Anomalous velocity distributions in inelastic Maxwell gases
R. Brito, M. H. Ernst

TL;DR
This review investigates how inelastic collisions affect the velocity distribution in Maxwell gases, revealing overpopulated high-energy tails with algebraic or stretched Gaussian forms in different cooling regimes.
Contribution
It demonstrates the existence of scaling solutions for velocity distributions in inelastic Maxwell gases and characterizes their high-energy tail behaviors.
Findings
High-energy tails are overpopulated compared to Maxwellian distributions.
Algebraic tails in freely cooling systems depend on inelasticity.
Stretched Gaussian tails appear in forced systems.
Abstract
This review is a kinetic theory study investigating the effects of inelasticity on the structure of the non-equilibrium states, in particular on the behavior of the velocity distribution in the high energy tails. Starting point is the nonlinear Boltzmann equation for spatially homogeneous systems, which supposedly describes the behavior of the velocity distribution function in dissipative systems as long as the system remains in the homogeneous cooling state, i.e. on relatively short time scales before the clustering and similar instabilities start to create spatial inhomogeneities. This is done for the two most common models for dissipative systems, i.e. inelastic hard spheres and inelastic Maxwell particles. In systems of Maxwell particles the collision frequency is independent of the relative velocity of the colliding particles, and in hard sphere systems it is linear. We then…
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Taxonomy
TopicsGranular flow and fluidized beds · High-pressure geophysics and materials · Earthquake Detection and Analysis
