rotating Space-Times ^* ⋮ The Kerr-Newman black hole as a rotating Van der Waals gas ⋮ The role of the cosmological constant as a pressure in the \((2 + 1)\)-dimensional black string ⋮ The modified first laws of thermodynamics of anti-de Sitter and de Sitter space-times ⋮ Modifying horizon thermodynamics by surface tensions

This page was built for publication: Criticality and surface tension in rotating horizon thermodynamics