Study of the s-process neutron source 22Ne(α, n)25Mg.

Astronomy and Astrophysics – Astrophysics

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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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