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- W1989350150 abstract "A two fluid (the normal fluid and the superfluid) spectral model based on the HVBK equations is used to compute the energy spectra of developed turbulence in superfluid helium (helium II) at different temperatures and different values of mutual friction coefficients, looking for both asymptotic and realistic helium II solutions. An original computational model is proposed, based on the model suggested by L’vov, Nazarenko, and Skrbek [JLTP 145, 125 (2006)] for mutual friction term and an eddy damped quasinormal Markovian closure for the energy flux term. On the one hand, the four asymptotic solutions predicted by theoretical analysis are confirmed. On the other hand, we present results for normal and superfluid energy spectra in realistic cases using experimental values of the mutual friction coefficients corresponding to helium II. Good qualitative agreement in the small scale range is found with the direct numerical simulation results obtained by Roche, Barenghi, and Leveque [Europhys. Lett. 87, 54006 (2009)]." @default.
- W1989350150 created "2016-06-24" @default.
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- W1989350150 date "2010-12-01" @default.
- W1989350150 modified "2023-09-26" @default.
- W1989350150 title "Eddy damped quasinormal Markovian simulations of superfluid turbulence in helium II" @default.
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- W1989350150 doi "https://doi.org/10.1063/1.3527282" @default.
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