Formal solutions of Boltzmann moment equations demonstrate that relativistic hydrodynamics works far from equilibrium because non-perturbative modes and modified transport coefficients enable interpolation between free streaming and hydrodynamic regimes.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
verdicts
UNVERDICTED 2representative citing papers
In the Israel-Stewart relativistic fluid model, fluid modes behave as overdamped oscillators with one decay rate approaching the Kolmogorov K41 value and a second diverging rate as c approaches infinity, supporting two flow patterns including one with an entropy cascade.
citing papers explorer
-
Validity of relativistic hydrodynamics beyond local equilibrium
Formal solutions of Boltzmann moment equations demonstrate that relativistic hydrodynamics works far from equilibrium because non-perturbative modes and modified transport coefficients enable interpolation between free streaming and hydrodynamic regimes.
-
Quantum field approach to relativistic turbulence
In the Israel-Stewart relativistic fluid model, fluid modes behave as overdamped oscillators with one decay rate approaching the Kolmogorov K41 value and a second diverging rate as c approaches infinity, supporting two flow patterns including one with an entropy cascade.