Viscosity of a classical gas: The rare-collision versus the frequent-collision regime

Abstract

The shear viscosity $\eta$ for a dilute classical gas of hard-sphere particles is calculated by solving the Boltzmann kinetic equation in terms of the weakly absorbed plane waves. For the rare-collision regime, the viscosity $\eta$ as a function of the equilibrium gas parameters -- temperature $T$, particle number density $n$, particle mass $m$, and hard-core particle diameter $d$ -- is quite different from that of the frequent-collision regime, e.g., from the well-known result of Chapman and Enskog. An important property of the rare-collision regime is the dependence of $\eta$ on the external ("non-equilibrium") parameter $\omega$, frequency of the sound plane wave, that is absent in the frequent-collision regime at leading order of the corresponding perturbation expansion. A transition from the frequent to the rare-collision regime takes place when the dimensionless parameter $n{d}^2(T/m{)}^{1/2}{\omega }^{-1}$ goes to zero.

7 pages, 1 figure

References in corpus (3)

• Quasi-Particle Theory of Shear and Bulk Viscosities of Hadronic Matter
• Van der Waals Equation of State with Fermi Statistics for Nuclear Matter
• Shear viscosity of nuclear matter

Cited by in corpus (3)

• Hydrodynamics of the electronic Fermi liquid: a pedagogical overview
• Nucleon matter equation of state, particle number fluctuations, and shear viscosity within UrQMD box calculations
• Ultrasonic waves in classical gases