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dc.creatorBrey Abalo, José Javieres
dc.creatorRuiz Montero, María Josées
dc.creatorMoreno Franco, Franciscoes
dc.date.accessioned2020-05-26T11:40:15Z
dc.date.available2020-05-26T11:40:15Z
dc.date.issued2004
dc.identifier.citationBrey Abalo, J.J., Ruiz Montero, M.J. y Moreno Franco, F. (2004). Steady-state representation of the homogeneous cooling state of a granular gas. Physical Review E, 69 (5), 051303-1-051303-13.
dc.identifier.issn1550-2376es
dc.identifier.urihttps://hdl.handle.net/11441/97154
dc.description.abstractThe properties of a dilute granular gas in the homogeneous cooling state are mapped to those of a stationary state by means of a change in the time scale that does not involve any internal property of the system. The new representation is closely related with a general property of the granular temperature in the long time limit. The physical and practical implications of the mapping are discussed. In particular, simulation results obtained by the direct simulation Monte Carlo method applied to the scaled dynamics are reported. This includes ensemble averages and also the velocity autocorrelation function, as well as the self-diffusion coefficient obtained from the latter by means of the Green-Kubo representation. In all cases, the obtained results are compared with theoretical predictions.es
dc.formatapplication/pdfes
dc.format.extent13 p.es
dc.language.isoenges
dc.publisherAmerican Physical Societyes
dc.relation.ispartofPhysical Review E, 69 (5), 051303-1-051303-13.
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 Internacional*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.titleSteady-state representation of the homogeneous cooling state of a granular gases
dc.typeinfo:eu-repo/semantics/articlees
dcterms.identifierhttps://ror.org/03yxnpp24
dc.type.versioninfo:eu-repo/semantics/publishedVersiones
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses
dc.contributor.affiliationUniversidad de Sevilla. Departamento de Física Atómica, Molecular y Nucleares
dc.relation.publisherversionhttps://doi.org/10.1103/PhysRevE.69.051303es
dc.identifier.doi10.1103/PhysRevE.69.051303es
dc.journaltitlePhysical Review Ees
dc.publication.volumen69es
dc.publication.issue5es
dc.publication.initialPage051303-1es
dc.publication.endPage051303-13es

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