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The discrepancy between calculated and observed abundances of rare isotopes such as 36S and 46Ca is a longstanding problem. One of the reasons for this discrepancy was the lack or even the complete absence of experimental data on (n,p)- and (n,alpha)-reactions occurring during the nucleosynthesis process. This paper reports on an experimental programme set up to investigate (n,p)- and (n,alpha)-reactions and to determine their cross-sections for neutron energies from thermal up to about 500 keV. The measurements with thermal neutrons were performed at the high flux reactor of the ILL (Grenoble, France).

Additional information

Authors: WAGEMANS C, RUG, Department of Subatomic and Radiation Physics, Gent (BE);DRUYTS S, RUG, Department of Subatomic and Radiation Physics, Gent (BE);BARTHÉLÉMY R, JRC Geel (BE)
Bibliographic Reference: Paper presented: 3rd International Symposium on Nuclear Astrophysics : Gran Sasso (IT), July 8-13, 1994
Availability: Available from (1) as Paper EN 38547 ORA
Record Number: 199411089 / Last updated on: 1994-11-28
Original language: en
Available languages: en