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                       THE NATURE OF THE NUCLEUS                                   150
                       The modern atomic theory does not picture the nucleus as a
                       group of stationary protons and neutrons clumped together by
                       some “nuclear glue.” The protons and neutrons are understood
                       to be held together by a nuclear force, a strong fundamental              1.5:1 ratio area         Band of
                       force of attraction that is functional only at very short dis-                                     stability
                                            –15
                       tances, on the order of 10  m or less. At distances greater than   100
                               –15
                       about 10  m, the nuclear force is negligible, and the weaker
                       electromagnetic force, the force of repulsion between like         1.25:1 ratio area
                       charges, is the operational force. Thus, like-charged protons
                       experience a repulsive force when they are farther apart than   Number of neutrons
                               –15
                                                             –15
                       about 10  m. When closer together than 10  m, the short-
                       range, stronger nuclear force predominates, and the protons       1:1 ratio area
                       experience a strong attractive force. This explains why the like-  50
                       charged protons of the nucleus are not repelled by their like                        1:1 ratio line
                       electric charges.
                           Observations of radioactive decay reactants and products
                       and experiments with nuclear stability have led to a shell model
                       of the nucleus. This model considers the protons and neutrons
                       moving in energy levels, or shells, in the nucleus analogous to
                       the orbital structure of electrons in the outermost part of the   0
                       atom. As in the electron orbitals, there are certain configura-  0  10 20 30 40 50 60 70 80 90 100
                       tions of nuclear shells that have a greater stability than others.        Number of protons
                       Considering electrons, filled and half-filled orbitals are more
                       stable than other arrangements, and maximum stability occurs   FIGURE 13.5  The shaded area indicates stable nuclei, which
                                                                               group in a band of stability according to their neutron-to-proton
                       with the noble gases and their 2, 10, 18, 36, 54, and 86 electrons.   ratio. As the size of nuclei increases, so does the neutron-to-proton
                       Considering the nucleus, atoms with 2, 8, 20, 28, 50, 82, or   ratio that represents stability. Nuclei outside this band of stability
                         126 protons or neutrons have a maximum nuclear stability. The   are radioactive.
                       stable numbers are not the same for electrons and nucleons
                       because of differences in nuclear and electromagnetic forces.    (not electrical) forces, which counter the increased electrical
                           Isotopes of uranium, radium, and plutonium, as well     repulsion from a larger number of positively charged protons.
                       as other isotopes, emit an alpha particle during radioactive   Thus, more neutrons are required in larger nuclei to produce
                       decay to a simpler nucleus. The alpha particle is a helium   a stable nucleus. However, there is a limit to the additional
                               4

                       nucleus,       He. The alpha particle contains two protons as well     attractive forces that can be provided by more and more

                               2
                       as two neutrons, which is one of the nucleon numbers of sta-    neutrons, and all isotopes of all elements with more than
                       bility, so you would expect the helium nucleus (or alpha par-    83 protons are unstable and thus undergo radioactive decay.
                       ticle) to have a stable nucleus, and it does. Stable means it does   The generalizations about nuclear stability provide a means
                       not undergo radioactive decay. Pairs of protons and pairs of   of predicting if a particular nucleus is radioactive. The general-
                       neutrons have increased stability, just as pairs of electrons in   izations are as follows:
                       a molecule do. As a result, nuclei with an even number of both
                       protons and neutrons are, in general, more stable than nuclei     1.  All isotopes with an atomic number greater than 83 have
                       with odd numbers of protons and neutrons. There are a little   an  unstable nucleus.
                       more than 150 stable isotopes with an even number of protons     2.  Isotopes that contain 2, 8, 20, 28, 50, 82, or 126 protons or
                       and an even number of neutrons, but there are only 4 stable     neutrons in their nuclei are more stable than those with
                       isotopes with odd numbers of each. Just as in the case of elec-  other numbers of protons or neutrons.
                       trons, there are other factors that come into play as the nucleus     3.  Pairs of protons and pairs of neutrons have increased
                       becomes larger and larger with increased numbers of nucleons.  stability, so isotopes that have nuclei with even numbers of
                           The results of some of these factors are shown in      both protons and neutrons are generally more stable than
                       Figure 13.5, which is a graph of the number of neutrons ver-  those that have nuclei with odd  numbers of both protons
                       sus the number of protons in nuclei. As the number of protons   and neutrons.
                         increases, the neutron-to-proton ratio of the stable nuclei also     4.  Isotopes with an atomic number less than 83 are stable when
                       increases in a band of stability. Within the band, the neutron-  the ratio of neutrons to protons in the nucleus is about 1:1
                       to-proton ratio increases from about 1:1 at the bottom left to   in  isotopes with up to 20 protons, but the ratio increases in
                              1
                       about 1 ⁄2:1 at the top right. The increased ratio of  neutrons   larger nuclei in a band of stability (see  Figure 13.5). Isotopes

                       is needed to produce a stable nucleus as the number of pro-  with a  ratio to the left or right of this band are unstable and
                       tons  increases. Neutrons provide additional attractive nuclear   thus will undergo radioactive decay.

                       13-5                                                                      CHAPTER 13  Nuclear Reactions   327
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