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.
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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.