Turbulence in Superfluid Helium-4 at mK Temperatures · R.J. Donnelly „Quantized Vortices in...
Transcript of Turbulence in Superfluid Helium-4 at mK Temperatures · R.J. Donnelly „Quantized Vortices in...
Turbulence in Superfluid Helium-4 atmK Temperatures
Otaniemi, 16. Nov. 2001
W. Schoepe
Institut für Experimentelle und Angewandte Physik
Universität Regensburg
Contents
1. Why is turbulence in superfluids at T = 0 interesting?
2. Basics of classical turbulence.
3. Basics of superfluid turbulence.
4. Classical character of superfluid turbulence at high vortex densities.
5. Quantum turbulence: our experiment.
6. Conclusion.
Literature:
R.J. Donnelly „Quantized Vortices in Helium II“Cambridge University Press, Cambridge 1991.
Lecture Notes in Physics „Quantized Vortex Dynamics andSuperfluid Turbulence“, Vol. 571, Springer 2001.
Classical turbulence
Navier-Stokes-equation:
( ) Vpgrad1VgradVtV rrrr
∆ν+ρ
−=⋅+∂∂
ρην = kinematic viscosity
air 1,4 · 10-5 m2/swater 10-6
HeI (2,2 K) 1,7 · 10-8
HeII (0K) 0
( ) L/V~VgradV 2rr⋅
VL
LVRe
22
ν⋅≡⇒
2L/V~V ν∆⋅νr
Reynoldszahlν
= VLRe
Example
Sphere in water
RV
L = 2 R = 10-2 m⇒ Re = 6
22
101010−
−− ⋅ = 102
V = 10-2 m/s
Re < 1: laminar flowdrag force 6πηRV (Stokes)
Re > 103: turbulent flowdrag force 22
D VRc21 ρπ
definition 22
DVR
21
forcedragcρπ
=
sphere: cD ≈ 0,4
Kolmogorov’s Law
1V l 2V
3/2221 l|VV| ∝−rr
|21 VV|rr
− can depend only on
=ε 3
2
sm
kgWatt and l (m)
⇒ | 3/121 )l(|VV ε∝−rr
3/23/23/23/2221 kl|VV|E −ε∝ε∝−∝rr
3/2
kkdk)k(FE −∫
∞∝= ⇒
3/5k)k(F −∝
Kolmogorov 1941v. Weizsäcker 1945
Decay of turbulence
>ω<ν=−=ε 2
dtdE , V
rrrot=ω
⇒∝ε⇒∝⇒∝ε −− 322/3 ttEE
2/3t−∝ω
Superfluid turbulence (T = 0)
(4He, BEC)
Equation of motion : nonlinearSchrödinger equation
ψψ+ψ∇−=∂ψ∂ 22
2||V
m2ti hh
Madelung transformation: φ=ψ iae
φ∇=m
v hr
2ma=ρ
0)v(t
=ρ⋅∇+∂ρ∂ r
continuity equation
mVav)v(
tv 2
∇−=∇⋅+∂∂ rrr
Euler equation
no viscosity, no Reynolds number
pure potential flow: 0vrot =r
quantized circulation: ∫ κ=⋅ Nrdv rr , vortices with N = 1
superfluid turbulence = tangle of singly quantized vortices
High vortex densities:
classical character
Examples:
1. rotating superfluid:
imitation of classical solid body rotation
rv rrr ×Ω= ( )Ω=rr 2vrot
by n vortices/area:
Ω==κ 2|vrot|n r
2. Tabeling’s “washing machine”:
Kolmogorov’s law
3. Decay of grid turbulence
Quantum turbulence
L line length density
= 23 m
1mm
κ circulation quantum
−
sm10
27
inter vortex spacing )m(L
1
energy/mass E ~ κ 2L
2
2
sm
dissipated power/mass
κε 3
223
smL~
vorticity
κω
s1L~
quantum turbulence when characteristic length scalel <
L1
41
3l
εκ<
Experimental Setup
• A magnetic microsphere is levitating between two ho-
rizontally arranged superconducting electrodes made of
niobium
• no mechanical suspension elements, horizontal stabi-
lity is provided by trapped flux lines
• the sphere is electrostatically charged by applying a high
dc voltage to the capacitor before cooling below Tc
• space between the electrodes is filled with pure 4He
• excitation of vertical oscillations of the sphere around its
equilibrium levitation position by applying a resonant ac
electric field
• measurement of: velocity amplitude of the oscillatons
• parameters: driving force amplitude / temperature
different regimes
0 200 400 600 8000
10
20
30
40
T = 300 mK
v (m
m/s
)
F (pN)
low driving forces: laminar flow, dissipation is givenby ballistic scattering of phonons
large driving forces: turbulent flow, large dissipati-on similiar to classical flow
intermediate range: state of system is unstable, sy-stem switches intermittently between laminar flowand turbulent flow
turbulent regime
0 2 4 6 8 10 120
20
40
60
80
100
T = 100 mK
v (m
m/s
)
F (nN)
In the turbulent regime a driving force similiar toturbulent flow in classical fluids is observed:
Ft = γ(v2−v20)
using the classic turbulent drag coefficient
γ = CDρπR2/2
with CD ≈ 0.4 for spheres, which describes thesolid line through the data.
Intermittent Switching
18
20
22
24
26
28
30
time (100 s / division)
18
20
22
24
26
28
30
v (m
m/s
)
18
20
22
24
26
28
30
Turbulent Statistics
20 30 40 501
10
100
1000
ba
32 mK 100 mK 200 mK 300 mK 403 mK
µ (s
)F-λvt (pN)
0 10 20 30 40 500.001
0.01
0.1
1
T = 300 mKF = 59 pN
t (s)
P(t
)
Laminar Statistics
0 10 20 30 40 500
1
2
3
4
5
6
7
b
+10%
-10%4.79
28mK 100mK 200mK 300mK 403mK
v w (
mm
/s)
F-λvt (pN)0 2 4 6 8 10 12
0.01
1
a
T = 300 mKF = 55 pN
P( ∆
v)
∆v (mm/s)
P (∆v) = exp(−(∆v/vw)2)
Lifetime of Laminar Phases
Cumulative distribution function:
P (t) = P (∆v(t)) = exp
(−
(∆v(t)
vw
)2)
where
∆v(t) = ∆vmax(1 − exp(−t/τ)).
Failure rate:
Λ(t) = −d lnP (t)dt
= v−2w
d(∆v2)dt
for long times t τ :
∆v = ∆vmax = const and therefore P = const
and hence Λ = 0:
stable laminar phases although v > v
Stability of Laminar Phases
0 100 200 300 400 5001E-3
0,01
0,1
1
45,0 pN
47,1 pN
49,1 pN
51,2 pN
300mK
rel.
Anz
ahl l
amin
arer
Pha
sen
t in s
0 200 400 600 800 1000 1200 14000.01
0.1
1
without 60
Co sourceτ = 25 min
T = 300 mKF = 47 pN
with 60
Co sourceτ = 3 min
norm
aliz
ed n
umbe
r of
lam
inar
pha
ses
t (s)
Summary
Statistics of turbulent phase laminar phase vortex nucleation
CDF exponential(t) Gauss(∆v) double exponential(∆v)
PDF exponential Weibull exp · double exponential
Failure rate const linear exponential
dependence Fturb vw vc(T ), ∆vc
Summary
• A levitating magnetic microsphere is oscillating in liquid
helium in the mK range, creating turbulence.
• Between turbulent and laminar regimes there is a unstable
regime where the system switches between both states
intermittently.
• The velocities reached during laminar phases are Weibull
distributed, while the lifetimes of turbulent phases are
exponentially distributed.
• The distributions are independent of temperature.
• Metastable laminar phases exist, their lifetime is only
limited by natural background radiation
Future
• using different sized spheres
• perform the experiment in superfluid 3He