Nuclear Shell model, how do we know energy levels?

In summary, the conversation discusses the use of quantum numbers l and n to classify shell model energy levels and the concept of magic numbers in nuclear physics. The use of mean field theory and potential models is also mentioned as a way to calculate these energy levels. It is noted that larger magic numbers are more difficult to calculate due to adjustments in the potential.
  • #1
UniPhysics90
16
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One of my 'course aims' is to be able to classify the shell model energy levels in terms of quantum numbers l and n and explain how magic numbers arise.

I'm using this to help to understand it as well as lecture notes. http://hyperphysics.phy-astr.gsu.edu/hbase/nuclear/shell.html

I know that l is the 'letter' in the energy states (s=0, p=1 etc) and n is the number (as in lowest s level is 1, second lowest 2 etc).

The energy levels are split into groups, but how are these groups actually decided? Is there some formula which predicts this? (I'm on about both the energy levels before and after spin orbit coupling)

Thanks
 
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  • #2
Quantum mechanics, solving the atom.
 
  • #3
It's basically the same process as in atomic physics. In atomic physics you have all electrons moving in a central potential caused by the nucleus. This causes the different quantum levels to appear.

In nuclear physics you can do the same. It is possible to use mean field theory on all the nucleons. This means that every nucleon moves in a potential caused by all the other nucleons. Averaging this for every nucleon gives a very different, but still central, potential problem. This can be solved assuming some shapes for the potential like Woods Saxon potential or square well. Again some quantum levels appear for the nucleons. That's why it is called the nuclear shell model.
 
  • #4
Thanks guys, I guess I'll just learn the splitting of the first few levels so I can draw the diagram if required.
 
  • #5
The first levels are easily calculated using simple potential models. The larger magic number are harder, because for more nucleons the potential gets adjusted and so do the magic numbers if you use a simple harmonic oscillator for example.
 

1. What is the Nuclear Shell Model?

The Nuclear Shell Model is a theoretical framework used to describe the structure of atomic nuclei. It is based on the idea that protons and neutrons inside the nucleus occupy specific energy levels, similar to electrons in an atom. These energy levels are determined by the nuclear force that holds the nucleus together.

2. How do we know about the energy levels in the Nuclear Shell Model?

The energy levels in the Nuclear Shell Model are determined through experiments such as nuclear spectroscopy. This involves studying the energy and momentum of particles emitted from the nucleus, which can provide information about the energy levels and their spacing.

3. What is the evidence for the existence of energy levels in the nucleus?

One of the main pieces of evidence for the existence of energy levels in the nucleus is the observation of discrete energy levels in the spectrum of emitted particles. This indicates that the energy levels are quantized, just like in the atomic shell model. Additionally, nuclear reactions and decay processes also support the idea of energy levels in the nucleus.

4. How do the energy levels in the Nuclear Shell Model affect nuclear stability?

The energy levels in the Nuclear Shell Model play a crucial role in determining the stability of a nucleus. Nuclei with filled energy levels or with a specific number of protons and neutrons on certain energy levels tend to be more stable. This explains why certain elements are more stable than others and why some isotopes are more stable than others.

5. Can the Nuclear Shell Model be applied to all nuclei?

The Nuclear Shell Model is a useful framework for understanding the structure of most nuclei, but it does have its limitations. It works best for nuclei with a closed shell structure, meaning that the energy levels are completely filled. However, for larger or more complex nuclei, other factors such as nuclear deformation and the presence of additional forces may need to be considered.

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