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Isobar masses and beta decay

The masses of the isobars for a given A can be examined by considering them as a function of tex2html_wrap_inline2435 (i.e., in terms of the deviation from tex2html_wrap_inline2437 ).

displaymath2415

Note the importance of the pairing term. For odd A it is zero, and all isobar masses lie on one parabola. For even A, the even-even and odd-odd nuclides lie on different parabolae. Decays will occur down to the lowest masses by beta decay, which can only connect neighbouring nuclides. There will thus be one minimum for odd A, and (one or) two for even A.

The beta decays are determined by the mass differences. Various modes of beta decay are possible.

tex2html_wrap_inline2061 decay
This is for tex2html_wrap_inline2063 . The decay can be written as

displaymath2045

Note that the masses we deal with are atomic masses; in increasing the atomic number, the atom acquires another electron; this is `provided' by the beta decay process. Thus the overall atomic process is

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The neutrino is massless. The energy released as kinetic energy is then

displaymath2047

tex2html_wrap_inline2065 decay
This is for tex2html_wrap_inline2067 . The decay can be written as

displaymath2048

However, the reduction in atomic number has liberated an atomic electron; in terms of atoms

displaymath2049

The energy released as kinetic energy is then

displaymath2050

Electron capture
The above process cannot occur if the mass difference is less than twice the electrom mass ( tex2html_wrap_inline2069 MeV). The competing process of electron capture then becomes important. The s electrons in particular have a non-vanishing density within the nuclear volume. An atomic electron can then be `captured' by a proton to yield

displaymath2051

Electron numbers are now balanced and the energy release is

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where tex2html_wrap_inline2073 is the binding energy of the captured electron.



Physics Department
Wed Nov 6 08:30:28 GMT+0200 1996