Relativistic Brownian Motion in 3+1 Dimensions

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dc.creatorOron, O.
dc.creatorHorwitz, L. P.
dc.date2003-11-30
dc.date.accessioned2026-07-07T04:30:47Z
dc.date.available2026-07-07T04:30:47Z
dc.descriptionWe solve the problem of formulating Brownian motion in a relativistically covariant framework in 3+1 dimensions. We obtain covariant Fokker-Planck equations with (for the isotropic case) a differential operator of d'Alembert form. Treating the spacelike and timelike fluctuations separately in order to maintain the covariance property, we show that it is essential to take into account the analytic continuation of "unphysical" fluctuations. We discuss the notion of locality in this framework and possible implications for entangled states.
dc.description19 pages Latex, one figure ps
dc.identifierhttps://arxiv.org/abs/math-ph/0312003
dc.identifierhttp://arxiv.org/abs/math-ph/0312003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/57584
dc.subjectMathematical Physics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectProbability
dc.subjectQuantum Physics
dc.titleRelativistic Brownian Motion in 3+1 Dimensions
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