The net internal angular momentum of a nucleus is called the “nuclear spin.” It is an important quantity for applications such as NMR and MRI, and it is also important for what nuclear decays and reactions occur and at what rate. One previous example was the categorical refusal of bismuth-209 to decay at the rate it was supposed to in section 14.11.3.
This section provides an overview of the ground-state spins of nuclei. According to the rules of quantum mechanics, the spin must be integer if the total number of nucleons is even, and half-integer if it is odd. The shell model can do a pretty good job of predicting actual values. Historically, this was one of the major reasons for physicists to accept the validity of the shell model.
For nuclei with both an even number of protons and an even number of neutrons, the odd-particle shell model predicts that the spin is zero. This prediction is fully vindicated by the experimental data, figure 14.29. There are no known exceptions to this rule.
Nuclei with an odd mass number
have either an odd number of
protons or an odd number of neutrons. For such nuclei, the
odd-particle shell model predicts that the nuclear spin is the net
angular momentum (orbital plus spin) of the last odd nucleon. To find
it, the subshell that the last particle is in must be identified.
That can be done by assuming that the subshells fill in the order
given in section 14.12.2. This ordering is indicated by the
colored lines in figures 14.30 and 14.31.
Nuclei for which the resulting nuclear spin prediction is correct are
indicated with a check mark.
The prediction is correct right off the bat for a considerable number
of nuclei. That is very much nontrivial. Still, there is an even
larger number for which the prediction is not correct. One major
reason is that many heavy nuclei are not spherical in shape. The
shell model was derived assuming a spherical nuclear shape and simply
does not apply for such nuclei. They are the rotational nuclei;
roughly the red squares in figure 14.20, the smallest
squares in figure 14.17. Their main regions are for atomic
number above
82 and in the interior of the
82,
82 wedge.
For almost all remaining nuclei near the stable line, the spin can be explained in terms of the shell model using various reasonable excuses, [34, p. 224ff]. However, it seems more interesting to see how may spins can be correctly predicted, rather than justified after the fact. It may be noted that even if the wrong value is predicted, the true value is usually either another value in the same major shell, or one less than such a value.
One modification of the odd-particle shell model has been allowed for in the figures. It is that if the subshell being filled is above one of lower spin, a particle from the lower subshell may be promoted to the higher one; it can then pair up at higher spin. Since the odd nucleon is now in the lower shell, the spin of the nucleus is predicted to be the one of that shell. The spin is lowered. In a sense of course, this gives the theory a second shot at the right answer. However, promotion was only allowed for subshells immediately above one with lower spin in the same major shell, so the nucleon could only be promoted a single subshell. Also, no promotion was allowed if the nucleon number was below 32. Nuclei for which spin lowering due to promotion can explain the observed spin are indicated with an “L” or “l” in figures 14.30 and 14.31. For the nuclei marked with “L,” the odd nucleon cannot be in the normal subshell because the nucleus has the wrong parity for that. Therefore, for these nuclei there is a solid additional reason besides the spin to assume that promotion has occurred.
Promotion greatly increases the number of nuclei whose spin can be
correctly predicted. Among the remaining failures, notable are nuclei
with odd proton numbers just above 50. The ![]()
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In a few exceptional cases, like the unstable nitrogen-11 and beryllium-11 mirror nuclei, the theoretical model predicted the right spin, but it was not counted as a hit because the nuclear parity was inconsistent with the predicted subshell.
If both the number of protons and the number of neutrons is odd, the
nuclear spin becomes much more difficult to predict. According to the
odd-particle shell model, the net nuclear spin
comes from
combining the net angular momenta
of the odd proton and
of
the odd neutron. In particular, quantum mechanics allows any integer
value for
in the range
| (14.25) |
The so-called “Nordheim rules” attempt to do so. The
underlying idea is that nuclei like to align the spins of the two odd
nucleons, just like the deuterium nucleus does. To describe the
rules, the net angular momentum
of an odd nucleon and its spin
will be called “parallel” if
,
the orbital angular momentum. The idea is that
then the spin acts to increase
,
.
.
To check those rules is not trivial, because it requires the values of
for the odd proton and neutron. Who will say in what shells the
odd proton and odd neutron really are? The simplest solution is to
simply take the shells to be the ones that the shell model predicts,
assuming the subshell ordering from section 14.12.2. The
nuclei that satisfy the Nordheim rules under that assumption are
indicated with a check mark in figure 14.32. A blue check
mark means that the new and improved version has been used. It is
seen that the rules get a number of nuclei right.
An “L” or “l” indicates that it has been assumed that the spin of at least one odd nucleon has been lowered due to promotion. The rules are the same as in the previous subsection. In case of “L,” the Nordheim rules were really verified. More specifically, for these nuclei there was no possibility consistent with nuclear spin and parity to violate the rules. For nuclei with an “l” there was, and the case that satisfied the Nordheim rules was cherry-picked among other otherwise valid possibilities that did not.
A further weakening of standards applies to nuclei marked with “N” or “n.” For those, one or two subshells of the odd nucleons were taken based on the spins of the immediately neighboring nuclei of odd mass number. For nuclei marked with “N” the Nordheim rules were again really verified, with no possibility of violation within the now larger context. For nuclei marked “n,” other possibilities violated the rules; obviously, for these nuclei the standards have become miserably low. Note how many “correct” predictions there are in the regions of nonspherical nuclei in which the shell model is quite meaningless.
Preston and Bhaduri [34, p. 239] suggest that the proton and neutron angular momenta be taken from the neighboring pairs of nuclei of odd mass number. Figure 14.33 shows results according to that approach. To minimize failures due to other causes than the Nordheim rules, it was demanded that both spin and parity of the odd-odd nucleus were solidly established. For the two pairs of odd mass nuclei, it was demanded that both spin and parity were known, and that the two members of each pair agreed on the values. It was also demanded that the orbital momenta of the pairs could be confidently predicted from the spins and parities. Correct predictions for these superclean cases are indicated by check marks in figure 14.33, incorrect ones by an “E” or cross. Light check marks indicate cases in which the spin of a pair of odd mass nuclei is not the spin of the odd nucleon.
Preston and Bhaduri [34, p. 239] write:
“When confronted with experimental data, Nordheim’s rules
are found to work quite well, most of the exceptions being for light
nuclei.” So be it. The results are definitely better than
chance. Below
50, the rules get 43 right out of 71. It may be
noted that if you simply take the shells directly from theory with no
promotion, like in figure 14.34, you get only 41 right, so
using the spins of the neighbors seems to help. The “Nuclear
Data Sheets” policies assume that the (unimproved) Nordheim
rules may be helpful if there is supporting evidence.
The nuclei marked with “E” in figure 14.33 are particularly interesting. For these nuclei spin or parity show that it is impossible for the odd proton and neutron to be in the same shells as their neighbors. In four cases, the discrepancy is in parity, which is particularly clear. It shows that for an odd proton, having an odd neutron is not necessarily intermediate between having no odd neutron and having one additional neutron besides the odd one. Or vice-versa for an odd neutron. Proton and neutron shells interact nontrivially.
It may be noted that the unmodified Nordheim rules imply that there
cannot be any odd-odd nuclei with ![]()
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