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/sup 186,187,188/Os(n,. gamma. ) cross sections and galactic nucleosynthesis

Journal Article · · Phys. Rev., C; (United States)
The /sup 186,187,188/Os(n,..gamma..) cross sections were measured over the incident neutron energy range 2.6--800 keV. Optimized statistical model fits to the average cross sections were made employing estimates of the /sup 186/Os, /sup 187/Os, and /sup 188/Os p-wave strength functions 0.29 x 10/sup -4/, 0.45 x 10/sup -4/, and 0.33 x 10/sup -4/, respectively, d-wave strength functions 1.3 x 10/sup -4/, 4.0 x 10/sup -4/, and 1.5 x 10/sup -4/, respectively, and gamma ray strength functions (Gamma-bar/sub ..gamma..//D/sub 0/) 26.8 x 10/sup -4/, 176 x 10/sup -4/, and 20.8 x 10/sup -4/, respectively. A lower bound for the /sup 187/Os neutron inelastic cross section is estimated as 0.25(20) b at 30 keV. The Maxwellian-averaged capture cross sections are presented as a function of temperature. The ratio of 30 keV Maxwellian-averaged cross sections /=0.504(17) is reported and the lack of agreement with earlier measurements of this ratio is discussed. The use of this cross section ratio in estimating, via the /sup 187/Re-/sup 187/Os beta decay, the duration of galactic nucleosynthesis is discussed. The cross section ratio from this work yields an estimate of 10.4(25) x 10/sup 9/ yr for the duration of galactic nucleosynthesis, a result higher than but still consistent with the estimate 7(2) x 10/sup 9/ yr derived from U/Th decay.
Research Organization:
Physics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37830
OSTI ID:
5727378
Journal Information:
Phys. Rev., C; (United States), Journal Name: Phys. Rev., C; (United States) Vol. 21:2; ISSN PRVCA
Country of Publication:
United States
Language:
English