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.
1 − τ ′ τ 2# ˆS (B16) Using this we can write e− log ( τ τ ′ )[(2l+1)ˆI−(2l−n)ˆS] = e− log ( τ τ ′ )(2l+1)ˆIe − (2l−n) 2 1− τ ′ τ 2 ˆS = τ ′ τ 2l+1 ∞X k=0
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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.