Bulk Viscosity of Interacting Hadrons
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We show that first approximations to the bulk viscosity $\eta_v$ are expressible in terms of factors that depend on the sound speed $v_s$, the enthalpy, and the interaction (elastic and inelastic) cross section. The explicit dependence of $\eta_v$ on the factor $(\frac 13 - v_s^2)$ is demonstrated in the Chapman-Enskog approximation as well as the variational and relaxation time approaches. The interesting feature of bulk viscosity is that the dominant contributions at a given temperature arise from particles which are neither extremely nonrelativistic nor extremely relativistic. Numerical results for a model binary mixture are reported.
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Bulk viscosity of a binary mixture: the role of the intra-species interaction
Derives second-order Chapman-Enskog bulk viscosity for binary mixtures showing improved physical properties and agreement with Green-Kubo.
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