Proves future global stability and explicit decay rates for small perturbations of Maxwell-Jüttner equilibria (and vacuum for q > 1/3) of the massless Boltzmann equation on FLRW backgrounds with scale factor t^q, q in [0,1].
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General constitutive equations for relativistic fluids are obtained by extending the projection method in the Chapman-Enskog expansion to arbitrary frames and representations, coupling dissipative fluxes to all derivatives of state variables including weak electromagnetic fields.
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First-order general constitutive equations for relativistic fluids using the projection method in the Chapman-Enskog expansion of the Boltzmann equation
General constitutive equations for relativistic fluids are obtained by extending the projection method in the Chapman-Enskog expansion to arbitrary frames and representations, coupling dissipative fluxes to all derivatives of state variables including weak electromagnetic fields.