Relativistic Brownian Motion

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dc.creatorOron, O.
dc.creatorHorwitz, L. P.
dc.date2002-12-08
dc.date2003-01-12
dc.date.accessioned2026-07-07T06:23:20Z
dc.date.available2026-07-07T06:23:20Z
dc.descriptionWe solve the problem of formulating Brownian motion in a relativistically covariant framework in 1+1 and 3+1 dimensions. We obtain covariant Fokker-Planck equations with (for the isotropic case) a differential operator of invariant d'Alembert form. Treating the spacelike and timelike fluctuations separately, we show that it is essential to take into account the analytic continuation of "unphysical" fluctuations in order to achieve these results.
dc.descriptionPlain TeX, 10 pages
dc.identifierhttps://arxiv.org/abs/physics/0212036
dc.identifierhttp://arxiv.org/abs/physics/0212036
dc.identifierRel.Grav.Cosmol. 1 (2004) 109-122
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/96194
dc.subjectClassical Physics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Physics
dc.titleRelativistic Brownian Motion
dc.typetext

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