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.
Kovtun, Journal of High Energy Physics10, 034 (2019)
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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.