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

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In summary, the conversation discusses a Compton collision between a photon and electron at rest, where the resulting electron and photon emerge symmetrically in equal and opposite angles. Given an initial photon energy of 30 keV, the conversation seeks to determine the corresponding scattering angle, as well as the final photon and electron energies. It is suggested to use the equation (delta)lambda=(h/mec)(1-cos(theta)) and then convert the resulting wavelength to energy. However, the correctness of this approach is questioned and an alternative suggestion is made.
  • #1
Quelsita
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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?
 
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  • #2
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.
 
  • #3


Your understanding is correct. In a Compton collision, the angle of deflection is determined by the equation (delta)lambda=(h/mec)(1-cos(theta)), where (delta)lambda is the change in wavelength, h is Planck's constant, me is the mass of the electron, and c is the speed of light. This equation can be rearranged to solve for the angle theta, which in this case is 180 degrees.

Using this value of theta, we can calculate the final energy of the photon using the equation E=hc/(delta)lambda. The initial energy of the photon is given as 30 keV, so we can plug in the values and solve for the final energy, which would be approximately 29.97 keV.

As you mentioned, due to conservation of energy, the energy lost by the photon must equal the energy gained by the electron. Therefore, the final energy of the electron would also be approximately 29.97 keV. This is because the initial energy of the electron was at rest, so all of the energy gained from the photon is transferred to the electron.

Overall, your understanding and approach to this problem is correct. Keep up the good work!
 

1. What is the Compton Collision and why is it important?

The Compton Collision is a phenomenon in which a photon and an electron collide at a 180° angle, resulting in the scattering of the photon and the recoil of the electron. It is important because it provides evidence for the existence of both particles and helps us understand their properties and interactions.

2. How does the energy of the photon affect the Compton Collision?

The energy of the photon is directly related to the amount of energy transferred to the electron during the Compton Collision. A higher energy photon will transfer more energy to the electron, resulting in a greater recoil and a larger scattering angle.

3. What is the significance of the 30keV energy in the Compton Collision?

The 30keV energy refers to the energy of the photon in the Compton Collision. This specific energy was chosen because it is in the range of X-rays, which are commonly used in medical imaging and other applications. Studying the Compton Collision at this energy can help us understand how X-rays interact with matter.

4. How does the scattering angle of the photon change with increasing electron recoil?

The scattering angle of the photon increases as the electron recoil increases. This is because a greater amount of energy is transferred from the photon to the electron, causing the electron to move at a higher speed and resulting in a larger scattering angle.

5. What other factors can affect the Compton Collision besides energy?

The Compton Collision can also be affected by the material of the target, the angle of incidence of the photon, and the mass of the electron. These factors can influence the amount of energy transferred and the resulting scattering angle.

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