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Abstract

In this paper the 36-Cl(n,p)36-S and 36-Cl(n,alpha)33-S reaction cross-sections have been measured with high resolution from 1 eV up to 300 keV. The corresponding Maxwellian averaged cross-sections and astrophysical reaction rates are calculated.

Additional information

Authors: BIEBER R, JRC Geel (BE);BARTHÉLÉMY R, JRC Geel (BE);VAN GILS J, JRC Geel (BE);WAGEMANS C, RUG, Department of Subatomic and Radiation Physics, Gent (BE);HEYSE J, RUG, Department of Subatomic and Radiation Physics, Gent (BE);BALCAEN N, RUG, Department of Subatomic and Radiation Physics, Gent (BE)
Bibliographic Reference: Paper presented: Ninth International Symposium on Capture Gamma Ray Spectroscopy and related topics, Budapest (HU), October 8-12, 1996
Availability: Available from (1) as Paper EN 40116 ORA
Record Number: 199611271 / Last updated on: 1996-10-29
Category: PUBLICATION
Original language: en
Available languages: en