00:01
Hi there, so for this problem we are told that although we have discussed single sleet diffraction only for a sleet, a similar result holds when light bends around a straight, thin object, such an strad of herd.
00:17
In that case, a is the width of the strat.
00:20
So, from actual laboratory measurements on a human herd, it was found that when a beam of light of a wavelength that is given, and that wavelength is equal to 632 .8 nanometers, nanometers, was shown on a single strut of herd, and the defrapted line was view on a screen, that it is at a distance of the word going to call capital l, that is equal to 1 .25 meters.
01:01
The first dark fringes on either side of the central bright spot were 5 .22 centimeters apart.
01:12
So we're going to call this the distance, yes, we're going to call this the distance y.
01:27
That is going to be a value in this case of 5 .22 centimeters.
01:41
So that is the same as 5 .22 times 10 to the minus 2 meters.
01:59
So for this disruption problem, they tell us that it is equivalent to the disruption.
02:12
Oh, sorry.
02:13
Well, the question is, how thick was this strut of herd? so we need to calculate the value of a.
02:22
Now, again, we know that for this problem, they tell us that it is equivalent to the disruption of a single slit, which is explained by the following equation.
02:31
That is that the thickness of the herd is equal to the function sign of theta, and then this is equal to plus or minus the order m times the wavelength.
02:50
Now, we can see that the disruption angle is missing in this case, but we can find it by trigonometry, where l is the distance of the strand of the herd to the observation screen, and y is the perpendicular distance to the first minimum intensity.
03:09
So remember that those values are given, l is equal to 1 .25 meters, and y is 5 .22 times 10 to the minus 2 meters, or 5 .22 centimeters.
03:19
Meters.
03:20
So we know that they are related by the tangent of theta by trigonometry.
03:25
That will be y divided by lt...