Non-Gaussian velocity distributions Maxwell would understand
J. A. S. Lima, M. H. Benetti

TL;DR
This paper presents a pedagogical approach to derive non-Gaussian power-law velocity distributions in gases, extending Maxwell's classical method and clarifying their relation to Tsallis entropy without requiring long-range interactions.
Contribution
It introduces a bottom-up derivation of non-Gaussian velocity distributions, providing new insights into their origin and relation to classical thermodynamics.
Findings
Derivation of power-law velocity distributions from Maxwell's approach.
Clarification that non-Gaussian distributions do not necessarily imply long-range interactions.
Insights into the zeroth law of thermodynamics in non-Gaussian contexts.
Abstract
In 1988, Constantino Tsallis proposed an extension of the Boltzmann statistical mechanics by postulating a new entropy formula, , where is the number of microstates accessible to the system, and defines a deformation of the logarithmic function. This ``top-down" , approach recovers the celebrated Boltzmann entropy in the limit since . However, for the entropy is non-additive and has been successfully applied for a variety of phenomena ranging from plasma physics to cosmology. For a system of particles, Tsallis' formula predicts a large class of power-law velocity distributions reducing to the Maxwellian result only for a particular case. Here a more pedagogical ``bottom-up" path is adopted. We show that a large set of power-law distributions for an ideal gas in equilibrium at temperature T is derived by slightly…
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