Compton Scattering (Back-Scattering)

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SUMMARY

The discussion focuses on Compton scattering, specifically the scenario where high-energy gamma rays scatter off electrons at a scattering angle of θ = 180 degrees. It is established that the detected scattered photons will have an energy of 0.26 MeV, regardless of the initial gamma ray energy, provided it exceeds the rest-mass energy of an electron. The relevant equation used is Δλ = (2h/(me)c), which leads to the conclusion that ΔE = 0.26 MeV when applying the appropriate assumptions about the wavelengths involved.

PREREQUISITES
  • Understanding of Compton scattering principles
  • Familiarity with energy-momentum relations in particle physics
  • Knowledge of the Planck constant (h) and electron rest mass (me)
  • Basic proficiency in algebra and calculus for manipulating equations
NEXT STEPS
  • Study the derivation of the Compton scattering formula
  • Learn about the implications of scattering angles in particle physics
  • Explore the concept of energy conservation in high-energy physics
  • Investigate applications of Compton scattering in medical imaging techniques
USEFUL FOR

This discussion is beneficial for physics students, particularly those studying particle physics or quantum mechanics, as well as educators and researchers interested in the applications of Compton scattering in experimental setups.

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Homework Statement



Consider the situation where high-energy gamma rays are striking a detector after
scattering off of the electrons in the material surrounding a detector. Show that if
the gamma rays are perfectly back-scattered by the material, such that the scattering
angle is θ = 180 degrees, then the detected scattered photons will all have essentially
the same energy of 0.26 MeV, independent of the precise energy of the incident gamma
rays as long as the incident gamma ray energy is much larger than the rest-mass energy
of an electron.

Homework Equations



\lambdafinal - \lambdainitial = \frac{h}{(me)c} (1 - cos\theta)

The Attempt at a Solution



Well for \theta = 180 degrees, the compton scattering eqn becomes
\lambdafinal - \lambdainitial = \frac{2h}{(me)c}.
I'm confused about where to go from here since \lambdafinal - \lambdainitial needs to be proven it is 0, and also that \lambdafinal = \lambdainitial = 0.26MeV.
I have a feeling I need to to use the binomial expansion somewhere since it is saying that the incident gamma ray energy has to be much larger than the rest-mass energy
of an electron. Can someone push me in the right direction?
 
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Hi person in the same PHYS242 class at Queen's I'm in.

You're on the right track. Just convert the equation you have right now to an energy equation using ∆E and you will get ∆E = 1/2mec2. Solve this and you will get 0.26 MeV with the assumptions that your initial lambda is much much smaller than your final lambda (and therefore your ∆E can be considered a final E rather than delta).
 

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