Calculating Final Photon Energy in Inverse Compton Scattering

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SUMMARY

The discussion focuses on calculating the final energy of a photon in inverse Compton scattering, specifically with an initial X-ray energy of Eγ=100 keV and a relativistic electron energy of Ee=100 GeV. The participant attempts to apply conservation of energy and momentum principles but struggles with the complexity of the problem, particularly in determining the relationship between the angles of the incoming and outgoing particles. The conservation equations presented include Eγ + Ee = E'γ + E'e, highlighting the need to account for both energy and momentum components in the solution.

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  • Understanding of inverse Compton scattering principles
  • Familiarity with conservation of energy and momentum in relativistic contexts
  • Knowledge of relativistic energy equations, including E=mc²
  • Basic proficiency in manipulating equations involving photons and electrons
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  • Study the derivation of the inverse Compton scattering formula
  • Learn how to apply conservation laws in relativistic collisions
  • Explore the relationship between scattering angles and energy transfer in particle physics
  • Review examples of similar problems involving photons and relativistic particles
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Homework Statement



Suppose that an X ray has initial energy Eγ=100keV, and the incident (relativistic) electron has energy Ee=100GeV. Compute the final energy of the photon E'γ assuming the final direction of the photon makes an angle θ=Π with the initial direction.

For solving this problem, use the conservation of energy and each component of the momentum.

Homework Equations



None yet - still setting up problem.

The Attempt at a Solution



I am familiar with normal Compton scattering where a photon interacts with a rest electron, but not the inverse.

Maybe this works a certain way, but here is how I see it and what I want to verify.

I picture relativistic electron moving along the x-axis and getting rear ended by the x ray. The resulting gamma ray goes the other direction, still along x, and the electron continues moving along the x-axis with much less energy and momentum. At least that's what I hope because it makes the problem easier - although I am pretty sure that is wrong.:redface:

So a more realistic view is the electron is coming in at an angle and leave at an angle with the resulting photon going the opposite direction but still along the x-axis.

Is there a relationship between the initial angle and the resulting angle of the electron? I have it half setup but end up with way too many unknowns.
 
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I worked a little more on this one and came up with the following. Since it is a sketch I just threw the equations on the attachment as well.

This diagram makes sense to me.

Any ideas?
 

Attachments

  • inverse compton scattering.jpg
    inverse compton scattering.jpg
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I've narrowed the question down some and now it's more conceptual. I am missing something.

So I have the energy of the x-ray, and the energy of the relativistic electron. I don't know the final energy of the produced gamma ray. My equation is this for conservation of energy.

[tex]E_{\gamma} + E_{e} = E^{'}_{\gamma} +E^{'}_{e}[/tex]

[tex]h\frac{c}{\lambda}+\gamma m_{e} c^{2} = h\frac{c}{\lambda'}+m_{e} c^{2}[/tex]

I also know mec2 since those are both known values. Since energy is conserved couldn't I just do this?


[tex]h\frac{c}{\lambda}+\gamma m_{e} c^{2} - m_{e} c^{2} = h\frac{c}{\lambda'}[/tex]

The question states I need to use both energy and both components of momentum to solve.

What am I missing?
 

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