Velocity distribution of driven granular gases
V. V. Prasad, Dibyendu Das, Sanjib Sabhapandit, and R. Rajesh

TL;DR
This paper derives microscopic models for driven granular gases, revealing two universal velocity distribution regimes: a Gaussian decay with logarithmic corrections for typical driving, and an exponential decay contradicting kinetic theory predictions.
Contribution
It provides the first microscopic derivation of velocity distribution tails in driven granular gases, challenging existing kinetic theory assumptions.
Findings
Velocity distribution is Gaussian with logarithmic corrections under typical driving.
In a less generic regime, the distribution decays exponentially, contradicting kinetic theory.
Microscopic model results necessitate re-examining kinetic theory assumptions.
Abstract
The granular gas is a paradigm for understanding the effects of inelastic interactions in granular materials. Kinetic theory provides a general theoretical framework for describing the granular gas. Its central result is that the tail of the velocity distribution of a driven granular gas is a stretched exponential that, counterintuitively, decays slower than that of the corresponding elastic gas in equilibrium. However, a derivation of this result starting from a microscopic model is lacking. Here, we obtain analytical results for a microscopic model for a granular gas where particles with two-dimensional velocities are driven homogeneously and isotropically by reducing the velocities by a factor and adding a stochastic noise. We find two universal regimes. For generic physically relevant driving, we find that the tail of the velocity distribution is a Gaussian with additional…
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