Abstract
Measurements have been made of the energy spectra, angular distributions, and absolute cross sections of protons emitted from bombardments of Co59, Ni58, Ni60, Ni62, Cu63, Cu65, Nb, Rh, Pd, and Pt targets by 42-MeV alpha particles. A dEdXE scintillation telescope was used in conjunction with an x, y oscilloscope to detect and identify protons in the energy range from 2 to 40 MeV. The data were compared with predictions of the statistical model of nuclear reactions. A calculation was made of the expected proton energy spectra based on this model. The cascade was restricted to neutron and proton emission only, and a level density of the form {exp2[a(Uδ)]12}(Uδ)2 was used. Except for Pt, the calculated and experimental energy spectra matched in slope over a relatively wide intermediate-energy region with the observed spectrum, exceeding the calculated spectrum in both the lowest and highest energy regions. The lowest energy protons were assumed to be caused by compound-nuclear events and the data were separated into compound-nuclear and non-compound-nuclear portions. It was found that the compound-nuclear portions agree well with expectations of the statistical model for yields, spectra, and angular distributions, and they account for 90% of the proton yield for targets in the Ni region, 65% of the proton yield for targets in the Rh region, and probably less than 6% of the proton yield for Pt. The non-compound-nuclear component exhibits a relatively constant yield of ≈85 mb for all the targets studied.