Transcript
Page 1: Vortex instability and the onset of superfluid turbulence

Vortex instability and the onset of superfluid turbulenceN.B. Kopnin

Low Temperature Lab., HUT, Finland,L.D. Landau Institute for Theoretical Physics, Moscow.

Collaboration

Experiment: M. Krusius, V. Eltsov, A. Finne, HUTL. Skrbek, Charles University, Prague

Theory:T. Araki, M. Tsubota, Osaka University G. Volovik, HUT

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Contents

New class of superfluid turbulence.

Experiment in superfluid He 3 B: Onset independent of the Reynolds number

(Res is the ratio of superflow and the Feynman critical velocity)

Theoretical model for vortex instability

•Results of numerical simulations

•Mutual-friction controlled onset of turbulence

Normal fluid Superfluid

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Superfluid turbulence. Results.[ Finne et al., Nature 424, 1022 (2002)]

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Forces on vortices

• Magnus force

• Force from the normal component

Mutual friction parameters d, d’

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Force balance

couples the velocities:

Hall and Vinen mutual friction parameters

Mutual friction force on the superfluid

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Mutual friction parameters in He-3 B.

Microscopic theory [Rep. Prog. Phys (2002)]

Mutual friction parameters

Distance between the CdGM states

Effective relaxation time

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Mutual friction parameters in He-3 B.

Experiment [Hook, Hall, et al. (1997)]

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Numerical simulations Vortex evolution is integrated from [Schwartz 1988]

The local superflow: all the Biot—Savart contributions

Boundary conditions: Image vortices

Vortex interconnections for crossing vortices

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Numerical results: High temperatures, high friction

Parameters• Rotation velocity rad/s

• Superfluid “Reynolds number”

• Temperature and the MF ratio

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Numerical results: Low temperatures, low friction

Rotation velocity and the Reynolds number

Temperature and the MF ratio

Evolution time

Enormous multiplication of vortices !

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Numerical simulations of vortex evolution in a rotating container

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Model for the onset of turbulence

Distinguish two regions Multiplication region: • high flow velocity, high density of

entangled vortex loops, • vortex crossings and interconnections Rest of the liquid (bulk): • low flow velocity, polarized vortex

linesCompetition between vortex

multiplication and their extraction into the bulk

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Multiplication region

• Loop size l

• 3D vortex density n~l

• 2D (vortex line) density L=nl=l

Multiplication due to collisions and reconnections

Extraction due to inflation

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Total vortex evolution

MF parameters

Superflow velocity

The counterflow velocityThe self-induced velocity

Finally,

Similarly to the Vinen equation (1957)

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Another approach: Vorticity equationNavier—Stokes equation

Vorticity equation

In superfluids: mutual friction force instead of viscosity

Superfluid vorticity equation

Averaged over random vortex loops assuming

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Vortex instabilityEvolution equation

Two regimes of evolution:

Low temperatures,

Solution saturates at

Instability towards turbulent vortex tangle

Higher temperatures,

No multiplication of vortices

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Summary:Superfluid turbulence in other

systems He-3 A: High vortex friction; q>>1 except for very low

temperatures T<<Tc .

No turbulence. Superconductors: High vortex friction; q>>1 except for

very clean materials, l>>(EF /Tc) , and low temperatures.

No turbulence. Superfluid He II: Low vortex friction: q<<1 except for

temperatures very close to T .

Unstable towards turbulence.


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