Photo-Neutron Sources and the Energy of the Photo-Neutrons
Open Access
- 15 April 1947
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review B
- Vol. 71 (8) , 497-507
- https://doi.org/10.1103/PhysRev.71.497
Abstract
In a preliminary study photo-neutrons were observed to be produced by the -rays from , , , , and when these artificially radioactive isotopes were placed in O or Be; , , , , and produced neutrons only in Be. The first group of isotopes must have -rays with energy higher than 2.18 Mev, and the second group must have -rays greater than 1.63 Mev but less than 2.18 Mev. No photo-neutrons were observed from , , Ag (225 day ½-life), , , , , , Ir (19 hours ½-life), and in Be; the intense -rays from these isotopes must have energies less than 1.63 Mev. In a second experiment the energy of the photo-neutrons from nine of these sources was determined by measuring the hydrogen scattering cross section of the emitted neutrons. Seven, of the sources seem to emit homogeneous groups of neutrons; they are: Sb+Be, Ga+O, La+O, Mn+O, Na+O, La+Be, and Na+Be with neutron energies 0.024, 0.13, 0.13, 0.22, 0.22, 0.62, and 0.83 Mev, respectively, for the particular sized sources studied. Mn+Be emits three groups of neutrons of different energies, but more than 80 percent of the neutrons seem to be in a group at 0.14 Mev. The energy of the -rays calculated to produce neutrons of these energies are: for , 2.74 Mev; for , 1.81 and 2.7 Mev (a third -ray is present); for , 2.50 Mev (at least one other -ray is present with an energy between 2.2 and 1.63 Mev); for , 1.67 Mev; and for , 2.49 Mev. The total neutron cross section of carbon is also given for seven of these photo-neutron sources.
Keywords
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