Superfluid Droplets on a Solid Surface

D. Ross, J. E. Rutledge and P. Taborek
Department of Physics and Astronomy
University of California, Irvine 92697

Science, 278, 664(1997)



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Paper

Superfluid helium has unusual thermal and mechanical properties[1] and is well known for it ability to spread over surfaces and to flow without dissipation through even microscopic holes. Virtually all of the walls and surfaces used in previous dissipationless flow experiments are wet by superfluid helium. This effect means that droplets on these substrates are unstable and immediately spread to form a smooth continuous film over the entire surface so that vapor and substrate are never in contact. Recent work [2] has shown that alkali metals are a special class of materials not completely wetted by superfluid helium. In particular, cesium substrates can be used to prepare superfluid samples with a distinctly different topology consisting of a droplet with an edge where substrate, superfluid, and vapor meet at a three-phase contact line [3]. We present here direct observations of isolated droplets of superfluid on a substrate [4]. Both the static and dynamic behavior of the droplets are unusual. We found that the contact angle was an extremely hysteretic function of the volume of the drop. Perhaps the most remarkable property of superfluid droplets is that they would not move across the surface until a considerable force was applied to them. This result is surprising because solid surfaces are well known not to exert transverse forces on bulk superfluid or superfluid films without edges.
Our apparatus consisted of a substrate that can be rotated about a horizontal axis mounted in an optical dewar with windows that provide an edge-on view of the substrate as well as a view from above at an angle of 60° from the normal. The substrate is a quartz microbalance with gold electrodes similar to those used in our previous thermodynamic studies[5,6]. Fifty atomic layers of cesium were vapor deposited onto the quartz and gold surfaces of the microbalance at a rate of 0.01 layers/sec. During the evaporation, the temperature of the substrate and the walls of the container were maintained below 6 K to maintain ultra high vacuum conditions. The microbalance was used to monitor the deposition and to perform thermodynamic characterizations of the surface; the wetting temperature was measured to be Tw=2.04 K. A capillary tube (0.04 cm, outside diameter) attached to a source of room-temperature gas through a mass flow controller provided a means of putting drops of superfluid on the surface. The system was maintained at liquid-vapor coexistence by filling the bottom of the container with bulk liquid 4He. The drops were observed with a long focal distance microscope that provided a magnification of approximately 30.
Figures 1 and 2 show a sequence of photographs of superfluid drops on a cesiated substrate at T=1.16K. Figure 1 shows pictures taken with the microscope looking down on the substrate at an angle of 30° above the horizontal. The dark bar at the top of the pictures is the capillary tube, and the lower bar is its shadow. The tube was left in contact with the superfluid drop so that fluid could be added and withdrawn. This geometry is conventional for contact angle measurements and typically yields the advancing and receding contact angle[7]. The drops appear oval because of the viewing angle. The edge of the gold electrode can be seen in the extreme and upper left; the cesium film is too thin to provide appreciable optical contrast. Figure 2 shows edge-on views of the same droplets as shown in Figure1 illuminated from the back. The optical axis is a fraction of a degree above horizontal, so that both the free surface of the drop and its reflection in the substrate are visible. The capillary tube is clearly visible protruding from the top of the drop. The focus was adjusted so that a diameter of the drop lies in the focal plane.
The plane of the substrate can be located by drawing a line between the two points where the profile of the drop meets its mirror image. The contact angle is the angle between the tangent to the drop profile and the substrate at the point of contact. Despite the superfluidity of the drops, the value of the contact angle which we observed depended critically on the way the drop was prepared. When the volume of the drop was increasing, the contact angle was approximately 32° [8] and independent of the volume of the drop; Figure 2A and B, show snapshots of the same drop as fluid was added (the corresponding top view of the growing drop is shown in Figure 1A and B). When fluid was withdrawn, the contact line remained stationary and the receding contact angle approached zero, (Figures 1C and 2C). The bulk fluid could be completely removed, but apparently a thin film remained in the region bounded by the original contact line, since when fluid is added, the drop immediately obtained its previous diameter and only slowly increased its volume and contact angle. The only way to prepare a smaller drop (such as Figure 1A) in the same area was to remove the microscopic film by briefly heating the substrate with a flash of light.
Contact angle hysteresis is a common phenomenon in wetting measurements of conventional liquids and substrates that is typically attributed to substrate heterogeneity, or kinetic effects associated with the viscosity of the liquid, or both [7,9,10]. Because our experiment utilized superfluid and the time scale of the observations was several minutes, kinetics cannot be invoked to explain the hysteresis we observed. Similarly, it is difficult to find a plausible source of surface heterogeneity, because the substrate exhibits the same sharp thermodynamic signatures of the wetting transition that we have explored in previous work[5,6]. In order to explain a receding contact angle of zero, standard models based on consideration of metastable states on a heterogeneous substrate would require that more than half of the surface be covered with patches where the local contact angle is zero, that is, where the liquid wets[7,10]. This possibility is ruled out by microbalance measurements which show that the average equilibrium coverage at liquid-vapor coexistence on our substrate at temperatures far below the wetting temperature is less than 2 monolayers, which implies that the fraction of the surface that was wetted is less than 4%. The possibility of point-like pinning centers also seems unlikely because the contact line (Fig 1) appears perfectly smooth on length scales of a few micrometers.
Although the conventional explanations of contact angle hysteresis due to surface heterogeneity do not apply to our experiment, there must nevertheless be some mechanism which provides metastable states that can trap the droplet in configurations with a continuous range of contact angles. The fact that the contact line did not move even when the apparent contact angle was reduced to zero when the drop was deflated allows us to place a lower limit on the pinning force per unit length which these metastable states can sustain. We assume as is customary that the advancing contact angle is equal to the thermodynamic equilibrium contact angle q [8] which satisfies Young’s equation , slv cosq = ssv- ssl where the sij are surface tensions, and the l,s,v subscripts denote liquid, substrate, and vapor, respectively. In this case, the force per unit length on the contact line due to surface tension when the contact angle was reduced to zero is slv (1- cosq) = 46 mdyne/cm. The maximum pinning force must be at least as large.
Another manifestation of forces on the contact line can be seen when a superfluid drop was placed on an inclined surface. Figure 3 shows an edge-on view of a drop on a cesiated surface inclined at ~ 10° to the horizontal; a pendant drop of fluid formed by forcing helium down the capillary faster than the superfluid film on the outer surface could drain it, can also be seen in the upper right corner. The most remarkable feature of the drop on the substrate is that it is stationary. Even vigorous shaking of the apparatus, which caused easily discernible waves in the drop, did not cause it to flow down the incline. The downhill edge of the drop had the same contact angle as the advancing edge of a growing drop, while the uphill edge had a vanishing contact angle. As more fluid was added to the drop, it eventually rolled down the incline, often with a jerky stick-slip motion. Subsequent drops immediately spread out across the path of the previous drop and rapidly flowed downhill. It seems as if the first drop, which moves across a dry substrate left a trailing film that “lubricates” the motion of subsequent drops. This film, which persisted for hours, may be related to the metastable thick films we have observed in previous experiments[6]. The trailing film had submicroscopic thickness and was invisible in an edge-on view. It could be detected ellipsometrically and was superfluid because locally heating a spot with a laser beam produced a thermo-mechanically driven bump in the film profile.
Superfluid droplets on cesiated substrates have remarkable spreading and flow properties that are not simple consequences of bulk superfluid behavior. Liquid helium has exceptional chemical purity and the heterogeneity of our cesium surface is constrained by thermodynamic adsorption measurements. For these reasons, helium on cesium would naively be expected to display nearly ideal reversible spreading behavior, because even the complications due to viscosity are negligible. In contrast, superfluid contact angles are found to be even more hysteretic than typical classical fluid drops on macroscopically heterogeneous surfaces. The hysteresis is so extreme that the superfluid contact line appears to move in only one direction, that is so as to increase the wetted area.
It is difficult to reconcile these observations with standard models of contact angle hysteresis. Regarded as a superfluid, droplets are remarkable because they can resist flow against a substantial chemical potential gradient. Both of these effects are presumably due to metastable configurations of the superfluid contact line, which have been inaccessible to experimental observation until very recently. In order to attribute the metastability to extrinsic defects, a mechanism allowing small defect concentrations to cause extremely large hysteresis would need to be identified.

This work supported by NSF grant DMR 9623976.