Surface tension, hydrophobicity, and black holes: The entropic connection
arXiv:cond-mat/9601111 · doi:10.1103/PhysRevE.53.3738
Abstract
Recent calculations have shown that the linear proportionality between black hole entropy and area can be explained by performing a density matrix calculation for a massless free field theory. By applying the same formalism to an empirical fluid ``field theory,'' entropic quantities such as surface tension can be calculated in a novel fashion. Good agreement with experiment is obtained for a number of liquids. This approach may lead to a practical new technique for the evaluation of thermodynamic quantities important entropic components. Implications for the protein folding problem are discussed.
18 pages, plain LATEX, to appear in Physical Review E
References in corpus (3)
Cited by in corpus (6)
- An entanglement-area law for general bosonic harmonic lattice systems
- Rayleigh-Plateau and Gregory-Laflamme instabilities of black strings
- Equilibrium configurations of fluids and their stability in higher dimensions
- Fluid/Gravity Correspondence For General Non-rotating Black Holes
- A Liquid Model Analogue for Black Hole Thermodynamics
- Large Gauge Symmetries of an Asymptotically de Sitter Horizon: An Extended First Law of Thermodynamics