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Modelling levitated 2-lobed droplets in rotation using Cassinian oval curves

Published online by Cambridge University Press:  15 May 2018

Haruki Ishikawa*
Affiliation:
Department of Aeronautics and Astronautics, School of Engineering, The University of Tokyo, 7-3-1, Hongo, Bunkyo-ku, Tokyo 113-8656, Japan
Katsuhiro Nishinari
Affiliation:
Research Center for Advanced Science and Technology, The University of Tokyo, 4-6-1, Komaba, Meguro-ku, Tokyo 153-8904, Japan
*
†Email address for correspondence: ishikawa@jamology.rcast.u-tokyo.ac.jp

Abstract

A simple model of rotating 2-lobed droplets is proposed by setting the outline shape of the droplet to the Cassinian oval, a mathematical curve that closely resembles in shape. By deriving the governing equation of the proposed model and obtaining its stationary solutions, the relationship between the angular velocity of rotation and the maximum deformation length is explicitly and precisely calculated. The linear stability analysis is performed for the stationary solutions, and it is demonstrated that the stability of the solutions depends only on the ratio of the deformation length to the radius of the central cross-section of the droplet, which is independent of the physical properties of the droplet. Via comparison with an experimental study, it is observed that the calculated result is consistent with the deformation behaviour of actual 2-lobed droplets in the range where the stationary solution of the proposed model is linearly stable. Therefore, the proposed model is a suitable model for reproducing the steady deformation behaviour of 2-lobed droplets in a wide range of viscosities, surface tensions, densities and initial radii of the droplet, and especially if the viscosity of the droplet is low, the entire process of deformation of the 2-lobed droplet, including the unsteady breakup process, can be very well reproduced by the proposed model.

Information

Type
JFM Papers
Copyright
© 2018 Cambridge University Press 
Figure 0

Figure 1.(a) Schematic of a 2-lobed droplet and the rotational Cartesian frame fixed to the rotating droplet. The origin is located at the centre of gravity of the droplet, the $z$ axis and the $x$ axis are fixed to the vector of angular velocity $\unicode[STIX]{x1D74E}$ and the axisymmetrical axis of the droplet shape, respectively. The cross-sectional radius at the position $x$ is $h(x)$. (b) Side view of Cassinian droplets in the rotating frame drawn using (2.9) and the equation of volume conservation. The parameter $A$ is 0.8210, which is the same value as $A_{\mathit{opt}}$ determined in § 3. The solid lines are a series of Cassinian droplets for $u_{\ast }/v_{\ast }:=R_{\mathit{Max}\ast }/H_{\mathit{mid}\ast }=2,~3,~5,~10$ and $150$ (blue, light blue, green, purple, red lines, respectively). The outward arrow at the bottom right of the figure shows the increase in $k$, that is, the progress of deformation. The broken line indicates a spherical drop with the same volume.

Figure 1

Figure 2.Results of least squares fittings using the ascending part of the 2-lobed branch of Brown and Scriven’s numerical calculation (figure 6 of Brown & Scriven (1980), red lines shown in panels (b) and (d)) and the experimentally obtained scatter plot (figure 4 of Tanaka et al.2013). (a,b) Least squares regression between (3.11) and Brown and Scriven’s numerical solution. The plot of Brown and Scriven’s solution is fitted best when $A=0.821$. The coefficient of determination, $R^{2}$, is approximately 0.984. (c,d) Result of the least squares fitting using the experimentally obtained scatter plot as the dataset. The experimental result is very well approximated by (3.11) when $A=0.8185$. The coefficient of determination is approximately 0.928. Panel (d) is created by using the data provided by authors of Tanaka et al. (2013). The entire data are shown in figure 4 of Tanaka et al. (2013).

Figure 2

Figure 3.The outline shape of an experimentally stretched low-viscosity 2-lobed droplet ($\unicode[STIX]{x1D702}=0.0026~\text{Pa}~\text{s}$) is compared with a corresponding Cassinian oval curve $z_{\ast }=h_{\ast }(x_{\ast };k,A_{\mathit{opt}})$. (a) The Cassinian oval curve of $A_{\mathit{opt}}=0.821$ (solid lines) fits the outline shape of the experimentally stretched 2-lobed droplet very well. The rotation rate and deformation length of the Cassinian droplet are calculated as $(\unicode[STIX]{x1D714}_{\ast },R_{\mathit{Max}\ast })\simeq (0.331,2.06)$ using (3.11), and this calculated result closely approximates the deformation state $(\unicode[STIX]{x1D714}_{\ast },R_{\mathit{Max}\ast })=(0.332,2.091)$ in the experiment. (b)–(d) Three snapshots capturing the low-viscosity droplet immediately before its neck region pinches off. Although the outline shape of the low-viscosity droplet is not fitted well by the Cassinian oval curve itself for snapshots (c,d), the outline shape of the droplet is expressed by the combination of the breakup limit of the Cassinian oval curve and the interpolating hyperbolic cosine function (the broken line) smoothly connected with the Cassinian oval. Each snapshot is provided by the authors of Tanaka et al. (2013), and each snapshot is binarised by authors of this paper in order to clarify the outline shape of the droplet.

Figure 3

Figure 4.(a) Relationship between angular momentum and rotation rate of the droplet that has the equilibrium shape belonging to the 2-lobed branch computed in Heine (2006) and that of the proposed ‘Cassinian droplet’ of $A_{\mathit{opt}}=0.821$ are compared. The scatter plot shown in panel (a) is created by reading off values from the 2-lobed branch of the computational result that is presented in figure 12 of Heine (2006). (b) The deformation of the Cassinian droplet is compared with the deformation of the actual droplet in rotation presented in Baldwin et al. (2015). The solid line shows $v_{\ast }^{3}/(4\unicode[STIX]{x03C0}/3)$ of the Cassinian droplet of $A_{\mathit{opt}}=0.821$, which models 2-lobed droplets of circular cross-section, and is consistent with the deforming behaviour of the 2-lobed droplet obtained from Baldwin et al. (2015). The scatter plot shown in panel (b) is created by reading off values from figure 4 of Baldwin et al. (2015).

Figure 4

Figure 5.The solution of (3.16) is plotted for different values of the integral constant $C$ in case of $A_{\mathit{opt}}=0.821$. For each value of $C$, the limit $\lim _{k\rightarrow \infty }t_{\ast }(k)$, the time required for the extremely low-viscosity Cassinian droplet to reach breakup, is a finite value.

Figure 5

Figure 6.Calculation results derived from the proposed model are plotted for different values of the parameter $A$. Red lines, green lines and blue lines correspond to the plots for $A=1.0$, $A=0.9$, $A=0.8$, respectively. (a) $D(k;A)$ and $(\text{d}/\text{d}k)(2\unicode[STIX]{x1D714}_{\ast ,s}(k;A)I_{zz\ast }(k;A))$ are plotted as functions of $k$. For each value of $A$, $D(k;A)$ and $(\text{d}/\text{d}k)(2\unicode[STIX]{x1D714}_{\ast ,s}I_{zz\ast })$ are monotonic functions that intercept the horizontal line at $k=k_{\mathit{crit},A}$. (b) Parametric plots of $(\unicode[STIX]{x1D714}_{\ast ,s}(k;A),u_{\ast }(k;A))$ are illustrated for $A=1.0$, $0.9$ and $0.8$. Each solid line is a set of linearly stable solutions and each broken line is the set of unstable solutions for the corresponding value of $A$.