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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Neutrino interaction model uncertainties from nuclear physics details remain a dominant systematic in oscillation analyses and will require improved modeling plus near-detector constraints to reach the precision goals of next-generation experiments.
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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.