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Physical review. B, Condensed matter

Superfluid turbulence in a nonuniform rectangular channel

Julie F. Kafkalidis, G. Klinich, J. T. Tough

Published Dec 1, 1994• 10 citations
Publisher

Abstract

In this detailed study of inhomogeneous superfluid turbulence created in a spatially nonuniform flow, we measure the turbulent dissipation produced by thermal counterflow in a nonuniform rectangular channel. The width of the channel increases linearly with position r along the channel length to impose a known spatial nonuniformity on the velocity in the flow direction, V\ensuremath{\propto}Q\ifmmode \dot{}\else \.{}\fi{}/r, where Q\ifmmode \dot{}\else \.{}\fi{} is the heat current. Because the channel widens gradually, this divergence is weak, producing a small deviation from uniform flow. Probes embedded in the channel walls allow access to the local temperature at several positions r. We employ sensitive differential thermometry to measure the temperature difference between any two of these locations to high precision. The single turbulent state we observe is clearly the analog of the T-II state of fully developed, homogeneous turbulence present in uniform flows. Making an approximation of local uniformity, we attempt to extend the theoretical description of turbulence in uniform flows to our results by replacing the uniform velocity with the local velocity in the expression for the temperature gradient. When applied locally, the Schwarz model of homogeneous turbulence, so successful in describing the T-II state in uniform flows, has the wrong dependence on both r and Q\ifmmode \dot{}\else \.{}\fi{} to characterize our results. The Geurst three-fluid model, which extends to situations where a gradient is present in the line density in an otherwise uniform flow, likewise does not agree with our observations when used in the local approximation.We therefore find that even a small perturbation imposed on a uniform flow radically changes the nature of the T-II state, and the inhomogeneous T-II state we observe is markedly different from that of homogeneous turbulence. This rather surprising result points to the need for a proper theory, or direct numerical simulation, of inhomogeneous turbulence in nonuniform flow. By introducing a substantial modification to the Schwarz line density, we identity a modified line density that constitutes a three-parameter fit yielding excellent agreement with our results. Finally, we find that the transition from laminar to turbulent flow occurs at a stationary front. Observations of the location of this front as a function of Q\ifmmode \dot{}\else \.{}\fi{} show that the critical condition for maintaining turbulence is more consistent with a minimum line density than a critical velocity.

DOI
10.1103/physrevb.50.15909

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In this detailed study of inhomogeneous superfluid turbulence created in a spatially nonuniform flow, we measure the turbulent dissipation produced by thermal counterflow in a nonuniform rectangular channel. The width of the channel increases linearly with position r along the channel length to impose a known spatial nonuniformity on the velocity in the flow direction, V\ensuremath{\propto}Q\ifmmode \dot{}\else .{}\fi{}/r, where Q\ifmmode \dot{}\else .{}\fi{} is the heat current. Because the channel widens gradually, this divergence is weak, producing a small deviation from uniform flow. Probes embedded in the channel walls allow access to the local temperature at several positions r. We employ sensitive differential thermometry to measure the temperature difference between any two of these locations to high precision. The single turbulent state we observe is clearly the analog of the T-II state of fully developed, homogeneous turbulence present in uniform flows. Making an approximation of local uniformity, we attempt to extend the theoretical description of turbulence in uniform flows to our results by replacing the uniform velocity with the local velocity in the expression for the temperature gradient. When applied locally, the Schwarz model of homogeneous turbulence, so successful in describing the T-II state in uniform flows, has the wrong dependence on both r and Q\ifmmode \dot{}\else .{}\fi{} to characterize our results. The Geurst three-fluid model, which extends to situations where a gradient is present in the line density in an otherwise uniform flow, likewise does not agree with our observations when used in the local approximation.We therefore find that even a small perturbation imposed on a uniform flow radically changes the nature of the T-II state, and the inhomogeneous T-II state we observe is markedly different from that of homogeneous turbulence. This rather surprising result points to the need for a proper theory, or direct numerical simulation, of inhomogeneous turbulence in nonuniform flow. By introducing a substantial modification to the Schwarz line density, we identity a modified line density that constitutes a three-parameter fit yielding excellent agreement with our results. Finally, we find that the transition from laminar to turbulent flow occurs at a stationary front. Observations of the location of this front as a function of Q\ifmmode \dot{}\else .{}\fi{} show that the critical condition for maintaining turbulence is more consistent with a minimum line density than a critical velocity.
Finite-temperature quantum turbulence is often described in terms of two immiscible fluids that can flow with a nonzero-mean relative velocity. Such out-of-equilibrium state is known as counterflow superfluid turbulence. We report here the emergence of a counterflow-induced inverse energy cascade in three-dimensional superfluid flows by performing extensive numerical simulations of the Hall-Vinen-Bekarevich-Khalatnikov model. As the intensity of the mean counterflow is increased, an abrupt transition, from a fully three-dimensional turbulent flow to a quasi-two-dimensional system exhibiting a split cascade, is observed. The findings of this work could motivate new experimental settings to study quasi-two-dimensional superfluid turbulence in the bulk of three-dimensional experiments. They might also find applications beyond superfluids in systems described by more than one fluid component.
Describing superfluid turbulence at intermediate scales between the intervortex distance and the macroscale requires an acceptable equation of motion for the density of quantized vortex lines L\mathcal{L}L. The closure of such an equation for superfluid inhomogeneous flows requires additional inputs besides L\mathcal{L}L and the normal and superfluid velocity fields. In this paper, we offer a minimal closure using one additional anisotropy parameter Il0{I}_{l0}Il0​. Using the example of counterflow superfluid turbulence, we derive two coupled closure equations for the vortex line density and the anisotropy parameter Il0{I}_{l0}Il0​ with an input of the normal and superfluid velocity fields. The various closure assumptions and the predictions of the resulting theory are tested against numerical simulations.
The quantization of vortex lines in superfluids requires the introduction of their density $\mathcal{L}(\mathbit{r},t)$ in the description of quantum turbulence. The space homogeneous balance equation for L(t)\mathcal{L}(t)L(t), proposed by Vinen on the basis of dimensional and physical considerations, allows a number of competing forms for the production term P\mathcal{P}P. Attempts to choose the correct one on the basis of time-dependent homogeneous experiments ended inconclusively. To overcome this difficulty we announce here an approach that employs an inhomogeneous channel flow which is very suitable to distinguish the implications of the various possible forms of the desired equation. We demonstrate that the originally selected form which was extensively used in the literature is in strong contradiction with our data. We therefore present a new form of an inhomogeneous equation for $\mathcal{L}(\mathbit{r},t)$ that is in agreement with our data and propose that it should be considered for further studies of superfluid turbulence.
Turbulence, the irregular motion of fluids, is a challenging problem in physics. Yet some properties of turbulence appear to be universal, independent of the underlying host fluid supporting the motion. Recent studies have found that turbulence in superfluid helium, a quantum fluid, exhibits two of the most fundamental laws of classical fluid turbulence: the Kolmogorov −5/3 law, and the dissipation anomaly. These laws appear despite the fluid being highly constrained by quantum mechanical effects, and completely lacking kinematic viscosity. Such findings suggest further insight into the universal features of turbulent phenomena can be gained by studying analogies between classical and quantum turbulence.\nAtomic Bose-Einstein condensates (BECs) offer a new platform for the study of quantum turbulence; the geometric control available in BEC experiments offers the possibility of studying quantum turbulence in effectively two-dimensional fluids. As two-dimensional turbulence exhibits dramatically different features from its 3D counterpart, BEC systems allow for further study of the analogies between classical and quantum turbulence. In this thesis we numerically and theoretically study 2D quantum turbulence in BECs within the framework of the Gross-Pitaevskii model. We focus on analogies with classical 2D turbulence, with the aim of identifying common or universal features.\nFirst we investigate coherent vortex structures in negative temperature equilibria via an experimentally accessible flow-field measure. Coherent vortices are shown to produce a clear signal in this measure that is independent of the confinement geometry, and we demonstrate that it can be observed in dynamical simulations.\nSecond, studying a quantum analogue of the two-dimensional cylinder wake, we investigate the phenomenon of Strouhal oscillations. We find that the Strouhal number obeys a universal relation, similar to the classical form, upon introducing a modified superfluid Reynolds number that accounts for the critical velocity for vortex nucleation. Like the classical Reynolds number, the superfluid Reynolds number is found to govern the transition from laminar to turbulent behaviour in the quantum fluid.\nFinally, simulating decaying 2D quantum turbulence for very large vortex numbers, we show that quantum fluids are capable of supporting the direct enstrophy cascade, a fundamental feature of two-dimensional turbulent flows. The quantum fluid manifests key features of the classical cascade, including Batchelor’s −3 law of the inertial range, scaling of the inertial range against the superfluid Reynolds number, and the value of the Kraichnan-Batchelor constant.\nThe findings from this work thus provide some new insight into the universality of fundamental turbulence concepts, and their applicability to quantum fluids.
We describe a technique, using thin lines of triplet-state He2∗\mathrm{He}_{2}^{*}He2∗​ molecular tracers created by femtosecond-laser field ionization of helium atoms, for visualizing the flow of the normal fluid in superfluid 4He^{4}\mathrm{He}4He, together with its application to thermal counterflow in a channel. We show that, at relatively small velocities, where the superfluid is already turbulent, the flow of the normal fluid remains laminar, but with a distorted velocity profile, while at a higher velocity there is a transition to turbulence. The form of the structure function in this turbulent state differs significantly from that found in types of conventional turbulence. This visualization technique also promises to be applicable to other fluid dynamical problems involving cryogenic helium.
Using the classical field method, we study numerically the characteristics and decay of the turbulent tangle of superfluid vortices which is created in the evolution of a Bose gas from highly nonequilibrium initial conditions. By analyzing the vortex line density, the energy spectrum, and the velocity correlation function, we determine that the turbulence resulting from this effective thermal quench lacks the coherent structures and the Kolmogorov scaling; these properties are typical of both ordinary classical fluids and of superfluid helium when driven by grids or propellers. Instead, thermal quench turbulence has properties akin to a random flow, more similar to another turbulent regime called ultraquantum turbulence, which has been observed in superfluid helium.