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Rayleigh--Taylor turbulence in two dimensions

Antonio Celani·Andrea Mazzino·Lara Vozella
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Abstract

The first consistent phenomenological theory for two and three dimensional Rayleigh--Taylor (RT) turbulence has recently been presented by Chertkov [Phys. Rev. Lett. {\bf 91} 115001 (2003)]. By means of direct numerical simulations we confirm the spatio/temporal prediction of the theory in two dimensions and explore the breakdown of the phenomenological description due to intermittency effects. We show that small-scale statistics of velocity and temperature follow Bolgiano-Obukhov scaling. At the level of global observables we show that the time-dependent Nusselt and Reynolds numbers scale as the square root of the Rayleigh number. These results point to the conclusion that Rayleigh-Taylor turbulence in two and three dimensions, thanks to the absence of boundaries, provides a natural physical realization of the Kraichnan scaling regime hitherto associated with the elusive ``ultimate state of thermal convection''.

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Antonio Celani, Andrea Mazzino, Lara Vozella. 2006-04-28. Rayleigh--Taylor turbulence in two dimensions. https://doi.org/10.1103/physrevlett.96.134504

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