The bound on viscosity and the generalized second law of thermodynamics
Itzhak Fouxon, Gerold Betschart, Jacob D. Bekenstein
TL;DR
The paper shows that treating a fluid as an ideal continuum leads to a paradox when slow accretion onto a black hole appears to violate the generalized second law (GSL). By incorporating a finite correlation length, it derives a lower bound on this length from a universal entropy bound and, subsequently, a lower bound on viscosity relative to entropy density that scales with the sound speed. This framework naturally connects to the Kovtun–Son–Starinets (KSS) bound and suggests that the GSL underpins a fundamental limit on fluid dissipation in strongly coupled systems, including the quark–gluon plasma. Overall, the GSL provides a unifying, macroscopic principle that links microscopic structure to transport properties and offers insight into the origin of viscosity bounds for fluids.
Abstract
We describe a new paradox for ideal fluids. It arises in the accretion of an \textit{ideal} fluid onto a black hole, where, under suitable boundary conditions, the flow can violate the generalized second law of thermodynamics. The paradox indicates that there is in fact a lower bound to the correlation length of any \textit{real} fluid, the value of which is determined by the thermodynamic properties of that fluid. We observe that the universal bound on entropy, itself suggested by the generalized second law, puts a lower bound on the correlation length of any fluid in terms of its specific entropy. With the help of a new, efficient estimate for the viscosity of liquids, we argue that this also means that viscosity is bounded from below in a way reminiscent of the conjectured Kovtun-Son-Starinets lower bound on the ratio of viscosity to entropy density. We conclude that much light may be shed on the Kovtun-Son-Starinets bound by suitable arguments based on the generalized second law.
