Nonextensivity and the power-law distributions for the systems with self-gravitating long-range interactions
Jiulin Du

TL;DR
This paper explores how nonextensive statistical mechanics explains power-law distributions in self-gravitating systems, linking the nonextensive parameter to observable properties and deriving equations for density profiles.
Contribution
It introduces a nonextensive kinetic framework for self-gravitating systems, establishing a relation between the nonextensive parameter q and physical observables, and deriving equations for density distributions.
Findings
Power-law distributions describe long-range interactions and correlations.
The nonextensive parameter q is linked to velocity dispersion and density.
Derived equations accurately model dark matter density profiles.
Abstract
By a natural nonextensive generalization of the conservation of energy in the q-kinetic theory, we study the nonextensivity and the power-law distributions for the many-body systems with the self-gravitating long-range interactions. It is shown that the power-law distributions describe the long-range nature of the interactions and the non-local correlations within the self-gravitating system with the inhomogeneous velocity dispersion. A relation is established between the nonextensive parameter q and the measurable quantities of the self-gravitating system: the velocity dispersion and the mass density. Correspondingly, the nonextensive parameter q can be uniquely determined from the microscopic dynamical equation and thus the physical interpretation of q different from unity can be clearly presented. We derive a nonlinear differential equation for the radial density dependence of the…
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