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Rayleigh Instability of an Annulus

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Introduction<br />

A slow-moving, thin cylindrical stream <strong>of</strong> water will become non-uniform in<br />

diameter <strong>an</strong>d eventually break-up into droplets. This is <strong>an</strong> example <strong>of</strong> capillary break-up<br />

<strong>an</strong>d commonly known as <strong>Rayleigh</strong> instability. For a cylindrical jet, Lord <strong>Rayleigh</strong><br />

calculated that the most unstable disturb<strong>an</strong>ce wavelength is about nine times the radius <strong>of</strong><br />

the jet. This “most d<strong>an</strong>gerous mode” (λ = 9.016*r) has been proven experimentally <strong>an</strong>d<br />

c<strong>an</strong> be derived via linear stability <strong>an</strong>alysis.<br />

The purpose <strong>of</strong> this project was to predict the most unstable disturb<strong>an</strong>ce<br />

wavelength for liquid jet <strong>of</strong> varying <strong>an</strong>nular geometry (0 < κ < 1).<br />

κa 0<br />

a 0<br />

Surface Energy Argument<br />

Figure 1. <strong>Annulus</strong> with outer diameter a 0<br />

A disturb<strong>an</strong>ce will grow only if the process is energetically favorable. The<br />

surface energy argument says that if a disturb<strong>an</strong>ce increases the surface energy <strong>of</strong> the<br />

system, that disturb<strong>an</strong>ce will decay due to restoring forces (viscosity), which will bring<br />

the system to its lowest energy state. Figure 1 shows the cross section <strong>of</strong> the unperturbed<br />

<strong>an</strong>nulus with outer radius, a 0 . Figure 2 shows the lengthwise view <strong>of</strong> the jet <strong>of</strong> const<strong>an</strong>t<br />

thickness with a sinusoidal disturb<strong>an</strong>ce.<br />

a(1+Asin(2πx/L))<br />

a(1+Asin(2πx/L)) - (1-κ)a 0<br />

a 0 (1-κ)<br />

Figure 2. Lengthwise view <strong>of</strong> disturbed system<br />

For <strong>an</strong> inviscid, one-dimensional <strong>an</strong>nular jet, the surface energy argument utilizes<br />

the following equation to establish a relationship between a <strong>an</strong>d a 0 (see figure 2 for<br />

definition <strong>of</strong> a <strong>an</strong>d a 0 ). V is the volume <strong>of</strong> the fluid, x is the axial dist<strong>an</strong>ce, L is the<br />

2

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