Gibbsian Theory of Power-Law Distributions

R. A. Treumann and C. H. Jaroschek
Phys. Rev. Lett. 100, 155005 – Published 18 April 2008; Erratum Phys. Rev. Lett. 102, 089902 (2009)

Abstract

It is shown that power-law phase space distributions describe marginally stable Gibbsian equilibria far from thermal equilibrium, which are expected to occur in collisionless plasmas containing fully developed quasistationary turbulence. Gibbsian theory is extended on the fundamental level to statistically dependent subsystems introducing an “ordering parameter“ κ. Particular forms for the entropy and partition functions are derived with superadditive (nonextensive) entropy, and a redefinition of temperature in such systems is given.

  • Received 25 October 2007

DOI:https://doi.org/10.1103/PhysRevLett.100.155005

©2008 American Physical Society

Erratum

Erratum: Gibbsian Theory of Power-Law Distributions [Phys. Rev. Lett. 100, 155005 (2008)]

R. A. Treumann and C. H. Jaroschek
Phys. Rev. Lett. 102, 089902 (2009)

Authors & Affiliations

R. A. Treumann1,2,* and C. H. Jaroschek3,†

  • 1Department of Geophysics and Environmental Sciences, Munich University, D-80333 Munich, Germany
  • 2Department of Physics, Dartmouth College, Hanover, New Hampshire 03755, USA
  • 3Department Earth & Planetary Science, University of Tokyo, Tokyo, Japan

  • *Visiting the Technical University of Braunschweig, Braunschweig, Germany.
  • treumann@issibern.ch

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Issue

Vol. 100, Iss. 15 — 18 April 2008

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