The Compton Effect: Find the angles of scattered photon and electron

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SUMMARY

The discussion focuses on solving a Compton scattering problem involving a photon with an energy of 120 keV and a recoiling electron with an energy of 40 keV. The participant successfully calculated the wavelength of the incident photon as 7.75E-12 m using the equation λ = h/P, where P is the momentum derived from the total energy before scattering. The participant encountered difficulties in calculating the angles of the scattered photon and electron due to the electron's kinetic energy being less than its rest mass energy. The solution emphasizes the importance of using electron volts for energy calculations and incorporating factors of c to simplify momentum calculations.

PREREQUISITES
  • Understanding of Compton scattering principles
  • Familiarity with photon and electron energy-momentum relationships
  • Knowledge of conservation of momentum and energy in particle physics
  • Proficiency in unit conversions, particularly between joules and electron volts
NEXT STEPS
  • Study the derivation of the Compton wavelength shift formula
  • Learn about relativistic momentum and energy equations for particles
  • Explore the implications of energy conservation in particle interactions
  • Investigate the significance of using natural units in high-energy physics calculations
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Physics students, educators, and researchers interested in particle physics, specifically those studying photon-electron interactions and Compton scattering phenomena.

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Homework Statement



In the Compton scattering event seen in the figure, the scattered photon has an energy of 120 keV and the recoiling electron has an energy of 40 keV.

Find:

a) The wavelength of the incident photon
b) The angle θ at which the photon is scattered
c) The recoil angle ϕ of the electron

http://img11.imageshack.us/img11/9245/328q.jpg

Homework Equations



For photons:


P=E/c=hf/c=h/λ

h=6.626E-34 Js


For electron:


P=mv/√(1-v^2/c^2)

E=mc^2/√(1-v^2/c^2)

E=√(P^2c^2+m^2c^4)


Conservation of momentum and energy:


Pbefore=Pafter

Ebefore=Eafter


The Attempt at a Solution



I solved part (a) as follows:

Ebefore=Eafter

--> Ebefore=40keV+120keV=160keV=2.563E-14J

P=E/c=(2.563E-14J)/(2.998E8m/s)=8.55E-23 kgm/s

P=h/λ ---> λ=h/P=(6.626E-34Js)/(8.55E-23 kgm/s)=7.75E-12m


I have an idea on how to solve parts (b) and (c). I would simply calculate the momentum of the scattered photon and the electron, and then use conservation of momentum in the x and y directions, and conservation of energy.

Scattered photon:

P'=E'/c=(1.922E-14J)/(2.998E8m/s)=6.412E-23kgm/s

Recoiling electron:

E=√(P^2c^2+m^2c^4)

6.408E-15J=√(P^2(2.998E8m/s)^2+(9.109E-31kg)^2(2.998E8m/s)^4)


This is where I get stuck. I cannot solve for "P" because it would create a negative under the square root.

After observing the givens, I found that this is because the energy of the electron is given as 40keV which is less than the rest mass energy of an electron of 511keV. Is it possible for an electron to have a total energy less than its rest mass energy? How would you solve for this? Thanks!
 
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The energy you are given is the kinetic energy (call it K). So you have E = K + mc^2.

Oh, and stick to electron volts in a calculation like this. There is no reason to fool around with kilograms.
 
It's useful to know that ##hc = 1240\text{ nm eV}##. Don't plug in a value for ##c##. Pull the factors of ##c## into the units. For example, the 120-keV photon has a momentum of 120 keV/c, and the mass of the electron is 511 keV/c2.

Sometimes, you'll want to introduce factors of ##c## to make formulas work out more easily. For instance, you found ##E_\text{before} = 160\text{ keV}##. The momentum of the photon is then ##p = 160\text{ keV/}c##. To find its wavelength, you used ##\lambda = h/p##. If you throw in some factors of ##c##, everything works out nicely:
$$ \lambda = \frac{h}{p} = \frac{hc}{pc} = \frac{1240\text{ nm eV}}{160\text{ keV}} = 7.75\times 10^{-3}\text{ nm}.$$ It's worth taking a little time to learn how to work in these units. It'll save you from a lot of tedious unit conversions.
 

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