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

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

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003nupha.718..533s&link_type=abstract

Nuclear Physics A, Volume 718, p. 533-535.

Physics

Nuclear Physics

Scientific paper

The (γ, n) reaction rate of 186W was measured in order to deduce the (n, γ) 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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