Symmetries of turbulent state Gregory Falkovich Weizmann Institute of Science Rutgers, May 10, 2009 D. Bernard, A. Celani, G. Boffetta, S. Musacchio.

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Presentation transcript:

Symmetries of turbulent state Gregory Falkovich Weizmann Institute of Science Rutgers, May 10, 2009 D. Bernard, A. Celani, G. Boffetta, S. Musacchio

 L Physics Today 59(4), 43 (2006) Turbulence is a state of a physical system with many degrees of freedom deviated far from equilibrium. It is irregular both in time and in space.

Energy cascade and Kolmogorov scaling

Lack of scale-invariance in direct turbulent cascades

Euler equation in 2d describes transport of vorticity

Family of transport-type equations m=2 Navier-Stokes m=1 Surface quasi-geostrophic model, m=-2 Charney-Hasegawa-Mima model Electrostatic analogy: Coulomb law in d=4-m dimensions

This system describes geodesics on an infinitely-dimensional Riemannian manifold of the area-preserving diffeomorfisms. On a torus,

(*) Add force and dissipation to provide for turbulence lhs of (*) conserves

pumping k Q Kraichnan’s double cascade picture P

Inverse Q-cascade

Small-scale forcing – inverse cascades

Locality + scale invariance → conformal invariance ? Polyakov 1993

_____________ =

perimeter P  Boundary  Frontier  Cut points  Boundary  Frontier  Cut points Bernard, Boffetta, Celani &GF, Nature Physics 2006, PRL2007

Vorticity clusters

Schramm-Loewner Evolution (SLE)

What it has to do with turbulence?

C=ξ(t)

m

Different systems producing SLE Critical phenomena with local Hamiltonians Random walks, non necessarily local Inverse cascades in turbulence Nodal lines of wave functions in chaotic systems Spin glasses Rocky coastlines

Conclusion Inverse cascades seems to be scale invariant. Within experimental accuracy, isolines of advected quantities are conformal invariant (SLE) in turbulent inverse cascades. Why?