Section 53.7 Quantum Nature of Light Bootcamp
Subsection 53.7.1 Photon and Blackbody Radiation
Problem 53.7.1. Number of Photons in a Laser Beam.
Follow the link: Checkpoint 53.3.3.
Problem 53.7.2. Energy of a Photon in He-Ne Laser.
Follow the link: Checkpoint 53.3.6.
Problem 53.7.3. Photons in Sodium Lamp.
Follow the link: Checkpoint 53.3.7.
Problem 53.7.4. Photons in Green Laser.
Follow the link: Checkpoint 53.3.8.
Problem 53.7.5. Comparing Photon Rates in Two Lasers.
Follow the link: Checkpoint 53.3.9.
Problem 53.7.6. Exciting an Electron in Silicon Bandgap.
Follow the link: Checkpoint 53.3.10.
Problem 53.7.7. Absorbing Most Power from the Sun Light.
Follow the link: Checkpoint 53.3.11.
Problem 53.7.8. Sun Radiating as a Blackbody.
Follow the link: Checkpoint 53.3.4.
Problem 53.7.9. Stefan-Boltzman law from Planck's Radiation Law.
Follow the link: Checkpoint 53.3.5.
Problem 53.7.10. Electromagnetic Radiation Emitted by Earth.
Follow the link: Checkpoint 53.3.12.
Problem 53.7.11. Electromagnetic Radiation Emitted by a Heated Tungsten Filament.
Follow the link: Checkpoint 53.3.13.
Problem 53.7.12. Temperature of the Universe from Cosmic Background Radiation.
Follow the link: Checkpoint 53.3.14.
Problem 53.7.13. Power Radiated by Proxima Centauri.
Follow the link: Checkpoint 53.3.15.
Problem 53.7.14. Varying Intensity of Radiation with Temperature.
Follow the link: Checkpoint 53.3.16.
Problem 53.7.15. Varying Peak Wavelength of Radiation with Temperature.
Follow the link: Checkpoint 53.3.17.
Problem 53.7.16. Radiation Emitted by Human Body.
Follow the link: Checkpoint 53.3.18.
Problem 53.7.17. Total Intensity of Cosmic Microwave Background.
Follow the link: Checkpoint 53.3.19.
Subsection 53.7.2 Photoelectric effect
Problem 53.7.18. Speed of Photoelectrons.
Follow the link: Checkpoint 53.4.5.
Problem 53.7.19. Photocurrents from Zinc.
Follow the link: Checkpoint 53.4.6.
Problem 53.7.20. Photoelectric Effect on a Sodium Target.
Follow the link: Checkpoint 53.4.7.
Problem 53.7.21. Photoelectric Effect on a Platinum Target.
Follow the link: Checkpoint 53.4.8.
Problem 53.7.22. Work Function from Photoelectric Effect.
Follow the link: Checkpoint 53.4.9.
Problem 53.7.23. Stopping Potential and Photocurrent in Photoelectric Effect.
Follow the link: Checkpoint 53.4.10.
Problem 53.7.24. Finding the Value of Planck Constant from Photoelectric Effect.
Follow the link: Checkpoint 53.4.11.
Subsection 53.7.3 Compton effect
Problem 53.7.25. Compton scattering of X-ray by electrons.
Follow the link: Checkpoint 53.5.4.
Problem 53.7.26. Compton Shift in X-ray on Graphite Target.
Follow the link: Checkpoint 53.5.5.
Problem 53.7.27. Energy and Momentum of Scattered Electron in Compoton Experiment.
Follow the link: Checkpoint 53.5.6.
Problem 53.7.28. Wavelength of Scattered Photon from a Free-Electron Target.
Follow the link: Checkpoint 53.5.7.
Problem 53.7.29. Energy and Momentum of X-ray Scattered at Right Angle.
Follow the link: Checkpoint 53.5.8.
Problem 53.7.30. Energy and Momentum of Gamma RayScattered at Right Angle.
Follow the link: Checkpoint 53.5.9.
Subsection 53.7.4 Miscellaneous
Problem 53.7.31. Temperature of an Oven from Blackbody Radiation Data TODO.
An oven is heated to a high temperature and the electromagnetic radiation coming out of the oven through a tiny hole in the oven is analyzed for radiance \(R_T(\lambda)\text{,}\) which is the power content per unit wavelength range per unit cross-section area of the hole. The data obtained at five wavelengths are:
(a) Plot \(R_T\) versus \(\lambda\text{.}\) (b) From the data find the temperature of the oven. (c) Find the total power radiated per unit area of cross-section of the hole.
Problem 53.7.32. Colision of a Photon with a Free Electron TODO.
A photon of energy \(hf\) collides head-on with a nearly free electron at rest. Let \(E_0\) be the rest energy of an electron. Show that the kinetic energy of the recoiled electron is given by
Problem 53.7.33. Percentage of Energy that Photon can Transfer in Compton Scattering TODO.
(a) Prove that in the Compton scattering, a photon cannot transfer all of its energy to an electron. (b) Is there a maximum percentage of energy that a photon can transfer to an electron at rest? If so, what is it? If not, why not?
Problem 53.7.34. Formula for Wavelength for Maximum Blackbody Radiation TODO.
(a) Treating \(R_T(\lambda)\) as a function of \(\lambda\text{,}\) prove that the maximum of the radiance occurs at a wavelength \(\lambda_{\textrm{max}}\) whose product with temperature is a constant.
(b) Find the value of the constant.