vanesch said:
Or still in other words, if there are many more Ba-132 around than Ba-133, the probability for a neutron to be captured by the Ba-132 is still way higher than the probability for it to destroy a Ba-133, so you should win by neutron irradiation.
That's the thing I love about this stuff - scientific notation. The equilibrium ratio 9 to 4,
is way more to us, but when we're talking 1.2 10E20 atoms of Ba-132 (in 100 mg Barium carbonate enriched to 40%, natural Barium has only .1% atoms of Ba-132) that gets us to 2.7 10E20 which just doesn't seem to be way more with all those zeros.
The folks at MURR (Missouri U Research Reactor) estimated it would take 5
weeks of irradiation in their hi flux neutron nook (4 10E14 n/s/cmE2) to get 100 mCi of Ba-133 from our 100 mg starting sample, at a cost on the order of $100,000 (if we could get the time, doubtful). And the cost of barium enriched in Ba-132 at $90 per mg was nothing to sneeze at either (not being a national lab). Doubling the amount of Ba-132 would cut the time in half (increasing Ba-132 cost from $9,000 to $18,000 though), but I had some volume constraints for the source size.
I can see why all the commercial isotope vendors seem to have 10mCi Ba-133 as an upper limit of activity. What's driving this is an industrial gaging application where I need a source of modest energy gammas. Cs-137 @ 662 KeV is way too high, Co-57 @ 122/136 KeV is fine, but the half life of 270 days is a nuisance in a machine that might be used for 20 years. Ba-133 with gammas ~ 300 KeV was a bit higher in energy than wanted, but the 10.5 year half life was useful.
Looks like I'll be sticking to Co-57, but it's interesting to look for other isotopes with low energy gammas, with a half life long enough to be useful, but short enough to get decent activity from a small volume.
For example, Rh-101 has 3.3 year half life and plentiful gammas @ 127 KeV and 198 KeV. But it doesn't look like it could be produced in a reactor (other than as a fission product). However, it might be made in an accelerator from Ru-100 + p -> Rh-101, but then Rh-101 + p -> Pd-102 which is stable + p -> Ag-103, etc. etc. and tables of proton capture seem not very comprehensive, for a reason I'm sure.