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dc.contributor.authorMellado González, Juan Pedro
dc.contributor.authorSarkar, Sutanu
dc.contributor.authorZhou, Ye
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Física
dc.date.accessioned2020-06-15T10:41:14Z
dc.date.available2020-06-15T10:41:14Z
dc.date.issued2005-07-13
dc.identifier.citationMellado, J. P.; Sarkar, S.; Zhou, Y. Large-eddy simulation of Rayleigh-Taylor turbulence with compressible miscible fluids. "Physics of fluids", 13 Juliol 2005, vol. 17, núm. 076101, p. 1-20.
dc.identifier.issn1070-6631
dc.identifier.urihttp://hdl.handle.net/2117/190715
dc.description.abstractTurbulence developed from Rayleigh-Taylor instability between two compressible miscible fluids in an unbounded domain is addressed in this paper. It is demonstrated that the turbulent Mach number in the turbulent core has an upper bound, independent of the density ratio under a broad range of initial mean configurations. The initial thermodynamic state of the system determines the amount of potential energy per unit mass involved in the turbulent mixing stage, and thus the characteristic level of turbulent fluctuations that is achievable is linked to the characteristic speed of sound such that the turbulent Mach number is limited. For the particular case of an ideal gas, this bound on the turbulent Mach number is found to be between 0.25 and 0.6, depending on the particular initial thermodynamic state. Hence, intrinsic compressibility effects those owing to large Mach number are likely to be limited in the turbulent stage of a pure Rayleigh-Taylor problem. This result is confirmed by large-eddy simulations LES of systems with density jumps at the interface of 3: 1, a density ratio for which there is extensive data available in the literature. The LES predictions of the mixing depth growth and overall mixing agree with results previously obtained in incompressible configurations with a negligibly small Mach number, and the data fully describing the Reynolds stresses and the budget of the resolved turbulent kinetic energy equation are provided.
dc.format.extent20 p.
dc.language.isoeng
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Spain
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subjectÀrees temàtiques de la UPC::Física
dc.subject.lcshEddies--Mathematical models
dc.subject.lcshTurbulence--Mathematical models
dc.subject.lcshFluid dynamics
dc.subject.lcshMach number
dc.subject.otherTurbulence
dc.subject.otherLarge-eddy simulations
dc.titleLarge-eddy simulation of Rayleigh-Taylor turbulence with compressible miscible fluids
dc.typeArticle
dc.subject.lemacCapa límit (Meteorologia)
dc.subject.lemacDinàmica de fluids
dc.identifier.doi10.1063/1.1965130
dc.description.peerreviewedPeer Reviewed
dc.relation.publisherversionhttps://aip.scitation.org/doi/10.1063/1.1965130
dc.rights.accessOpen Access
local.identifier.drac27658418
dc.description.versionPostprint (published version)
local.citation.authorMellado, J. P.; Sarkar, S.; Zhou, Y.
local.citation.publicationNamePhysics of fluids
local.citation.volume17
local.citation.number076101
local.citation.startingPage1
local.citation.endingPage20


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