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Europhys. Lett., 67 (1) , pp. 56-62 (2004)
DOI: 10.1209/epl/i2004-10081-1
Vortex waves in a rotating superfluid
K. L. Henderson1 and C. F. Barenghi21 School of Mathematical Sciences, CEMS, University of the West of England Bristol, BS16 1QY, UK
2 School of Mathematics and Statistics, University of Newcastle Newcastle upon Tyne, NE1 7RU, UK
(Received 14 January 2004; accepted in final form 30 April 2004)
Abstract
In a recent experiment, Finne et al. discovered an intrinsic
condition for the onset of quantum turbulence in
-
, that
, where
and
are mutual friction parameters. The
authors put forward a qualitative argument that
q is the ratio
of dissipative and inertial forces on the superfluid, so for
q<1 inertial forces should overcome the dissipative forces and
cause turbulence. Thus
1/q would play, for a quantum fluid, the
same role played in classical fluid dynamics by the Reynolds
number (the ratio of inertial forces and dissipative forces in
the Navier-Stokes equation). The aim of this work is to
supplement this qualitative condition
q=1 with a quantitative
calculation. By analysing both axisymmetric and non-axisymmetric
modes of a continuum of vortices in a rotating superfluid, we
find that in the long axial wavelength limit the condition
q=1
is the crossover between damped and propagating Kelvin waves;
thus, for
q>1, perturbations on the vortices are unlikely to
cause vortex reconnections and turbulence. Besides the relevance
to the experiment of Finne et al. , the spectrum of oscillations
which we find is relevant to the study of torsional oscillations
of a rotating superfluid and generalises to three dimensions the
spectrum of Kelvin waves on an isolated vortex line.
67.40.Vs - Vortices and turbulence.
67.57.-z - Superfluid phase of liquid
© EDP Sciences 2004
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