Energy level transition questions

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SUMMARY

The discussion centers on energy level transitions in hydrogen atoms, specifically the ability of an electron to transition from n = 5 to lower energy levels (n = 4, n = 3, n = 2, and n = 1) by emitting multiple photons. It is established that while an electron can transition through multiple levels, selection rules based on conservation laws dictate which transitions are allowed. The probability of these transitions is influenced by the fine structure constant (α), with single photon transitions being significantly more probable than multiphoton transitions, which are allowed under certain conditions.

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  • Understanding of quantum mechanics principles
  • Familiarity with selection rules in quantum electrodynamics (QED)
  • Knowledge of the fine structure constant (α) and its significance
  • Basic concepts of photon emission and absorption
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  • Research quantum electrodynamics (QED) and its applications
  • Study the implications of selection rules on atomic transitions
  • Explore the fine structure constant (α) and its role in quantum mechanics
  • Investigate multiphoton transitions and their experimental observations
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Masonn
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Say for a simple hydrogen atom, an electron absorbs just the right amount of energy such that it jumps up from energy levels n = 1 to n = 5. When it comes back down, is it possible to say, do n = 5 to n =3 to n = 2 to n =1, releasing 3 photons with their respective specific frequencies/energies? Or is it only able to go from n = 5 to n = 1? And why?

Thanks in advance.

It's not a homework question, it's a question that came out of a classroom discussion.
 
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Emission and absorption of photons from an electron is described by quantum electrodynamics, called QED for short. This is an example of a quantum field theory and to properly describe the transitions in hydrogen would require a lot of background and technology. But we can get some qualitative information out using some information that requires a bit of quantum mechanics knowledge and some intuition.

Basically, the important idea is that the strength of the electromagnetic interaction is proportional to the electric charge, ##e##. The amplitude for a single photon transition is then proportional to ##e##, so the probability of a single photon transition is proportional to ##e^2##. Since the value of the electric charge depends on the system of units that we use, it turns out to be a much simpler to express this in terms of the dimensionless fine structure constant

$$\alpha = \frac{e^2}{4\pi \epsilon_0 \hbar c} \sim \frac{1}{137}.$$

So we can as well say that the probability for the emission of a single photon carries a factor of ##\alpha##.

Now suppose there is a particular transition from n=5 to n=1 that satisfies the angular momentum selection rules that Jolb pointed out. This transition can indeed proceed by the emission of 2 photons, but the probability of this happening is now proportional to ##\alpha^2##, so it is roughly 100 times less likely than the single photon transition. Similarly, the probability for the 3 photon transition will be proportional to ##\alpha^3##, so it is 10000 times less likely than the single photon transition.

Multiphoton transitions have indeed been observed and in fact allow certain transitions that are forbidden from occurring via a single photon transition by the selection rules. An important example is the 2s to 1s transition in hydrogen.
 

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