What Are the Key Concepts of the Shell Model in Nuclear Physics?

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The discussion focuses on the shell model of the nucleus, drawing parallels to the periodic table and electron configurations. The shell model suggests that closed shells or subshells lead to chemically inert atoms, with specific atomic numbers (Z = 2, 10, 18, 36, 54) where this occurs. The participant expresses confusion about how these numbers are derived, contrasting them with expected values based on the hydrogen atom model. It is noted that the strong interaction in the nucleus differs significantly from the electron-nucleus interaction, affecting energy levels and leading to distinct "magic numbers." The calculation of these numbers is acknowledged as complex but theoretically possible through numerical methods.
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I'm currently reading about nuclear and particle physics in B.R.Martins 'An introduction to nuclear and particle physics'.

In chapter 7.3 he introduces the shell model of the nucleus and draws an analogy to the periodic table and how we think of it being constructed of progressively placing more and more electrons in 'orbitals' given by the quantum numbers n,l and ml.

From the study of the hydrogen atom we know that the energy levels are degenerate with 2n^2. Martin further notes that if a shell or a subshell is filled then

\sum m_s = \sum m_l = 0
which implies that
\vec L = \vec S = 0 = \vec J = \vec L + \vec S.
He then states that 'For any atom with a closed shell or a closed sub-shell, the electrons are paired off and thus no valence electrons are avaiable. Such atoms are therefore chemically inert. It is straight forward to work out the atomic numbers at which this occurs. These are

Z = 2,10,18,36,54.'

But I do not understand how these numbers are obtained. If one follows the 'hydrogen model' I would think that the numbers at which we have a closed shell or subshell would be

Z = 2,4,10,12,18,28, \ldots

corresponding to the electron configurations

1s^2, 1s^2 2s^2, 1s^2 2s^2 2p^6,1s^2 2s^2 2p^63s^2, \ldots

What have I missunderstood here?
 
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The strong interaction in a nucleus is a bit different from the hydrogen atom. There, electrons have a potential given by other particles (the nucleus), with an 1/r^2-law. This is not true for the strong interaction, where the interaction is short-ranged and given by other nucleons in the same volume. As a result, the energy levels depend heavily on the quantum states, and you get a nice mess with different magic numbers.
 
But how, then, can it be that

It is straight forward to work out the atomic numbers at which this occurs
?
Can these be calculated within a theoretical framework?
 
You can work out these numbers if you know the energy levels.
Calculating these energy levels (numerically) is not so easy, but it is possible.
 

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