The Single Slit

To understand this, you need to know how to analyze the grating by means of phasors, because a grating with N slits of spacing d becomes a single slit as N --> ¥ and d --> 0 in such a way that the product Nd is the slit width, a. Nd = a. And if infinity and zero bother you, rest assured that if you had 105 slits in a millimeter width, you would not be able to tell the difference between the pattern obtained by shining light on this grating and the pattern obtained by shining the light on a 1 millimeter single slit.

We showed that the first zero for a grating occurs when the phasor diagram becomes a polygon, and we found that dsinq = l /N, or Ndsinq = l . So for a single slit, the phasor diagram is a circle at the first zero, and it occurs when asinq = l , where a is the slit width.

Then as you increase q you encounter a small relative maximum, then eventually another zero when the phasor diagram winds up on itself to form two circles- the total phase change from one side of the slit to the other is 4p radians, and asinq = 2l .

So in general asinq = ml for minima with a single slit. The same is true for grating minima, replacing a with Nd. But usually no one is concerned with these in a grating; we are concerned with the big maxima. These don't occur with a single slit (just the central maximum is large), nor would they occur with the grating of 105 slits in a millimeter. (Why?)

The central maximum phasor diagram is just a straight line. Then move a little away from center and we have an arc (grating with 105 tiny straight segments or single slit with a true arc- no one can tell the difference). The arc length is the sum of the magnitudes of the E vectors, and this remains unchanged. The dotted line is the total E for that particular point. To calculate E, note that radius R has units of E, and if we bisect f , we hit the midpoint of the E vector. Hence E = 2Rsin(f /2). The arc length is the central maximum E (call it Em), and f in radians is arc length/radius. So R = Em/f . Substituting, we have E = (2Em/f )sin(f /2). Intensity is proportional to the square of E, so I=Imsin2(f /2)/(f /2)2. It is important to remember that f in the denominator must be in radians.


Note also that
f is the phase angle between the first an last ray,
so
f = (2p /l )asinq , or for the grating replace a with Nd.

Moving still farther along away from the central maximum, we come to the first zero, then a small maximum at  f = 8.99 radians, a second zero (two circles superimposed) at f = 2p rad, etc. The first ray is on the bottom, the last ray has the arrow (>), and the dotted line is the total E:


(I did these by eye. The m=2 circle should have half the diameter as the m=1, and I see that I made it too big.)

Now to answer the question why the 105 slits in a millimeter does not get out of the above pattern of decline and produce a spectacular maximum, just apply the equation dsinq = ml for m = 1 and d = 1/105 mm = 10-8 m, and you will see that for this to occur, l needs to be less than 10-8 m (x-rays).

Now undulate back to the other waves stuff.

My other main pages:

mechanics
fluids, heat, electricity and magnetism
quantum
index

Comments, questions: fredrick.gram at tri-c.edu  (but use @, not at)