Electron shell transitions between levels - conceptual question

AI Thread Summary
The probability of electron transitions between energy levels varies, with transitions from n=2 to n=1 generally being more common than those from n=4 to n=3. This is primarily due to the higher energy required to transition from outer shells, making lower energy transitions more likely. The context of these transitions often involves phenomena like X-ray fluorescence, where high-energy photons can displace inner shell electrons, leading to a cascade of lower energy transitions. The n=2 to n=1 transition is particularly notable as it corresponds to the K-alpha line, which is frequently observed. Additionally, outer shell transitions may be influenced by the Auger effect, complicating the overall transition probabilities.
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Homework Statement


Is the probability that an electron transitions from the N to M (n = 4 to n = 3) shell different than the electron going from L to K (n = 2 to n = 1)?

So basically, should I expect to see a lot more transitions from n = 2 to n = 1, than any other type of transition? If so, why?

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The Attempt at a Solution


I'm not really sure why this would be. Perhaps because you need more energy in the first place to knock electrons out of the higher levels? That's just a guess. Can anyone help me out, I'm curious if and why this is true.
 
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What's the context of these transitions? Are you talking about something like X-Ray fluorescence, wherein a high energy photon displaces an inner shell electron, followed by a cascade of electrons falling into lower energy orbitals to make up for the vacancy?

In that case, n=2 to n=1 transition is most likely and the strongest observed transition (K-alpha line), see: http://en.wikipedia.org/wiki/File:XRFScan.jpg

With outershell electrons, there is also a competing effect called the Auger effect.
 
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