Electron shell transitions between levels - conceptual question

In summary, the probability of an electron transitioning from the n = 4 to n = 3 shell is different from the electron going from n = 2 to n = 1. This is because the transition from n = 2 to n = 1 is the most likely and strongest observed transition, known as the K-alpha line. This is due to the high energy needed to knock electrons out of the higher levels and the competing Auger effect with outershell electrons.
  • #1
jumbogala
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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?

Homework Equations





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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  • #2
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.
 

1. What are electron shell transitions between levels?

Electron shell transitions refer to the movement of electrons from one energy level to another within an atom. These transitions occur when an electron gains or loses energy, causing it to move to a different orbit around the nucleus.

2. What is the significance of electron shell transitions?

Electron shell transitions play a crucial role in the behavior and properties of atoms. They are responsible for the absorption and emission of light, the formation of chemical bonds, and the generation of electricity in electronic devices.

3. How are electron shell transitions between levels represented?

Electron shell transitions are often represented using the Bohr model of the atom, which shows the different energy levels as concentric circles around the nucleus. The movement of electrons between these levels is depicted as arrows.

4. What determines the energy levels of electrons in an atom?

The energy levels of electrons in an atom are determined by the quantum numbers associated with each electron. These quantum numbers describe the position, energy, and spin of an electron in an atom.

5. Can electron shell transitions occur spontaneously?

Yes, electron shell transitions can occur spontaneously when an electron gains or loses energy. However, these transitions can also be induced by external factors such as heat, light, or electric fields.

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