Mattauch isobar rule

Technetium and promethium

A consequence of this rule is that neither technetium nor promethium have any stable isotopes, as each of the neighboring elements on the periodic table (molybdenum and ruthenium, and neodymium and samarium, respectively) have a beta-stable isotope for each mass number for the range in which the isotopes of the unstable elements usually would be stable to beta decay. Samarium-147 is not a counterexample; although it is unstable, it is stable to beta decay. These ranges can be calculated using the liquid drop model (for example the stability of technetium isotopes), in which the isobar with the lowest mass excess or greatest binding energy is shown to be stable to beta decay because energy conservation forbids a spontaneous transition to a less stable state. |url-access=limited

Thus no stable nuclides have proton number 43 or 61, and by the same reasoning no stable nuclides have neutron number 19, 21, 35, 39, 45, 61, 71, 89, 115, or 123.

Exceptions

The only known exceptions to the Mattauch isobar rule are the cases of antimony-123 and tellurium-123 and of hafnium-180 and tantalum-180m, where both nuclei are observationally stable. It is predicted that 123Te should undergo electron capture to form 123Sb, but this decay has not yet been observed; 180mTa should be able to undergo isomeric transition to 180Ta, beta decay to 180W, electron capture to 180Hf, or alpha decay to 176Lu, but none of these decay modes have been observed.

In addition, beta decay has been seen for neither curium-247 nor berkelium-247, though it is expected that the former should decay into the latter. Both nuclides are alpha-unstable.

As mentioned above, the Mattauch isobar rule cannot make predictions as to the half-lives of the beta-unstable isotopes. Hence there are a few cases where isobars of adjacent elements both occur primordially, as the half-life of the unstable isobar is over a billion years. This occurs for the following mass numbers:

• 40 (40Ar and 40Ca stable; 40K unstable)
• 50 (50Ti and 50Cr stable; 50V unstable)
• 87 (87Sr stable; 87Rb unstable)
• 113 (113In stable; 113Cd unstable)
• 115 (115Sn stable; 115In unstable)
• 138 (138Ba and 138Ce stable; 138La unstable)
• 176 (176Yb and 176Hf stable; 176Lu unstable)
• 187 (187Os stable; 187Re unstable)

References

References

1. {{Holleman&Wiberg
2. (2011). "Handbook on the Physics and Chemistry of Rare Earths". [[Elsevier]].
3. Sonzogni, Alejandro. "Interactive Chart of Nuclides". Brookhaven National Laboratory.