| dc.contributor.author | Sonnabend, K. | |
| dc.contributor.author | Mengoni, A. | |
| dc.contributor.author | Mohr, P. | |
| dc.contributor.author | Rauscher, T. | |
| dc.contributor.author | Vogt, K. | |
| dc.contributor.author | Zilges, A. | |
| dc.date.accessioned | 2013-07-02T13:02:00Z | |
| dc.date.available | 2013-07-02T13:02:00Z | |
| dc.date.issued | 2003-05-05 | |
| dc.identifier.citation | Sonnabend , K , Mengoni , A , Mohr , P , Rauscher , T , Vogt , K & 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 , vol. 718 , pp. 533C-535C . https://doi.org/10.1016/S0375-9474(03)00835-2 | |
| dc.identifier.issn | 0375-9474 | |
| dc.identifier.uri | http://hdl.handle.net/2299/11022 | |
| dc.description.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. | en |
| dc.format.extent | 3 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Nuclear Physics A | |
| dc.subject | GAMMA | |
| dc.title | Determination of the (n,gamma) reaction rate of unstable W-185 in the astrophysical s-process via its inverse reaction | en |
| dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
| dc.contributor.institution | School of Physics, Engineering & Computer Science | |
| dc.description.status | Peer reviewed | |
| rioxxterms.versionofrecord | 10.1016/S0375-9474(03)00835-2 | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
