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(n,p) and (n,alpha) cross-sections with astrophysical importance were measured for light nuclei with masses between 15 and 50 u. Thermal neutron induced measurements were performed at the high flux reactor of the I.L.L. (Grenoble), and the resonance and keV neutron energy region was covered at the Geel Linear Accelerator. The importance of these data is illustrated by means of a typical s-process nucleosynthesis reaction network.

Additional information

Authors: WAGEMANS C, University of Gent, Nuclear Physics Laboratory, Gent (BE);DRUYTS S ET AL., JRC Geel (BE);SCHILLEBEECKX P, JRC Ispra (IT);GELTENBORT P, Institut Laue-Langevin, Grenoble (FR)
Bibliographic Reference: Paper presented: International Conference on Nuclear data for Science and Technology, Jülich (DE), May 13-17, 1991
Availability: Available from (1) as Paper EN 36150 ORA
Record Number: 199110845 / Last updated on: 1994-12-02
Original language: en
Available languages: en
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