Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ssns.book.....d&link_type=abstract
Study of the s-process neutron source 22Ne(α, n)25Mg., by Drotleff, H. W.. Bochum Univ. (Germany). Fakultät für Physik und Astr
Astronomy and Astrophysics
Astrophysics
Scientific paper
In the present thesis the astrophysically relevant reaction 22Ne(α, n)25Mg was studied from the reaction threshold at Eα = 570 keV up to a projectile energy of Eα = 2300 keV. The high sensitivity together with a small target thickness led to the detection of a series of new resonances in the 22Ne(α, n)25Mg reaction. The resonance strengths and widths were determined by a folding procedure from the measured neutron yields. With the new data a by several orders of magnitude lower uncertainty of the reaction rates important for star-model calculations results.
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