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

Sonnabend, K.
Mengoni, A.
Mohr, P.
Rauscher, T.
Vogt, K.
Zilges, A.

Open link

Publication date

May 2003

DOI

10.1016/S0375-9474(03)00835-2

Publisher

Elsevier BV

Journal

Nuclear Physics A

Abstract

The (gamma,n) reaction rate of W-186 was measured in order to deduce the (n,gamma) reaction rate of 185 W, 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.Peer reviewe

Extracted data

We use cookies to provide a better user experience.

Data Protection

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

Abstract

Extracted data

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

Abstract

Extracted data

Related items

Related items