The (gamma,n) reaction rate of 186W was measured in order to deduce the (n,gamma) reaction rate of 185W, an important branching point in the astrophysical s-process. The theoretical predictions have been confirmed and the error range was slightly decreased. The derived Maxwellian averaged cross section (MACS) at 30 keV is (687 ± 110) mb.

Determination of the (n,gamma) reaction rate of unstable 185W in the astrophysical s-process via its inverse reaction

Mengoni, A.
2003

Abstract

The (gamma,n) reaction rate of 186W was measured in order to deduce the (n,gamma) reaction rate of 185W, an important branching point in the astrophysical s-process. The theoretical predictions have been confirmed and the error range was slightly decreased. The derived Maxwellian averaged cross section (MACS) at 30 keV is (687 ± 110) mb.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.12079/210
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