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AbstractAbstract
[en] Predictions of capture cross sections by Hauser-Feshbach calculations should be based on accurate gamma-ray strength functions and level densities. In the mass region 135≤A≤205 gamma-ray strength function models for dipole radiation were evaluated by demanding a simultaneous reproduction of average resonance data, capture cross sections and gamma-ray production spectra. The best results for E1 are obtained with a strength derived from a 'generalized Lorentzian' with a non-zero limit as the energy tends to zero and a width dependent on energy and deformation. The authors recommend for M1 to derive the strength from a spin-flip giant resonance of Lorentzian shape. (author). 28 refs., 5 figs
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Oct 1992; 8 p; 2. International Symposium on Nuclear Astrophysics, Nuclei in Cosmos; Karlsruhe (Germany); 6-10 Jul 1992; Also available from Netherlands Energy Research Foundation, Library-ECN, P.O.Box 1, 1755 ZG Petten (NL)
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