Gibbsian theory of power law distributions

dc.creatorTreumann, R. A.
dc.creatorJaroschek, C. H.
dc.date2007-11-11
dc.date2008-02-08
dc.date.accessioned2026-07-07T09:33:36Z
dc.date.available2026-07-07T09:33:36Z
dc.descriptionIt 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 quasi-stationary 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 super-additive (non-extensive) entropy, and a redefinition of temperature in such systems is given.
dc.descriptionPhysical Review Letters revised second revision (and shortened because of overlength) co-author added
dc.identifierhttps://arxiv.org/abs/0711.1676
dc.identifierhttp://arxiv.org/abs/0711.1676
dc.identifierPhysical Review Letters 100, 155005 (2008)
dc.identifierdoi:10.1103/PhysRevLett.100.155005
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/159188
dc.subjectPlasma Physics
dc.titleGibbsian theory of power law distributions
dc.typetext

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