Experiment description
Experiment description
The experiment is designed to detect an acoustic signal generated
by vortex slips in superfluid 4He flowing through an aperture.
The acoustic spectrum is expected to have a Fourier component
at a frequency proportional to the chemical potential (pressure)
difference between the regions on either side of the aperture.
The coefficient of proportionality is independent of the experimental
details and can be expressed through fundamental constants only,
providing a possible pressure standard.
Simplified experimental setup
The experimental setup consists of two reservoirs filled with
superfluid helium, separated by a small aperture. A pressure
differential is applied by means of a "piston". Flow rate of a normal
fluid in such system would be uniform, limited by viscosity in the aperture.
Superfluid flow
One of the remarkable properties of liquid helium is its ability
under certain circumstances to flow without dissipation of energy.
For example, superfluid flow will persist in a ring-shaped pipe
indefinitely. The viscosity associated with such flow is exactly
zero. The flow is potential: the curl of the velocity field
is zero and the velocity field itself can be described by a
gradient of a scalar potential. It is easy to show that in
a quantum mechanical description this potential is the phase
of the superfluid wave function. The quantum mechanical description
applies an additional restriction on the potential. For the
wave function to remain single-valued, the phase variation integral
along any path originating and ending at the same point
can only be a multiple of
. Since the phase gradient is
proportional to flow velocity, the
path integral of the velocity field
is also quantized.
This condition is called circulation quantization, and the
unit of such quantization is
,
where
is Plank's constant and
is the mass of a helium atom.
Vortex generation
Consider a system of two reservoirs connected with a small aperture
filled with superfluid helium.
The implication of viscosity-free flow is that there can be a
constant non-zero flow from one side of the system into the other
without any pressure difference between them.
When a pressure difference is applied, the liquid in the flow
channel accelerates until some critical flow is reached.
At this point, the flow becomes dissipative. Although Landau
theory predicts breakdown of superfluidity via creation of
elementary excitations when the relative velocity of the superfluid
and normal components reaches a critical velocity (of the order of
55 meters per second), in macroscopic systems the observed
critical velocities are typically lower and appear to depend
on the flow channel geometry.
This dissipation is believed to be due to formation of
quantized vortices.
Superfluidity is broken near the center (core) of such vortex.
The circulation
for any path that has the vortex inside is exactly
.
Vortices
with mutiple quanta are unstable and will break up into several
vortices with one quantum of circulation each.
The vortex is most likely to spawn from the surface in the spot
with the highest local velocity, probably near a protrusion on the
inside surface of the aperture. Once the vortex is formed, it is
driven across the flow by Magnus force and collapses after crossing
the aperture. The typical time to cross the aperture is estimated
to be several to tens of microseconds.
Slip size quantization
The crossing of the vortex results in a flow velocity drop near the
aperture.
The phase difference between velocity path integrals
taken along Path 1 and Path 2 differ by one unit of circulation
.
(only a single vortex is inside the loop formed by the two paths).
If points A and B
are taken to be in the regions where the velocity does not change
significantly during the phase slip, the velocity path integral
before and after the slip occurred differ by one unit of circulation,
or
. Assuming that velocities
along any given path scale with the velocity
at some point on that path inside the aperture ,
the jump in
during the slip
is
, where
is the effective length of the
aperture, i.e., the characteristic length over which the velocity
varies. In a long channel, the effective length is equivalent to the
length of the channel; in case of an aperture the length is the thickness of
the membrane plus a length associated with edge effects.
Phase evolution; Josephson frequency
In the time interval between the slips, the liquid accelerates due to the
pressure differential. In the absence of energy loss, the effect of the
pressure gradient is to accelerate helium uniformly, with acceleration
proportional to the pressure gradient.
The difference in phases of the superfluid wave function between points A and B evolves according to the Josephson-Anderson phase evolution formula:
.
Indeed, if the points A and B are
in regions of space little perturbed by the flow through the aperture,
the amplitude of the wave function remains constant and
the phase evolution is linear in time, with the
rate of evolution proportional to the local potential. Although the potential
is only defined up to an additive constant, the potential difference is a well
defined quantity as long as the pressure in each of the volumes is well
defined.
If the phase difference
(which is proportional to the helium flow velocity), at which the slips
occur, is
the same for all slips, and the size of the phase slip is exactly
, the slip rate (frequency) is
.
There are several important points regarding this frequency dependence:
- The frequency is independent of the experimental details: aperture
size and shape, temperature (except through density), size of reservoirs, etc.
- Slip frequency is 6.9x104
Hz/Pa.
- Although the formula relating the frequency and the chemical potential
is the same for vortex slips and {Josephson weak links} -- {Irene: add link to 3He weak links}, the two processes are fundamentally different. In the
the ideal weak link, the current-phase relationship is sinusoidal with
no net flow, whereas in the system described here the current varies around
some average current.
The velocity step size is a function of the aperture size, with larger
steps accuring in smaller apertures.
Detection Method
The idea of the experiment is to detect sound waves generated by periodic
velocity variations in the aperture. A microphone mounted in one of the
helium reservoirs can detect pressure oscillations associated with the
periodic flow. In addition, the reservoir itself acts as a resonant cavity,
amplifying the weak signal.
A constant pressure drop across the aperture is maintained by a feedback loop
which includes a capacitive pressure gauge and a piezoelectric driver
(piston).
The signal is detected at the resonance frequencies of the cavity as
a function of the applied pressure differential.
Stochastic vortex generation
In the discussion above the assumption was that all the slips will happen at
exactly the same velocity. This assumption, however, is not justified. In fact,
critical flow velocities in an aperture typically have some finite
distribution width. Moreover, critical flow velocities show a characteristic
temperature dependence, increasing linearly as the temperature is lowered from
the superfluid transition temperature. The average critical flow velocity
also appears to increase logarithmically with the pressure head.
Phenomenologically, both of these effects can be explained by a model
(Packard
and Vitale 1992) in which the vortex nucleation process is stochastic with probability
described by Arrhenius equation

where
is the attempt frequency and
is the activation energy.
Instead of the regular sawtooth velocity evolution described above, one expects
to find an irregular pattern. The extent of the irregularity can be quantified by
the ratio of the critical velocity distribution width to the slip size.
The fourier components of the velocity spectrum
get less pronounced and the signal appears more noise-like as this ratio
increases.
The noise is similar to shot noise due to finite electron charge in
electronics.
Computer simulations
The effect of the stochastic nature of phase slip generation is illustrated
in the results of a computer simulation below. For a set of different
distribution widths, the velocity evolution is simulated. The fourier
spectrum is then computed. For each set, an ideal (zero width) distribution
and 1/f noise of the same RMS amplitude are shown. You can also listen to the
generated waveform
Narrow distribution
Time evolution (.wav format sound):

Fourier transform:

Medium distribution
Time evolution (.wav format sound):

Fourier transform:

Wide distribution
Time evolution (.wav format sound):

Fourier transform:

Past results and future research directions
Shot-like noise generated by superfluid flow through an aperture was
detected and characterized in this laboratory
(Backhaus and Packard 1998).
The acoustic noise amplitude was measured as a function of the pressure head
for two different cell resonances. However, the signal did not appear to
contain features corresponding to the Josephson frequency.
The size of the apertures used in the experiment was such that the
critical velocity distribution width was larger than the slip size, and
the stochastic spectrum dominated.
To see the signal at the Josephson frequency one has to use apertures
of smaller size. The acoustic amplitude of a signal generated by a smaller
aperture is reduced. However, if the detection limit is determined by the
signal to noise ratio rather than by the signal intensity, this would not be a
problem. In the past experiments, a capacitance microphone was used to detect
the acoustic signal. In addition to the acoustic noise generated by the
phase slips, the microphone was sensitive to electric noise
from elsewhere. A SQUID-based displacement transducer will provide a less
noisy and a more sensitive method of detection. Other possible directions
of research include the use of aperture arrays and attempts to approach
the superfluid transition temperature where the coherence length approaches
the aperture size.
Further reading
- Richard E. Packard. The role of the Josephson-Anderson equation in superfluid helium.
Review of Modern Physics, Vol. 70, No. 2, p. 641 (1998)
- Scott Backhaus and Richard E. Packard. Shot Noise Radiation Generated by Phase Slippage is Superfluid 4He. Physical Review Letters, Vol. 81, No. 9, p 1893 (1998)
- Richard E. Packard and Stefano Vitale. Physical Review B 45, 2512-2515 (1992)