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• W3100834934 abstract "We conduct direct numerical simulations (DNS) of the Cahn–Hilliard–Navier–Stokes (CHNS) equations to investigate the statistical properties of a turbulent phase-separating symmetric binary-fluid mixture. Turbulence causes an arrest of the phase separation which leads to the formation of a statistically steady emulsion. We characterise turbulent velocity fluctuations in an emulsion for different values of the Reynolds number and the Weber number. Our scale-by-scale kinetic energy budget analysis shows that the interfacial terms in the CHNS equations provide an alternative route for the kinetic energy transfer. By studying the probability distribution function (p.d.f.) of the energy dissipation rate, the vorticity magnitude and the joint-p.d.f. of the velocity-gradient invariants we show that the statistics of the turbulent fluctuations do not change with the Weber number." @default.
• W3100834934 created "2020-11-23" @default.
• W3100834934 creator A5077737460 @default.
• W3100834934 date "2019-06-24" @default.
• W3100834934 modified "2023-10-16" @default.
• W3100834934 title "Kinetic energy spectra and flux in turbulent phase-separating symmetric binary-fluid mixtures" @default.
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• W3100834934 doi "https://doi.org/10.1017/jfm.2019.425" @default.
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