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. and Zilges, A.
(2003)
Determination of the (n,gamma) reaction rate of unstable W-185 in the astrophysical s-process via its inverse reaction.
Nuclear Physics A.
533C-535C.
ISSN 0375-9474
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.
| Item Type | Article |
|---|---|
| Keywords | GAMMA |
| Date Deposited | 29 May 2025 09:06 |
| Last Modified | 29 May 2025 09:06 |