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MULTIPLE SLITS: THE DIFFRACTION GRATING sin θ = nλ d , n = 0, 1, 2, 3,... as for the double slit (Equation 2). Figure 6 shows the situation.
Typology: Lecture notes
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In this experiment you will demonstrate the wave nature of light by investigating how it bends around edges and how it interferes constructively and destructively. You will observe these effects in a variety of situations and use the wave theory of light to measure wavelength.
If light is made of particles, a beam of such particles should pass straight through a long, narrow slit and form a single spot on a screen placed beyond the slit. If it is wavelike in nature, a more complex pattern results. The light waves reaching a given point on the screen each arrive from a different part of the slit, so their amplitudes must be added, and an interference pattern results. Consider pairs of points separated by a distance of half the slit width, such as (A,B) or (C,D) in Figure 1 below. There exists a location on the screen for which waves coming from point C are out of phase with waves from point D by exactly one-half of a wavelength, so their amplitudes add to zero.
A
B
C
D
θ^ brightn = 0
n = 1
dark
n = 2
dark
n = 3
dark
n = 1
dark
n = 2
dark
n = 3
dark
SCREEN
λ 2
a
Figure 1
The situation shown (n=1) in Figure 1 is for the first destructive minimum and occurs at two positions with angles sin^ θ^ =^ λ^ /^ a.
Additional minima occur at sin θ = n λ / a. The n = 1 minimum is the most important one. For small^ θ, the angle in radians is^ θ^ =^ λ /a^. This angle is important because it is the
limit of the angular resolution of an optical system. For a circular lens, the smallest angle between two points of light which can be resolved is θ = 1.22 λ/ a , where the 1.22 factor depends on the shape of the lens and a is the diameter of the lens.
Waves passing through one of two long, narrow slits will diffract in passing through each slit as described above, but in addition there will be interference with the waves from the other slit. Figure 2 below shows the geometry so you can convince yourself that there is constructive interference causing intensity maxima at points on the screen for which
sin θ = n^ λ d
, n = 0, 1, 2, 3, … (2)
The slits are separated by a distance d. If the distance nS (distance of maxima from n = 0) to the (^) n th maximum is much smaller than the slit to screen distance (^) L, one can also approximate: sin θ = θ = nS/L. In this case, the maxima are equally spaced.
bright
λ
d θ
2λ
bright
bright
bright
bright
0
1
2
1
2
S
S
S
S
2 S
nλ
θ
θ
d
Figure 2
The interference is completely destructive (intensity (^) minima ) where
sin θ =
( n + 21 ) λ d
, n = 0, 1, 2, 3, … (3)
The diffraction pattern that is actually observed from the double slit is the theoretical double slit maximum pattern shown in Figure 3 -- from Equations (2) and (3) -- modulated
Figure 6
A reflector with rulings on it will work in a similar way to the grating described above. In this case, the waves are not incident normal to the surface but instead are incident at a small angle. Light is not reflected from the ruling but from the smooth surfaces between the rulings. Consider the waves that reflect from between the rulings. It is possible for interference to occur. From Figure 7 below, convince yourself that the difference in the lengths of light paths #1 and #2 is d (cos α -cos β) where d is the spacing of the lines. There will be constructive interference for all pairs of angles α and β that satisfy
Ruler (^) d
Figure 7
From Figure 7, the path length difference is seen to be smaller than the ruling separation d. Cos α and cos β are nearly equal to 1 if the angles are small (a few degrees). By using the small angle approximation for the cosine function, we can derive an expression that can be
more easily used to explain the pattern you will observe. If α is expressed in radians, we have for small angles cos α ♠ 1-{1/2} α^2. Substituting this in Equation (5) gives
2
2
2
2 (6)
The last step uses the additional approximation that for small angles, α ♠ tan α. As shown in Figure 8, Sn is the distance from the n th^ order to a line extended from the ruler to the screen.
Wall
n = 2 ORDER n = 1
Ruler
Figure 8
Because the path length difference is so small, this method can be used to measure wavelengths λ that are of order 1000 times smaller than the groove spacing d. One important use of grazing incidence is measuring the wavelength of X-rays ( λ ♠ 10 -8^ cm) by means of an ordinary grating ( d ♠ 10 -4^ cm).
We have provided a diffraction grating, a steel ruler to be used for grazing incidence, and a glass plate containing a variety of single and multiple slits. Figure 9 is a key to the glass plate. The three numbers for each slit or set of slits are, from top to bottom: the number of slits; width of each slit; and separation between slits, respectively (the third number is obviously missing for single slits). The separation is given in points (a point in this instance is equivalent to .0017296 inch). The continuous line varies smoothly both in
o Optical bench o 4 Rod holders o Meterstick o 1 Lens Clamp o Twometerstick o 6” steel ruler with 1/100 divisions o mountings for gratings o Interference and diffraction glass slide o Masking tape o Magnetic holder for diffraction grating o 8.5 x 11” paper o HeNe laser o Diffraction grating/replica grating
This is both quantitative and qualitative. Set up the glass diffraction set slide so that the laser beam is normal to the glass surface. If the glass plate has a magnet attached to it, use the U-shaped metal holder; otherwise, the glass slide can be mounted in a clamp with a rubber cushion -- be careful not to tighten the clamp too much, or you may break the glass slide. Adjust the height of the laser and/or plate so that the incident beam strikes an opening and a diffraction pattern appears on the wall (at least 2 meters away). Observe the patterns of bright and dark spots. Tape a piece of paper to the wall so you can mark their locations. In doing this, include enough information to answer the following questions:
Remove the glass plate and mount the ruler so that the laser light grazes the rulings at a small angle as shown in Figure 8. Aim the laser at the part of the ruler with the smallest spacing between the rulings. You should observe a diffraction pattern on the wall. Is it similar to any you have looked at? Try to explain the separation of the orders (bright spots) in terms of Equation (6) (i.e., how should the distance S (^) n vary with n ?). Also,
compare the separation of these bright spots to the separation of those obtained when you double or halve the spacing between rulings.
Now you are ready to make measurements. Tape a piece of paper to the wall for marking the positions of the spots. Record as many as you can; include the direct beam spot and the spot caused by mirror reflection from the ruler. The direct beam spot is recorded before the ruler is put in place. These are both needed to calculate the angle α. Take care to identify the mirror reflection spot carefully. Record also the spacing of the markings on the ruler in inches or millimeters, and the distance from ruler to wall. Use equation (6) to find λ for laser light using the ruler.