Change in the energy of photon due to recoil of the nucleus

In summary, the conversation discusses the problem of finding the energy of a photon based on the conservation of linear momentum and kinetic energy. The solution involves solving a quadratic equation and making approximations to avoid dealing with a large number of significant figures.
  • #1
Pushoam
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Homework Statement


upload_2017-12-22_18-50-7.png


Homework Equations

The Attempt at a Solution



Since energy of photon is very low compared to the rest mass energy of the nucleus, I consider non – relativistic calculation.

Conservation of linear momentum gives : momentum of nucleus = momentum of photon = p...(1)

Conservation of kinetic energy gives : ## \frac { p^2 c^2}{2mc^2} + pc = 14.4keV ## ...(2)

Solving the above equation gives,

pc = 14.39999806 keV, m = 57 ## m_p ##

So, the energy of the photon gets reduced by 2m eV. Is this correct?
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  • #2
Your work looks correct. Notice how your method of solving the equation requires keeping a large number of significant figures. There are ways to avoid this.

For example, let ##E = pc## and let ##E_0 = 14.4## kev. So your equation (2) is ##\frac{E^2}{2mc^2} +E = E_0##. Solve this quadratic equation symbolically for ##E##. Then make an approximation before plugging in numbers using the fact that ##E_0 << mc^2##.

Or, rearrange (2) to get ##E_0 - E = \frac{E^2}{2mc^2}##. Since ##E## will be close to ##E_0##, you can let ##E = E_0## on the right hand side to obtain a good approximation for ##E_0 - E##.
 
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  • #3
TSny said:
Your work looks correct. Notice how your method of solving the equation requires keeping a large number of significant figures. There are ways to avoid this.

For example, let ##E = pc## and let ##E_0 = 14.4## kev. So your equation (2) is ##\frac{E^2}{2mc^2} +E = E_0##. Solve this quadratic equation symbolically for ##E##. Then make an approximation before plugging in numbers using the fact that ##E_0 << mc^2##.

Or, rearrange (2) to get ##E_0 - E = \frac{E^2}{2mc^2}##. Since ##E## will be close to ##E_0##, you can let ##E = E_0## on the right hand side to obtain a good approximation for ##E_0 - E##.

Thanks for the insights. It's easy and clear.
 

Related to Change in the energy of photon due to recoil of the nucleus

1. How does the recoil of a nucleus affect the energy of a photon?

The recoil of a nucleus can cause a change in the energy of a photon through the process of Compton scattering. This occurs when a high energy photon interacts with an atom or nucleus and transfers some of its energy to the particle, causing it to recoil. This change in momentum results in a decrease in the energy of the photon.

2. Can the energy of a photon be completely transferred to a recoiling nucleus?

No, the energy transfer between a photon and a recoiling nucleus is not 100% efficient. Some energy will always be lost to other forms, such as heat or sound, during the scattering process. However, in most cases, the change in the energy of the photon is negligible compared to the energy of the recoiling nucleus.

3. How does the mass of the nucleus affect the change in energy of a photon due to recoil?

The change in energy of a photon due to recoil is directly proportional to the mass of the recoiling nucleus. This means that a heavier nucleus will cause a larger change in the energy of the photon compared to a lighter nucleus, assuming the same initial energy of the photon.

4. Can the energy of a photon be increased through recoil of the nucleus?

No, the energy of a photon can only decrease due to recoil of the nucleus. This is because the recoil process involves an energy transfer from the photon to the nucleus, resulting in a decrease in the energy of the photon.

5. Is the change in energy of a photon due to recoil significant in everyday life?

In most cases, the change in energy of a photon due to recoil is very small and not noticeable in everyday life. However, it plays a crucial role in understanding the behavior of particles and electromagnetic radiation at the atomic level, and is essential in fields such as nuclear physics and astrophysics.

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