Thermodynamic stability of superflows in General Relativity and Newtonian gravity
arXiv:2507.19985 · doi:10.1088/1361-6382/ae1d0a
Abstract
Landau's criterion for superfluidity is a special case of a broader principle: A moving fluid cannot be stopped by frictional forces if its state of motion is a local minimum of the grand potential. We employ this general thermodynamic criterion to derive a set of inequalities that any superfluid mixture (with an arbitrary number of order parameters) must satisfy for a certain state of motion to be long-lived and unimpeded by friction. These macroscopic constraints complement Landau's original criterion, in that they hold at all temperatures, and remain valid even for gapless superfluids. Unfortunately, they are only necessary conditions for the existence of a frictionless hydrodynamic motion, since they presuppose the validity of a fluid description. However, they do provide sufficient conditions for stability against stochastic hydrodynamic fluctuations. We first formulate our analysis within the framework of General Relativity, and then we take the Newtonian limit.
14 pages, 1 figure, published on CQG (see https://iopscience.iop.org/article/10.1088/1361-6382/ae1d0a)
References in corpus (15)
- Holographic model of superfluidity
- Bulk viscosity of superfluid neutron stars
- Temperature-dependent pulsations of superfluid neutron stars
- Bounds on transport from hydrodynamic stability
- Stability and causality of Carter's multifluid theory
- Universality Classes of Relativistic Fluid Dynamics: Foundations
- Thermodynamic origin of the Landau instability of superfluids
- Superfluid dynamics in neutron star crusts: the Iordanskii force and chemical gauge covariance
- Gapless neutron superfluidity can explain the late time cooling of transiently accreting neutron stars
- Gapless superfluidity in neutron stars: Thermal properties
- Gapless superfluidity in neutron stars: Normal-fluid fraction
- Consistent inclusion of fluctuations in first-order causal and stable relativistic hydrodynamics
- Gapless neutron superfluidity in the crust of the accreting neutron stars KS 1731-260 and MXB 1659-29
- Causal and Stable Superfluid Hydrodynamics
- Exergy of an open continuous medium