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Fluctuations, correlations, and Casimir-like forces in the homogeneous cooling state of a granular gas

dc.contributor.authorJiménez Oliva, Jesús David
dc.contributor.authorRodriguez-Lopez, Pablo
dc.contributor.authorKhalil, Nagi
dc.date.accessioned2024-01-23T15:00:06Z
dc.date.available2024-01-23T15:00:06Z
dc.date.issued2024-01-22
dc.identifier.citationPhys. Fluids 36, 013326 (2024); doi: 10.1063/5.0189492es
dc.identifier.issn1089-7666
dc.identifier.urihttps://hdl.handle.net/10115/28739
dc.description.abstractThe fluctuating hydrodynamics by Brey et. al. is analytically solved to get the long-time limit of the fluctuations of the number density, velocity field, and energy density around the homogeneous cooling state of a granular gas, under physical conditions where it keeps stable. Explicit expressions are given for the non-white contributions in the elastic limit. For small dissipation, the latter is shown to be much smaller than the inelastic contributions, in general. The fluctuation-induced Casimir-like forces on the walls of the system are calculated assuming a fluctuating pressure tensor resulting from perturbing its Navier-Stokes expression. This way, the Casimir-like forces emerges as the correlation between the longitudinal velocity and the energy density. Interestingly, the fluctuation-induced forces push/pull the system towards the square or rectangular geometry when they vanish, in good agreement with the event-driven numerical simulations.es
dc.publisherAIPes
dc.rightsAtribución-NoComercial-CompartirIgual 4.0 Internacional*
dc.subjectStatistical Mechanicses
dc.titleFluctuations, correlations, and Casimir-like forces in the homogeneous cooling state of a granular gases
dc.typeinfo:eu-repo/semantics/articlees
dc.identifier.doi10.1063/5.0189492es
dc.rights.accessRightsinfo:eu-repo/semantics/embargoedAccesses


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