Thermodynamic stability of superflows in General Relativity and Newtonian gravity

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1. Verfasser: Gavassino, Lorenzo
Format: Preprint
Veröffentlicht: 2025
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author Gavassino, Lorenzo
author_facet Gavassino, Lorenzo
contents 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.
format Preprint
id arxiv_https___arxiv_org_abs_2507_19985
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Thermodynamic stability of superflows in General Relativity and Newtonian gravity
Gavassino, Lorenzo
General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
Statistical Mechanics
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.
title Thermodynamic stability of superflows in General Relativity and Newtonian gravity
topic General Relativity and Quantum Cosmology
High Energy Astrophysical Phenomena
Statistical Mechanics
url https://arxiv.org/abs/2507.19985