Section 51.9 Diffraction of Light Bootcamp
Subsection 51.9.1 Single-slit Diffraction
Problem 51.9.1. Angles and Position for Diffraction Minima for a Single Slit Diffraction.
Problem 51.9.2. Widths and Positions of Diffraction Through a Single Wide Slit.
Problem 51.9.3. Width of a Single Slit from Width of Central Maximum on Screen.
Problem 51.9.4. Separation of Two Wavelengths in a Single-slit Diffraction.
Problem 51.9.5. Intensity of Light in a Particular Direction behind a Single Slit.
Subsection 51.9.2 Double-slit Diffraction
Problem 51.9.6. Interference Maxima Within Central Peak of a Double-slit Diffraction.
Problem 51.9.7. Combined Diffraction and Interference in a Double-Slit Diffraction.
Problem 51.9.8. Separation of Slits from Number of Interference Peaks within Central Maximum.
Subsection 51.9.3 Diffraction by a Circular Aperture
Problem 51.9.9. Radius of Central Bright Disk in Diffraction through a Lens.
Problem 51.9.10. Applying Raleigh Criterion on Diffraction-limited Image from a Circular Lens.
Problem 51.9.11. Effect of Diffraction on Resolution of an Image of Moon in Yerkes Observatory.
Problem 51.9.12. Distance Two Objects can be Moved and Still Resolvable by Eye If Diffraction-Limited.
Subsection 51.9.4 Diffraction Grating
Problem 51.9.13. Wavelength from Direction of First-order Peak in a Diffraction Grating.
Problem 51.9.14. Spacing Between Slits in a Diffraction Grating from the Direction of First Order Peaks.
Problem 51.9.15. Number of Lines in a Transmission Diffraction Grating from Angle of Second Principal Maximum.
Problem 51.9.16. Separation of Light of Different Wavelengths By a Diffraction Grating.
Problem 51.9.17. Resolving the Sodium Doublet By Diffraction Grating.
Problem 51.9.18. Determine if a Diffraction Grating can Resolve Mercury Yellow-Orange Doublet.
Problem 51.9.19. Resolving Mercury Doublet by a Powerful Diffraction Grating.
Problem 51.9.20. Resolving Power and Dispersion of a Transmission Grating.
Subsection 51.9.5 Miscellaneous
Problem 51.9.21. Wavelength from Diffraction Overlaps of Two Wavelengths.
Equate the sines of the angles of the two conditions.
\(293.3\:\textrm{nm}\text{.}\)
Equating the angles is the same as equating the sines of those angles. Therefore, we will get the following condition from the given data.
Problem 51.9.22. General Formula for Number of Interference Peaks in Central Maximum of Diffraction.
First find half width or \(m^\prime=1\) minimum of the central peak of diffraction, and, then find the maximum interference order for that angle.
\(2p+1\text{.}\)
The half width of the central peak of the diffraction pattern gives
Within this angle the maximum constructive interference order will be
The total number of constructive interference max will be
Problem 51.9.23. Angular Width of Central Peak when Instrument Immersed in Water.
Red light (wavelength 632.8 nm in air) from a helium-neon laser is incident on a single slit of width 0.05 mm. The entire apparatus is immersed in water of refractive index \(\frac{4}{3}\text{.}\) Determine the angular width of the central peak.
Wavelength wil lbe different in water.
\(0.19\:\textrm{rad}\text{.}\)
The wavelength in water, \(\lambda = \lambda_0/n = 474.6\) nm. The angular width will be obtained from twice the angle for \(m=1\) diffraction minimum.
Problem 51.9.24. Widening of the Central Spot of a Laser Light with Increasing Distance.
A light ray of wavelength 461.9 nm emerges from a 2 mm circular aperture of a krypton ion laser. Due to diffraction the beam expands as it moves out. How large is the central bright spot at (a) 1 m, (b) 1 km, (c) 1000 km, and (d) at the surface of the Moon at a distance of 400,000 km from the Earth.
Find angular width in radians first, then multiply it by distance.
(a) \(0.28\: \textrm{mm}\text{,}\) (b) \(280\: \textrm{mm}\text{,}\) (c) \(280\: \textrm{m}\text{,}\) (d) \(112\: \textrm{km}\text{.}\)
We start with the angular width calculation. \[ \Delta \theta = 1.22 \dfrac{\lambda}{D} = 1.22\: \dfrac{ 461.9\:\textrm{nm}}{2\: \textrm{mm}} = 0.00028\:\textrm{rad}. \] Using \(L\Delta \theta\) we find the diameter of the beam at different \(L\)'s.
Problem 51.9.25. Aperture Diameter of the Telescope of a Spy Satellite.
A spy satellite is reputed to be able to resolve objects 10 cm apart while operating 200 km above the surface of the Earth. What is the diameter of the aperture of the telescope if the resolution is only limited by the diffraction effects? Use 550 nm for light.
At the Raleigh criterion, angle of separation will equal width of the Airy's disk.
\(1.34\text{ m}\text{.}\)
We can use the same setup as we used for resolving objects on the moon.

Here, we want the angular separation, \(\theta\approx y/x \) to be greater than the angular width of the Airy's disk, namely, \(\theta_R=1.22\lambda/D\text{.}\) Therefore, we get at-the-Raleigh-criterion to be
Therefore,