English

Relativity, nonextensivity, and extended power law distributions

Statistical Mechanics 2009-11-11 v1 Astrophysics

Abstract

A proof of the relativistic HH-theorem by including nonextensive effects is given. As it happens in the nonrelativistic limit, the molecular chaos hypothesis advanced by Boltzmann does not remain valid, and the second law of thermodynamics combined with a duality transformation implies that the q-parameter lies on the interval [0,2]. It is also proved that the collisional equilibrium states (null entropy source term) are described by the relativistic qq-power law extension of the exponential Juttner distribution which reduces, in the nonrelativistic domain, to the Tsallis power law function. As a simple illustration of the basic approach, we derive the relativistic nonextensive equilibrium distribution for a dilute charged gas under the action of an electromagnetic field FμνF^{{\mu\nu}}. Such results reduce to the standard ones in the extensive limit, thereby showing that the nonextensive entropic framework can be harmonized with the space-time ideas contained in the special relativity theory.

Keywords

Cite

@article{arxiv.cond-mat/0510201,
  title  = {Relativity, nonextensivity, and extended power law distributions},
  author = {R. Silva and J. A. S. Lima},
  journal= {arXiv preprint arXiv:cond-mat/0510201},
  year   = {2009}
}

Comments

Accepted for publication in PRE

R2 v1 2026-07-22T11:23:46.086Z