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How far from equilibrium is active matter?

dc.creatorFodor, Etienne Paul
dc.creatorNardini, Cesare
dc.creatorCates, Michael Elmhirst
dc.creatorTailleur, Julien
dc.creatorVisco, Paolo
dc.creatorvan, Wijland Frédéric
dc.date.accessioned2016-06-09
dc.date.accessioned2018-11-24T23:19:03Z
dc.date.available2016-07-07T15:48:11Z
dc.date.available2018-11-24T23:19:03Z
dc.date.issued2016
dc.identifierhttps://www.repository.cam.ac.uk/handle/1810/256677
dc.identifier.urihttp://repository.aust.edu.ng/xmlui/handle/123456789/3398
dc.description.abstractActive matter systems are driven out of thermal equilibrium by a lack of generalized Stokes-Einstein relation between injection and dissipation of energy at the microscopic scale. We consider such a system of interacting particles, propelled by persistent noises, and show that, at small but finite persistence time, their dynamics still satisfy a time-reversal symmetry. To do so, we compute perturbatively their steady-state measure and show that, for short persistent times, the entropy production rate vanishes. This endows such systems with an effective Fluctuation-Dissipation theorem akin to that of thermal equilibrium systems. Last we show how interacting particle systems with viscous drags and correlated noises can be seen as in equilibrium with a visco-elastic bath but driven out of equilibrium by non-conservative forces, hence providing an energetic insight on the departure of active systems from equilibrium.
dc.languageen
dc.publisherAmerican Physical Society
dc.publisherPhysical Review Letters
dc.rightshttp://creativecommons.org/licenses/by-nc/4.0/
dc.rightsAttribution-NonCommercial 4.0 International
dc.titleHow far from equilibrium is active matter?
dc.typeArticle


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