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Gamma-Ray Yields from Nuclear Reactions and Level Densities of Deformed Nuclei
Phys. Rev. 151, 992 – Published 18 November, 1966
DOI: https://doi.org/10.1103/PhysRev.151.992
Abstract
Theoretical calculations of spin distributions of compound nuclei and subsequent neutron-evaporation products are made for 27-MeV alpha particles on , 52-MeV alpha particles on , and 56-MeV ions on . The first two cases were chosen to match experimental work of Lark and Morinaga. We use our calculations as a basis for interpretation of their relative yield of , the isomer, and the state of the ground rotational band. We find these yields consistent with the simple assumption that after the last neutron is evaporated to form the excited nucleus all products with spin feed into the isomer and those with spin contribute to the prompt radiation from the first level. Possible relationships between the course of the gamma-ray cascade and the nature of the Nilsson orbitals nearest the Fermi surface are discussed. Finally, the importance of measuring gamma-ray angular distributions in addition to integrated yields is stressed, and formulas of possible value for the analysis of such angular distributions are collected and presented.
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