This analysis reveals how bulk viscosity relates to hydrodynamics in n-component fluids, indicating the effects of chemical potentials.
Understanding the hydrodynamics of out-of-equilibrium dense viscous fluids is of key importance to accurate descriptions of physical systems such as compact stars, particularly their mergers. We consider a near-equilibrium relativistic fluid with n independent and small chemical potentials restoring the system back towards equilibrium. By diagonalising the evolution equation for the out-of-equilibrium chemical potentials, we construct an explicit evolution equation for the bulk scalar of the system in second-order hydrodynamics in terms of equilibrium quantities. We find expressions for the $2n$ transport quantities and show that in the rest frame of the fluid, the system admits a Green's function corresponding to an n-component fluid.
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Saga Säppi (2025) studied this question.
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