Phase transitions and flux-loop metastable states in rotating turbulence
POSTER
Abstract
By using direct numerical simulations of up to a record resolution of 512x512x32768 grid points we discover the existence of a new metastable out-of-equilibrium state in rotating turbulence. We scan the phase space by varying both the rotation rate and the dimensionless aspect ratio, $\lambda=H/L$, where $L$ and $H$ are the sizes of the domain perpendicular and parallel to the direction of rotation, respectively. We show the existence of three turbulent phases. For small $Ro$ but finite $\lambda$, we have a split cascade where the injected energy is transferred to both large and small scales. For large $\lambda$ and finite $Ro$ there is no inverse cascade and the energy is transferred downscale in Fourier space only. Surprisingly, between these two regimes, a third phase is observed as reported here for the first time. Consequently, for certain intervals of $Ro$ and $\lambda$, energy is no longer accumulated at arbitrarily large scales, rather it stops at some characteristic intermediate length-scales from where it is then redistributed forward in Fourier space, leading to a flux-loop mechanism where the flow is out of equilibrium with vanishing net flux, and non-vanishing heterochiral and homochiral sub-fluxes. P. Clark Di Leoni, et al. arXiv preprint arXiv:2002.08784 (2020).
Authors
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Luca Biferale
Department of Physics and INFN, University of Rome Tor Vergata
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Patricio Clark Di Leoni
Department of Mechanical Engineering, Johns Hopkins University, Johns Hopkins University
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Alexandros Alexakis
Laboratoire de Physique de l'Ecole Normale Superieure, CNRS, PSL Research University
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Michele Buzzicotti
Department of Physics and INFN, University of Rome Tor Vergata