Fluctuation relations for a driven Brownian particle

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dc.creatorImparato, A.
dc.creatorPeliti, L.
dc.date2006-03-20
dc.date2006-06-01
dc.date.accessioned2026-07-07T07:04:49Z
dc.date.available2026-07-07T07:04:49Z
dc.descriptionWe consider a driven Brownian particle, subject to both conservative and non-conservative applied forces, whose probability evolves according to the Kramers equation. We derive a general fluctuation relation, expressing the ratio of the probability of a given Brownian path in phase space with that of the time-reversed path, in terms of the entropy flux to the heat reservoir. This fluctuation relation implies those of Seifert, Jarzynski and Gallavotti-Cohen in different special cases.
dc.identifierhttps://arxiv.org/abs/cond-mat/0603506
dc.identifierhttp://arxiv.org/abs/cond-mat/0603506
dc.identifierPHYS. REV. E 74, 026106 (2006).
dc.identifierdoi:10.1103/PhysRevE.74.026106
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/109462
dc.subjectStatistical Mechanics
dc.subjectOther Condensed Matter
dc.titleFluctuation relations for a driven Brownian particle
dc.typetext

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