From e2f6ff4487606f4052b9c912b9faa2c8d8f1ca10 Mon Sep 17 00:00:00 2001 From: Prefetch Date: Sun, 18 Jun 2023 17:59:42 +0200 Subject: Improve knowledge base --- source/know/concept/capillary-length/index.md | 79 +++++++++++++++++++++++++++ 1 file changed, 79 insertions(+) create mode 100644 source/know/concept/capillary-length/index.md (limited to 'source/know/concept/capillary-length') diff --git a/source/know/concept/capillary-length/index.md b/source/know/concept/capillary-length/index.md new file mode 100644 index 0000000..4dbb788 --- /dev/null +++ b/source/know/concept/capillary-length/index.md @@ -0,0 +1,79 @@ +--- +title: "Capillary length" +sort_title: "Capillary length" +date: 2021-03-29 +categories: +- Physics +- Fluid mechanics +- Fluid statics +- Surface tension +layout: "concept" +--- + +**Capillary action** refers to the movement of liquid +through narrow spaces due to surface tension, often against gravity. +It occurs when the [Laplace pressure](/know/concept/young-laplace-law/) +from surface tension is much larger in magnitude than the +[hydrostatic pressure](/know/concept/hydrostatic-pressure/) from gravity. + +Consider a spherical droplet of liquid with radius $$R$$. +The hydrostatic pressure difference +between the top and bottom of the drop +is much smaller than the Laplace pressure: + +$$\begin{aligned} + 2 R \rho g \ll 2 \frac{\alpha}{R} +\end{aligned}$$ + +Where $$\rho$$ is the density of the liquid, +$$g$$ is the acceleration due to gravity, +and $$\alpha$$ is the energy cost per unit surface area. +Rearranging the inequality yields: + +$$\begin{aligned} + R^2 \ll \frac{\alpha}{\rho g} +\end{aligned}$$ + +From this, we define the **capillary length** $$L_c$$ +such that gravity is negligible if $$R \ll L_c$$: + +$$\begin{aligned} + \boxed{ + L_c + \equiv \sqrt{\frac{\alpha}{\rho g}} + } +\end{aligned}$$ + +In general, for a system with characteristic length $$L$$, +the relative strength of gravity compared to surface tension +is described by the **Bond number** $$\mathrm{Bo}$$ +or **Eötvös number** $$\mathrm{Eo}$$: + +$$\begin{aligned} + \boxed{ + \mathrm{Bo} + \equiv \mathrm{Eo} + \equiv \frac{L^2}{L_c^2} + } +\end{aligned}$$ + +Capillary action is observed when $$\mathrm{Bo \ll 1}$$, +while for $$\mathrm{Bo} \gg 1$$ surface tension is negligible. + +For an alternative interpretation of $$\mathrm{Bo}$$, +let $$m \equiv \rho L^3$$ be the mass of a cube with side $$L$$ +such that its weight is $$m g$$. +The tension force on its face is $$\alpha L$$, +so $$\mathrm{Bo}$$ is simply the force ratio: + +$$\begin{aligned} + \mathrm{Bo} + = \frac{m g}{\alpha L} +\end{aligned}$$ + + + +## References +1. B. Lautrup, + *Physics of continuous matter: exotic and everyday phenomena in the macroscopic world*, 2nd edition, + CRC Press. -- cgit v1.2.3