30 keV /n, gamma/ cross-sections from the nuclear statistical model

Details 30 keV /n, gamma/ cross-sections from the nuclear statistical model 30 keV /n, gamma/ cross-sections from the nuclear statistical model

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981ap%26ss..77..357h&link_type=abstract

Astrophysics and Space Science, vol. 77, no. 2, July 1981, p. 357-367.

Physics

Nuclear Physics

68

Astronomical Models, Gamma Ray Astronomy, Neutron Cross Sections, Nuclear Fusion, Radiative Transfer, Reaction Kinetics, Density Distribution, Distribution Functions, Neutron Emission, Nuclei (Nuclear Physics), Statistical Analysis

Scientific paper

Preliminary results are reported for 30 keV (n, gamma) cross-sections calculated by means of a Hauser-Feshbach model program. The calculation allows for populated excited states of the target nucleus, for integration over level density functions when target or residual nucleus states are unknown, for departures of the cross-section from the calculated value due to width fluctuations, and for gamma-delayed neutron emission. Agreement with experimental results to within 70% is generally obtained.

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