The decay mode of high-energy tails in velocity distributions of astrophysical plasma particles

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dc.creatorLiu, Jian-Miin
dc.date2001-12-06
dc.date.accessioned2026-07-07T02:43:45Z
dc.date.available2026-07-07T02:43:45Z
dc.descriptionThe relativistic equilibrium velocity distribution coincides with the Maxwellian distribution for small velocities and vanishes at c, the velocity of light. Based on the decay pattern of high-energy tail in the relativistic equilibrium velocity distribution, it is predicted for velocity and velocity rate distributions of astrophysical plasma particles that they fall off to zero, as velocity goes to c, slower than any exponential decay but faster than any power-law decay.
dc.description4 pages with no figure
dc.identifierhttps://arxiv.org/abs/cond-mat/0112084
dc.identifierhttp://arxiv.org/abs/cond-mat/0112084
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/18619
dc.subjectStatistical Mechanics
dc.subjectAstrophysics
dc.titleThe decay mode of high-energy tails in velocity distributions of astrophysical plasma particles
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