The Optical Lever

An optical lever is a convenient device to magnify a small displacement and thus to make possible an accurate measurement of the displacement. Experiment M-11, Young's modulus, uses an optical lever to magnify the extension of a wire produced by a series of different loads.

The plate P carries a mirror M. The mirror mount has two points resting in a fixed groove, F, and at the other end has a single point resting on the object whose displacement one is measuring. Raising the object through a distance $ \Delta$L will tilt the mirror through an angle $ \theta$ or $ \Delta$L/d radians (approximately) but will turn the light beam through an angle 2$ \theta$.

\includegraphics[width=5.7in]{figs/a03-01.eps}

Figure 1: Schematic of the optical lever.

Hence

$\displaystyle \theta$   =  $\displaystyle {\frac{{\Delta L}}{{d}}}$ $\displaystyle \sim$ $\displaystyle {\frac{{\frac{1}{2}
( y_1-y_0)}}{{D}}}$

if $ \theta$ is small so that $ \theta$ $ \sim$ tan$ \theta$. Therefore

2$\displaystyle \theta$ = $\displaystyle {\frac{{2\Delta L}}{{d}}}$ = $\displaystyle {\frac{{y_1-y_0}}{{D}}}$,  and  $\displaystyle \Delta$l = (y1 - y0)$\displaystyle \left[\vphantom{ \frac{d}{2D}}\right.$$\displaystyle {\frac{{d}}{{2D}}}$$\displaystyle \left.\vphantom{ \frac{d}{2D}}\right]$  .

Note that with the telescope nearly perpendicular to the scale at the beginning then y0 is close to the telescope, and the difference between two elongations ( $ \Delta$L2  - $ \Delta$L1) is very accurately given by

$\displaystyle \Delta$L2  - $\displaystyle \Delta$L1 = $\displaystyle {\frac{{y_2~d}}{{2D}}}$ - $\displaystyle {\frac{{y_1~d}}{{2D}}}$ = $\displaystyle {\frac{{( y_2-y_1) d}}{{2D}}}$

where yi is the scale reading. This relation holds so long as 2$ \theta$ is small enough that tan 2$ \theta$  $ \sim$ 2$ \theta$.


Michael Winokur 2007-09-07