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.
2003-07-01

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: http://hdl.handle.net/20.500.12079/210
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