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Physics 251 Spring 1999
Modern Physics
Homework Assignment # 4, Due (in class) Monday February 15
Reading Ahead: Read Krane, Chapter 5, week of Feb. 7 Problem Assignment: Important! There are three formulas for kinetic energy:
A Eq.(1.1) KE = $\frac{1}{2}mv^2=\frac{p^2}{2m}$ usual classical formula
B Eq.(2.36) KE = $\sqrt{(mc^2)^2 +(pc)^2}-mc^2$ Einstein formula; general
C Eq.(2.42) KE = pc extreme relativistic or massless case
Case A is an approximation which is accurate when v is small compared with c or equivalently when KE is small compared with mc2, which is very often accurate. In each of the problems below you must specify which (A,B,C) of these three formulas is appropriate. It is significant that in all three cases the velocity v is given by dE/dp. In case B this is equivalent to the formula $p=mv/\sqrt{1-(v/c)^2}.$
1.
Krane, Chapter 4, p.132, #1. Reminder: according to elementary kinetic theory, the average kinetic energy of a particle of mass m in thermal equilibrium is 3kB T/2.
2.
Krane, Chapter 4, p.132, #2.
3.
Krane, Chapter 4, p.132, #3. Reminder: the optimal spatial resolution is approximately the same as the wavelength of the wave used to image the object.
4.
Krane, Chapter 4, p.133, #11. Refer to fig. 4.6 and use it to derive the formula $d \sin \phi=n \lambda$.
5.
Krane, Chapter 4, p.133, #15.
6.
Krane, Chapter 4, p.133, #17.
7.
Krane, Chapter 4, p.134, #26.


 
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Phil Allen
2/8/1999