In classical physics, we can classify optical phenomena into one of two categories: ray optics and wave optics.
Light is a transverse electromagnetic wave. In many situations, the wavelengths of the light being studied are very small
compared to the dimensions of the equipment used to study the light. Under these conditions we can make an approximation called
geometrical optics or ray optics. Consider the wavelength scale of light waves.
Wavelengths in the middle of the visible band are on the order of 500 nm.
So a laser beam with a diameter of 1 mm has a diameter of 2000 wavelengths.
Individual atoms in a solid are separated by distance on the order of 0.1 nm.
So, as far as visible light is concerned, matter is quasi-continuous.
If the wavelengths of the light become comparable to the dimensions of the equipment, then we study optical phenomena using the classical theory of radiation, or wave optics. Wave optics contains all of ray optics, but the mathematical treatment is much more involved.
Diffraction and interference are phenomena observed with all waves. Diffraction can only be observed with waves traveling in two or three dimensions. (We already encountered interference when studying mechanical waves on a string and sound waves in physics 221.)
Diffraction is the tendency of a wave emitted from a finite source or passing through a finite aperture to spread out as it propagates. Diffraction results from the interference of an infinite number of waves emitted by a continuous distribution of source points in two or three dimensions. Huygens' principle lets us treat wave propagation by considering every point on a wave front to be a secondary source of spherical wavelets. These wavelets propagate outward with the characteristic speed of the wave. The wavelets emitted by all points on the wave front interfere with each other to produce the traveling wave. Huygens' principle also holds for electromagnetic waves. When studying the propagation of light, we can replace any wave front by a collection of sources distributed uniformly over the wave front, radiating in phase.
When light passes through a small opening, comparable in size to the wavelength λ of the light, in an otherwise opaque obstacle, the wave front on the other side of the opening resembles the wave front shown on the right.
The light spreads around the edges of the obstacle. This is the phenomenon of diffraction. Diffraction is a wave phenomenon and is also observed with water waves in a ripple tank.
Water waves in a ripple tank
|A single large slit||A single small slit|
Please watch: Apertures and Diffraction - Exploring Wave Motion (YouTube)
When light passes through a single slit whose width w is on the order of the wavelength of the light, then we can observe a single slit diffraction pattern on a screen that is a distance L >> w away from the slit. The intensity is a function of angle. Huygens' principle tells us that each part of the slit can be thought of as an emitter of waves. All these waves interfere to produce the diffraction pattern. Where crest meets crest we have constructive interference and where crest meets trough we have destructive interference.
Very far from a point source the wave fronts are essentially plane
waves. This is called the Fraunhofer regime, and the diffraction pattern is called Fraunhofer diffraction. The positions of all
maxima (constructive interference) and minima (destructive interference) in the
Fraunhofer diffraction pattern can be calculated fairly easily.
The Fraunhofer approximation, however, is only valid when the source, aperture, and detector are all very far apart or when lenses are used to convert spherical waves into plane waves. Being very far apart means that the distances between source, aperture, and detector must be much greater than the width of the aperture.
The Fresnel regime is the near-field regime. In this regime the wave fronts are curved, and their mathematical description is more involved.
The positions of all maxima and minima in the Fraunhofer diffraction pattern from a single slit can be found from the following simple arguments.
If the optical path length of two rays differs by λ/2, the two rays interfere destructively. For ray 1 and ray 7 to be half a wavelength out of phase we need
(w/2)sinθ = λ/2 or w sinθ = λ.
But from geometry, if these two rays interfere destructively, so do rays 2 and
8, 3 and 8, and 6
and 10, 5 and 11, and 6 and 12.
In effect, light from one half of the opening interferes destructively and cancels out light from the other half.
Destructive interference produces the dark fringes. Dark fringes in the diffraction pattern of a single slit are found at angles θ for which
w sinθ = mλ,
where m is an integer, m = 1, 2, 3, ... . For the first dark fringe we have w sinθ = λ.
When w is smaller than λ , the equation w sinθ = λ has no solution and no dark fringes are produced.
If the interference pattern is viewed on a screen a distance L from the slits, then the wavelength can be found from the spacing of the fringes. We have λ = w sinθ/m and sinθ = z/(L2 + z2)½), or
λ = zw/(m(L2 + z2)½),
where z is the distance from the center of the interference pattern to the mth dark line in the pattern.
If L >> z then (L2 + z2)½ ~ z/L and we can write
λ = zw/(mL).
Please watch: Diffraction of Light - Exploring Wave Motion (YouTube)
Link: Diffraction Demo: Single Slit and Circular Aperture (Youtube)
When a monochromatic light source shines through a 0.2 mm wide slit onto a screen 3.5 m away, the first dark band in the pattern appears 9.1 mm from the center of the bright band. What is the wavelength of the light?
Consider a single slit diffraction pattern for a slit width w. It is observed that for light of wavelength 400 nm the angle between the first minimum and the central maximum is 4*10-3 radians. What is the value of w?