mfb said:
That does not make sense.
Sorry, what I was trying to say was this:
In the O.P.'s example of the first excited state of
116In, which normally emits a ##\gamma## with energy 127.267 keV or 1.039##\times##10
-14 Joules
Such a photon has a momentum of E/c or 6.8##\times##10
-23 kg m
2 s
-2
Since this state has J=5 and decays to one of J=1, it has to lose 4 units of angular momentum, and the photon can only carry off 1, and as (orbital angular momentum) ##L = r \times p##, then the emission must be at a point at least L/p = 4.65##\times##10
-12 m from the centre of the nucleus.
Given that the nucleus has radius roughly 1.5##\times##10
-15 m times the cube root of the mass number, say 7##\times##10
-15 m. This means that the nucleon that decays must be considerably outside the normal boundary of the nucleus, and because the probability of it being that far out is extremely low, the half-life is quite long. Longer than the beta decay half-life of the unexcited nucleus, which has to lose only 1 unit of spin to become
116Sn (J=0).
The same applies to a beta decay for the excited state, (I don't have the figures for that), but again the large delta-J would tend to suppress it, since an electron and antineutrino together can only carry off one unit of J.
Have I got this right ?