Compton Collision: Photon & Electron 180° Scatter, 30keV Energy

  • Thread starter Thread starter Quelsita
  • Start date Start date
  • Tags Tags
    Collision
Click For Summary
SUMMARY

The discussion focuses on the Compton collision between a photon and an electron, specifically analyzing a scenario where the photon has an initial energy of 30 keV and both particles scatter symmetrically at 180°. The Compton wavelength formula, Δλ = (h/mec)(1 - cos(θ)), is utilized to calculate the final energies of the photon and electron. The conservation of energy principle is emphasized, stating that the energy lost by the photon equals the energy gained by the electron. The participants debate the correct application of the Compton wavelength and energy conversion methods.

PREREQUISITES
  • Understanding of Compton scattering principles
  • Familiarity with the Compton wavelength formula
  • Knowledge of energy conservation in particle physics
  • Basic grasp of photon and electron interactions
NEXT STEPS
  • Study the derivation of the Compton wavelength formula
  • Learn about energy conservation in particle collisions
  • Explore the relationship between wavelength and energy in photons
  • Investigate advanced applications of Compton scattering in experimental physics
USEFUL FOR

Physics students, researchers in particle physics, and professionals working with photon-electron interactions will benefit from this discussion.

Quelsita
Messages
41
Reaction score
0
Suppose that after a Compton collision between a photon and electron initially at rest, the electron and photon emerge symmetrically (in equal and opposite angles).
If the initial energy of the photon=30 keV, a) what is the angle that corresponds to such scattering? and b) what is the final photon energy? c) final electron energy?

1. If the angle of deflection is symmetric, then theta=180?

2. since we know theta, we can use
(delta)lambda=(h/mec)(1-cos(theta))
where =(h/mec) is the compton wavelength=0.02426A
which can be rearranged
hc/(delta)E=(0.02426A)(1-cos(theta))
and plug in theta and the Eiphoton to find the final energy.

3. Due to conservation of energy the total energy lost for the photon must equal that of the energy gained by the electron and we know Eiphoton and Efphoton this would equal (delta)Eelectron.

Is this correct?
 
Physics news on Phys.org
Hi Quelsita,

Quelsita said:
Suppose that after a Compton collision between a photon and electron initially at rest, the electron and photon emerge symmetrically (in equal and opposite angles).
If the initial energy of the photon=30 keV, a) what is the angle that corresponds to such scattering? and b) what is the final photon energy? c) final electron energy?

1. If the angle of deflection is symmetric, then theta=180?

2. since we know theta, we can use
(delta)lambda=(h/mec)(1-cos(theta))
where =(h/mec) is the compton wavelength=0.02426A
which can be rearranged
hc/(delta)E=(0.02426A)(1-cos(theta))

I don't believe this is correct; because

[tex] \Delta \lambda \neq \frac{hc}{\Delta E}[/tex]

I would suggest finding the final wavelength (not using the [itex]\Delta[/itex] form) and then converting that to energy.
 

Similar threads

  • · Replies 9 ·
Replies
9
Views
1K
  • · Replies 10 ·
Replies
10
Views
2K
Replies
13
Views
2K
Replies
8
Views
2K
  • · Replies 9 ·
Replies
9
Views
3K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 3 ·
Replies
3
Views
3K
  • · Replies 2 ·
Replies
2
Views
2K
Replies
55
Views
6K
Replies
1
Views
2K