Introduction to Optics
Light has long captured the fascination of humankind and although we take phenomena such as
reflection, refraction, diffraction
and interference for granted, it is not hard to see why they posed perplexing
problems throughout most of history. Why should light bend upon entering water? Why does light
spread out after passing through a narrow gap? How does light travel to us from the sun, through
the void of space? These sorts of questions have ensured that optics has a long and engaging
history; mirrors were known to the ancients, eyeglasses were known by the thirteenth
century, and, of course, the telescope was invented by Galileo around 1608.
The law of refraction was discovered by Willebrord Snell in 1621 and the phenomenon of
diffraction was observed by both Francesco Maria Grimaldi and Robert Hooke by the mid-1600s. Sir
Isaac Newton made great contributions to optics, proposing that 'white light' was a combination
of all colors, and formulating a particle, or corpuscular, theory of light. At roughly the same time (the latter
half of the seventeenth century), the Dutch physicist Christian Huygens proposed a powerful wave theory of
light. As we shall discover, most of the history of optics is dominated by the debate over the nature of light:
is light a particle or a wave, or is it something in between (a wavicle?)?
Another important figure in the history of optics is Thomas Young, an Englishman who revived the wave
theory at the beginning of the nineteenth century by adding to it the principle of superposition.
The French scientist Augustin Jean Fresnel, also an advocate of the wave theory, proposed a mechanistic
description of light on the basis of it being a transverse oscillation through the
ether, rather than a longitudinal one as had previously been assumed. The
corpuscular theory seemed in very bad shape indeed. By 1845 Michael Faraday had performed several
experiments showing that the plane of polarization could be altered by magnetic fields. This
ultimately led to James Clerk Maxwell's brilliant unification of optics and electromagnetism, when his wave
equations predicted that the speed of light should be
1/
, which was remarkably
close to the experimental value. Light, then, was an electromagnetic disturbance propagating through the
ether.
As a wave, however, light must have a medium through which to propagate. Towards the end of the
nineteenth century this medium, called the ether, became increasingly problematic;
experiments by Michelson and Morley in particular could detect no motion of the ether
relative to the earth. Such considerations led to Einstein's theory of special
relativity and to the discarding of the idea of the ether altogether. Moreover, as the
twentieth century progressed, quantum mechanics showed that all particles have a
wavelike property; the distinction between waves and particles became less and less clear.
In this guide we will treat light usually as a wave, but sometimes as a particle, and as a general rule
it is both or either. First, we will examine light as a wave, the relationship between light and
electromagnetism, and gain some insight into how light interacts with matter. In the second topic, we will
apply the laws of reflection and refraction to geometric optics. Finally, we will consider the important
phenomena of interference, diffraction, and polarization.