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Quantum Turbulence in Superfluid 3 He-B at Ultra Low Temperatures. D.I.Bradley D.O.Clubb S.N.Fisher A.M.Guenault A.J.Hale R.P.Haley M.R.Lowe C.Mathhews.

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Presentation on theme: "Quantum Turbulence in Superfluid 3 He-B at Ultra Low Temperatures. D.I.Bradley D.O.Clubb S.N.Fisher A.M.Guenault A.J.Hale R.P.Haley M.R.Lowe C.Mathhews."— Presentation transcript:

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2 Quantum Turbulence in Superfluid 3 He-B at Ultra Low Temperatures. D.I.Bradley D.O.Clubb S.N.Fisher A.M.Guenault A.J.Hale R.P.Haley M.R.Lowe C.Mathhews Introduction Vibrating Wires in superfluid 3He-B Observation of Turbulence The Spatial Extent of Turbulence Direct measurements of Andreev scattering from Turbulence Grid Turbulence G.R.Pickett R.Rahm K.Zaki I.E.Miller M.G.Ward

3 3 He Phase Diagram Superfluid phases formed by Cooper pairs with S=1, L=1

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5 Vortices in the B-phase Formed by a 2  phase shift around the core superfluid flows around core with velocity, v S =  /2  r vortices are singly quantised with circulation :  =h/2m 3 Superfluid is distorted in the core, core size depends on pressure:  0 ~ 65nm to 15nm

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14 Decrease in damping at higher temperatures implies that the damping from thermal quasiparticles is reduced. i.e. thermal quasiparticles are prevented from scattering with the detector wire.

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18 Quasiholes propagate through flow field

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21 Quasiparticles Andreev Scattered into Quasiholes with very small momentum transfer

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24 Fraction of flux Reflected =0.5*[1-exp(-p F v(r)/k B T)] v(r)=  /2  r,  =h/2m 3 Shadow half Width = p F  /2  k B Tln2 ~8  m @ 100  K (vortex core size  0 ~ 65nm @low P)

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31 Flow barrier independent of temperature below.22T c

32 Flow barrier decreases above.22T c

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41 The heat input to the radiator (applied heat and heat leak) is balanced by a beam of ballistic quasiparticle excitations emitted from the radiator orifice.

42 In the presence of vortices, the change in width parameter is proportional to the fraction of excitations Andreev reflected.

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44 Take a thin slab of homogeneous vortex tangle of unit area, line density L and thickness  x Probability of qp passing within distance r of a vortex core is L  x r Mean qp energy =k B T Qps are Andreev scattered if p F v(r)> k B T v(r)=  2  r, so qps scattered if they approach within a distance, r ~  p F /2  k B T Simple Estimate of vortex Line Density Fraction of qps Andreev scattered after traveling  x through tangle, L  x  p F /2  k B T Total fraction transmitted through tangle of thickness x is exp(-x/ ), ~  2  k B T / L  p F

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46 Decay time of vortex tangle From Simulations by C.F.Barenghi and D.C.Samuels, PRL 89 155302 (2002) Tangle disperses by evaporating small rings of size R~L -1/2 Rings form after a time  ~1/(L  ) [~0.3s for our line densities] The tangle then expands at the self induced velocity of the rings, v R Time scale for tangle to disperse ~ S 0 / v R ~5s for our line densities VWR measurements show the tangle disperses in ~ 3-4s

47 Grid Mesh: 11  m rectangular wires, 40  m square holes.

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70 Summary Turbulence in 3 He-B Generated by VWRs: Generated above pair-breaking critical velocity v C =v L /3 ~ 9mm/s @ P=0 Spatial extent ~2mm Line densities up to ~5 x 10 7 m -2, line spacing ~ 150  m Disperses on a time scale of a few seconds, explained by ‘ring evaporation’ Turbulence in 3 He-B Generated by a Vibrating Grid: Generated above a velocity ~ 1mm/s Estimated Spatial extent ~2mm Estimated Line densities up to ~5x10 8 m -2, line spacing ~ 50  m Disperses on a time scale of: seconds above ~4mm/s <0.1s at lower velocities (sharp cross-over at 3.5 mm/s) - Possible explanation: The Grid is only generating fast propagating vortex rings at low velocities which become turbulent at high velocities.


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