05 October 2023

Webinar Marco Edoardo Rosti

Marco Edoardo Rosti is an Assistant Professor at the Okinawa Institute of Science and Technology (OIST), Japan, since 2020. He received a Master in Aeronautical Engineering from Politecnico di Milano in 2013, and PhD in Aeronautical Engineering at City, University of London in 2016. Before joining OIST, he spent time as postdoctoral fellow at the KTH Royal Institute of Technology, Sweden, and at the University of Tokyo, Japan. Marco's research interests are in the general area of multiphase turbulence and complex fluids. He was the recipient of the RYUMON Award for distinguished young researcher in fluid mechanics, by the Japanese Society of Fluid Mechanics in 2021, and he is associate editor of the European Journal of Mechanics/B and Editor of Results in Engineering.
Polymeric turbulence

Turbulent flows containing modest amounts of long-chained polymers have remained an intriguing area of research since the discovery of turbulent drag reduction. Here, we perform direct numerical simulations of statistically stationary, homogeneous, and isotropic turbulent flows of dilute solutions of polymers at various Reynolds and Deborah numbers.
At large Reynolds number, we present evidence that there is a range of scales r over which the energy spectra and the structure functions show new scaling consistent with recent experimental results. In particular, we find that for small wavenumbers k, the kinetic energy spectrum shows Kolmogorov–like behavior which crosses over at a larger k to a novel, elastic scaling regime, E(k)~k^(−ξ), with ξ≈2.3. We uncover the mechanism of the elastic scaling by studying the contribution of the polymers to the flux of kinetic energy through scales, and show that this elastic behaviour is non-monotonic in the Deborah number.
At low Reynolds number, our simulations show that elastic turbulence, though a low Reynolds number phenomenon, has more in common with classical, Newtonian turbulence than previously thought. In particular, we find power-law spectra for kinetic energy E(k)∼k^(−4), independent of the Deborah number. In real space, as expected, the velocity field is smooth, but, crucially, with a non-trivial sub-leading contribution. Interestingly, the results show clear evidence of intermittency and multifractality.

05 October 2023, 13h3014h30
Visio-conférence (please ask F. Romano for the link)