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- W1576593808 abstract "Maxwellian Neutron capture cross sections important for nucleosynthesis processes in stars are computed from the recommended individual resonance parameters, as well as from the measured energy dependent cross sections. The experimental neutron capture cross sections, spanning the energy range from a few keV to about 500 keV are evaluated in the framework of the Lane-Lynn capture formalism by including several partial waves in the analysis. In addition, in a few cases, the neutron inelastic scattering channels are included. The feasibility of extrapolating the calculations to nuclides off the stability line is examined. The effect of stellar temperature in the range from 10 keV to 50 keV on the Maxwellian neutron capture cross sections is investigated. The Maxwellian capture cross sections at 30-KeV for {sup 93}Nb, {sup 127}I, {sup 141}Pr, {sup 150}Sm, {sup 152}Sm, {sup 154}Sm, and {sup 181}Ta are computed and are compared with other determinations." @default.
- W1576593808 created "2016-06-24" @default.
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- W1576593808 date "1997-07-01" @default.
- W1576593808 modified "2023-09-27" @default.
- W1576593808 title "Neutron capture cross sections for nucleosynthesis" @default.
- W1576593808 hasPublicationYear "1997" @default.
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