Manifestly covariant classical correlation dynamics II. Transport equations and Hakim equilibrium conjecture
arXiv:0905.4796 · doi:10.1002/andp.200910404
Abstract
This is the second of a series of papers on the special relativistic classical statistical mechanics. Employing the general theory developed in the first paper we rigorously derive the relativistic Vlasov, Landau and Boltzmann equation. The latter two advocate the J{ü}ttner distribution as the equilibrium distribution. We thus, at the full microscopic level, provide a support for the recent numerical finding [D. Cubero {\it et. al.}, Phys. Rev. Lett. \textbf{99}, 170601 (2007)] of the special relativistic generalization of the Maxwell-Boltzmann distribution. Furthermore, the present theory allows us to rigorously calculate various correlation functions at the relativistic many-body equilibrium. Therefore, the relativistic many-body equilibrium conjecture of Hakim is justified.
20 pages, 3 figures
References in corpus (9)
- Relativistic Brownian Motion
- Collective cyclotron motion of the relativistic plasma in graphene
- Exact relativistic kinetic theory of an electron beam-plasma system: hierarchy of the competing modes in the system parameter space
- Thermal equilibrium and statistical thermometers in special relativity
- Fokker-Planck type equations for a simple gas and for a semi-relativistic Brownian motion from a relativistic kinetic theory
- Time parameters and Lorentz transformations of relativistic stochastic processes
- Relativistic non-instantaneous action-at-a-distance interactions
- Fokker-Planck-Rosenbluth-Type Equations for Self-gravitating Systems in 1PN Approximation
- Manifestly covariant classical correlation dynamics I. General theory