Kinetic energy of recoil atom in the photoelectric effect

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SUMMARY

The discussion focuses on calculating the kinetic energy of the recoil atom and the emitted photoelectron in the photoelectric effect, emphasizing the importance of accounting for both energies. The relevant equation is Etr (Energy transferred) = hf - EB, where hf represents the photon energy and EB is the binding energy. The derived equations for kinetic energy are EKe- = m(ionized atom)/M(total) * Etr and Ek(atom ionized) = me/M(total) * Etr. Conservation of momentum and energy principles are crucial for accurate calculations in this context.

PREREQUISITES
  • Understanding of the photoelectric effect
  • Familiarity with conservation of momentum and energy principles
  • Knowledge of kinetic energy equations
  • Basic grasp of binding energy concepts
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  • Study the derivation of kinetic energy equations in the context of the photoelectric effect
  • Learn about relativistic effects in particle physics
  • Explore advanced topics in conservation laws in quantum mechanics
  • Review the implications of binding energy on electron emission
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Students studying quantum mechanics, physicists interested in the photoelectric effect, and educators teaching advanced physics concepts.

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Homework Statement


In the photoelectric effect it is generalley assumed that all the energy is given as kinetic energy to the electron while the atom is neglected. Do not neglect the recoil kinetic energy of the atom and calculate the kinetic energy of the photoelectron and the ionized atom and determine their ratio

Note: Etr (Energy transferred) = hf - EB = EKe- + EKM+

Homework Equations



The above equation is relevant. I am not sure which other ones are relevant otherwise. most likely a few relativistic equations Ek = E-E0

The Attempt at a Solution


I already know the solution as it is given in the textbook except the author skipped quite a few steps.

The author gives Eke- = m(ionized atom)/M(total) * Etr and Ek(atom ionized) = me/M(total) * Etr
where m is the mass and Etr is defined above

I don't know how he gets this. I started off doing conservation of momentum:

xdir: h*nu/c = pecos(theta) + pacos(phi)
ydir: 0 = pesin(theta) + pasin(phi)

and it was suggested to me to use the relation p^2/2m and solve for the kinetic energy. I don't think that's correct. I also think solving the above equation won't yield the correct answer since it doesn't incorporate the binding energy and will require conservation of energy. At this point though I am wondering if I am going down the wrong rabbit hole since the author of the textbook just sort of wrote the equation down (when usually there is very strict derivation).

Any help would be appreciated. If clarifications are needed I will do that
 
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Ok, so you have the right idea. You need to apply conservation of momentum and energy to the system before and after the absorption and emission. You don't need to concern yourself with any angles for the momentum.

What do you think the initial energy of the atom and photon system is?
 

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