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diff --git a/source/know/concept/rayleigh-plesset-equation/index.md b/source/know/concept/rayleigh-plesset-equation/index.md new file mode 100644 index 0000000..9108d51 --- /dev/null +++ b/source/know/concept/rayleigh-plesset-equation/index.md @@ -0,0 +1,132 @@ +--- +title: "Rayleigh-Plesset equation" +date: 2021-04-06 +categories: +- Physics +- Fluid mechanics +- Fluid dynamics +layout: "concept" +--- + +In fluid dynamics, the **Rayleigh-Plesset equation** +describes how the radius of a spherical bubble evolves in time +inside an incompressible liquid. +Notably, it leads to [cavitation](/know/concept/cavitation/). + +Consider the main +[Navier-Stokes equation](/know/concept/navier-stokes-equations/) +for the velocity field $\va{v}$: + +$$\begin{aligned} + \frac{\mathrm{D} \va{v}}{\mathrm{D} t} + = \pdv{\va{v}}{t} + (\va{v} \cdot \nabla) \va{v} + = - \frac{\nabla p}{\rho} + \nu \nabla^2 \va{v} +\end{aligned}$$ + +We make the ansatz $\va{v} = v(r, t) \vu{e}_r$, +where $\vu{e}_r$ is the basis vector; +in other words, we demand that the only spatial variation of the flow is in $r$. +The above equation then becomes: + +$$\begin{aligned} + \pdv{v}{t} + v \pdv{v}{r} + = - \frac{1}{\rho} \pdv{p}{r} + + \nu \bigg( \frac{1}{r^2} \pdv{}{r}\Big( r^2 \pdv{v}{r} \Big) - \frac{2}{r^2} v \bigg) +\end{aligned}$$ + +Meanwhile, the incompressibility condition +in [spherical coordinates](/know/concept/spherical-coordinates/) yields: + +$$\begin{aligned} + \nabla \cdot \va{v} + = \frac{1}{r^2} \pdv{(r^2 v)}{r} + = 0 +\end{aligned}$$ + +This is only satisfied if $r^2 v$ is constant with respect to $r$, +leading us to a solution $v(r)$ given by: + +$$\begin{aligned} + v(r) + = \frac{C(t)}{r^2} +\end{aligned}$$ + +Where $C(t)$ is an unknown function that does not depend on $r$. +We then insert this result in the main Navier-Stokes equation, +and isolate it for $\ipdv{p}{r}$, yielding: + +$$\begin{aligned} + \pdv{p}{r} + = - \rho \bigg( \frac{1}{r^2} C' - \frac{2}{r^5} C^2 + - \nu \Big( \frac{2}{r^4} C - \frac{2}{r^4} C \Big) \bigg) + = - \rho \bigg( \frac{1}{r^2} C' - \frac{2}{r^5} C^2 \bigg) +\end{aligned}$$ + +Integrating this with respect to $r$ yields the following expression for $p$, +where $p_\infty(t)$ is the (possibly time-dependent) pressure at $r = \infty$: + +$$\begin{aligned} + p(r) + = p_\infty + \rho \bigg( \frac{1}{r} C' - \frac{1}{2 r^4} C^2 \bigg) +\end{aligned}$$ + +From the definition of [viscosity](/know/concept/viscosity/), +we know that the normal [stress](/know/concept/cauchy-stress-tensor/) +$\sigma_{rr}$ in the liquid is given by: + +$$\begin{aligned} + \sigma_{rr}(r) + = - p(r) + 2 \rho \nu \pdv{v(r)}{r} +\end{aligned}$$ + +We now consider a spherical bubble +with radius $R(t)$ and interior pressure $P(t)$ along its surface. +Since we know the liquid pressure $p(r)$, +we can find $P$ from $\sigma_{rr}(r)$. +Furthermore, to include the effects of surface tension, we simply add +the [Young-Laplace law](/know/concept/young-laplace-law/) to $P$: + +$$\begin{aligned} + P + = - \sigma_{rr}(R) + \alpha \frac{2}{R} + = p(R) - 2 \rho \nu \Big( \frac{-2}{R^3} C \Big) + \alpha \frac{2}{R} +\end{aligned}$$ + +We isolate this for $p(R)$, and equate it to +our expression for $p(r)$ +at the surface $r\!=\!R$: + +$$\begin{aligned} + P - \rho \nu \frac{4}{R^3} C - \alpha \frac{2}{R} + = p_\infty + \rho \bigg( \frac{1}{R} C' - \frac{1}{2 R^4} C^2 \bigg) +\end{aligned}$$ + +Isolating for $P$, +and inserting the fact that $R'(t) = v(t)$, +such that $C = r^2 v = R^2 R'$, +yields: + +$$\begin{aligned} + P + &= p_\infty + \rho \bigg( \frac{1}{R} \dv{(R^2 R')}{t} - \frac{1}{2 R^4} (R^2 R')^2 + + \nu \frac{4}{R^3} (R^2 R') \bigg) + \alpha \frac{2}{R} + \\ + &= p_\infty + \rho \bigg( 2 (R')^2 + R R'' - \frac{1}{2} (R')^2 + \nu \frac{4}{R} R' \bigg) + \alpha \frac{2}{R} +\end{aligned}$$ + +Rearranging this and defining $\Delta p \equiv P - p_\infty$ +leads to the Rayleigh-Plesset equation: + +$$\begin{aligned} + \boxed{ + \frac{\Delta p}{\rho} + = R \dvn{2}{R}{t} + \frac{3}{2} \bigg( \dv{R}{t} \bigg)^2 + \nu \frac{4}{R} \dv{R}{t} + \frac{\alpha}{\rho} \frac{2}{R} + } +\end{aligned}$$ + + + +## References +1. B. Lautrup, + *Physics of continuous matter: exotic and everyday phenomena in the macroscopic world*, 2nd edition, + CRC Press. |
