Stimulated emission per second per atom?

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SUMMARY

This discussion focuses on calculating the probability per atom and second for stimulated emission from the 2p to 1s state of hydrogen in a plasma at 4500 ºC. The relevant equations include Planck's radiation law and Einstein coefficients, specifically using the lifetime of the 2p state (1.6 ns) to derive the stimulated emission rate. The key insight is that the product of the Einstein coefficient B and the frequency density from Planck's law yields the desired unit of s-1 for the rate of stimulated emission per atom.

PREREQUISITES
  • Understanding of Planck's radiation law
  • Familiarity with Einstein coefficients in quantum mechanics
  • Knowledge of the Bohr model of the hydrogen atom
  • Basic concepts of plasma physics
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  • Learn about the implications of Planck's radiation law in different temperature regimes
  • Explore the Bohr model and its relevance to atomic transitions
  • Investigate the mathematical formulation of stimulated emission and its applications in laser physics
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Students and researchers in physics, particularly those focusing on atomic physics, plasma physics, and quantum mechanics, will benefit from this discussion.

Philip Land
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Homework Statement


We are investigating hydrogen in a plasma with the temperature 4500 ºC. Calculate the probability per atom and second for stimulated emission from 2p to 1s if the lifetime of 2p is 1.6 ns

Homework Equations


Planks radiation law:
##\rho (f) = \frac{8* \pi h}{c^3}\frac{1}{e^{\frac{hf}{kT}} -1}## (1)

Einstein coefficients :
##A=\frac{8 \pi f^3 h}{c^3} B## (2)

The Attempt at a Solution


I can take the inverse of the life-time to get A. Then I can just solve for B. Using that ##\lambda = 1.251*10^{-7}## (which I looked up).

I seek a unit that is per second per atom. Which I can't really get my head around.

I try to play around with the frequency density (1) but fail to find per atom. When I get "per atom" I can just multiply that with A.

Any tipps here?
 
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Finding B as you describe is fine. Planck’s radiation law which you show will also be necessary. You are almost there. What is B good for? How is it used? Do you perhaps see it in a differential equation relating the rate of stimulated emission to the upper state population density? What must be the units of the coefficient on the upper state population density?
 
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Cutter Ketch said:
Finding B as you describe is fine. Planck’s radiation law which you show will also be necessary. You are almost there. What is B good for? How is it used? Do you perhaps see it in a differential equation relating the rate of stimulated emission to the upper state population density? What must be the units of the coefficient on the upper state population density?
Thank you!

I figured out how to solve this. I wanted the unit ##s^-1##. (Which also A gave so I'm not sure I undertand the theory here). But evaluating the units I see that if I multiply B (which I can get if I know ##f##, which I can get from the Bohr model) by the frequency density I get the rate of stimulated emission per atom per second. So ##B * \rho ## is what I was seeking.
 
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