English

Relativistic statistical theory and generalized stosszahlansatz

Statistical Mechanics 2007-05-23 v1 Astrophysics

Abstract

We have investigated the proof of the HH theorem within a manifestly covariant approach by considering the relativistic statistical theory developed in [Phy. Rev. E {\bf 66}, 056125, 2002; {\it ibid.} {\bf 72}, 036108 2005]. In our analysis, however, we have not considered the so-called deformed mathematics as did in the above reference. As it happens in the nonrelativistic limit, the molecular chaos hypothesis is slightly extended within the κ\kappa-formalism, and the second law of thermodynamics implies that the κ\kappa parameter lies on the interval [-1,1]. It is shown that the collisional equilibrium states (null entropy source term) are described by a κ\kappa power law generalization of the exponential Juttner distribution, e.g., f(x,p)(1+κ2θ2+κθ)1/κexpκθf(x,p)\propto (\sqrt{1+ \kappa^2\theta^2}+\kappa\theta)^{1/\kappa}\equiv\exp_\kappa\theta, with θ=α(x)+βμpμ\theta=\alpha(x)+\beta_\mu p^\mu, where α(x)\alpha(x) is a scalar, βμ\beta_\mu is a four-vector, and pμp^\mu is the four-momentum. As a simple example, we calculate the relativistic κ\kappa power law for a dilute charged gas under the action of an electromagnetic field FμνF^{\mu\nu}. All standard results are readly recovered in the particular limit κ0\kappa\to 0.

Keywords

Cite

@article{arxiv.cond-mat/0603177,
  title  = {Relativistic statistical theory and generalized stosszahlansatz},
  author = {R. Silva},
  journal= {arXiv preprint arXiv:cond-mat/0603177},
  year   = {2007}
}

Comments

10 pages, no figures, standard LaTeX file