Download presentation
Presentation is loading. Please wait.
Published byIsaiah Lins Modified over 9 years ago
1
Quantization of Light Chapter 4
2
Chapter 4 Homework 4.9, 4.15, 4.23, 4.31 Due Monday 2/24
3
This week Lecture today Problems, questions Wednesday Quiz and makeup quizzes Friday –Makeups if you qualify –(Do the relevant HW by Wednesday)
4
Black-body Radiation Does not preferentially absorb or emit any particular frequency Light in thermal equilibrium with surroundings Experimentally realized as “Cavity” radiation
5
Black-Body Spectrum Classically, emission at short wavelengths would be infinite Planck correctly modeled spectrum by assuming E = hf Sharp drop in high-f “photons”
6
Photoelectric Effect Light absorbed by a metal can eject electrons Energy of photoelectrons did not depend on light intensity P/A (Instead, that determined the current) Light frequency determined photoelectron energy
7
Photoelectric Effect Explained by Einstein E = hf – Verified by Millikan slope = h E f –– 0
8
Photoelectric Effect Work function of metal –property of the metal –potential energy of bound electron light carries and delivers energy in hf packets (photons) Light can act as discrete particles, not just continuous waves
9
X rays “Braking radiation” from stopped electrons Electromagnetic radiation hf max = K e = Ve – + V X
10
X rays are Light Uncharged Diffract from crystals
11
Compton Effect X-rays lose energy scattering from electrons Interpreted as elastic scattering conserving momentum hf 1 hf 2
12
Photon Momentum E 2 = (mc 2 ) 2 + (pc) 2 (hf) 2 = (pc) 2 hf = pc p = hf/c p = h(c/ )/c p = h/
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.