| dc.contributor.author | Skakun, Ye | |
| dc.contributor.author | Rauscher, T. | |
| dc.contributor.editor | Bersillon, O. | |
| dc.contributor.editor | Gunsing, F. | |
| dc.contributor.editor | Bauge, E. | |
| dc.contributor.editor | Jacqmin, R. | |
| dc.contributor.editor | Leray, S. | |
| dc.date.accessioned | 2014-12-04T10:29:40Z | |
| dc.date.available | 2014-12-04T10:29:40Z | |
| dc.date.issued | 2008 | |
| dc.identifier.citation | Skakun , Y & Rauscher , T 2008 , Astrophysical S-factors and reaction rates of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn . in O Bersillon , F Gunsing , E Bauge , R Jacqmin & S Leray (eds) , Int Conf on Nuclear Data for Science and Technology . vol. 2 , EDP Sciences , CEDEX A , pp. 1325-1327 , International Conference on Nuclear Data for Science and Technology , Nice , France , 22/04/07 . https://doi.org/10.1051/ndata:07216 | |
| dc.identifier.citation | conference | |
| dc.identifier.isbn | 978-2-7598-0091-9 | |
| dc.identifier.uri | http://hdl.handle.net/2299/14884 | |
| dc.description.abstract | Astrophysical S-factors and reaction rates were derived from available cross sections of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn isotopes at incident proton energies up to 9 MeV. The statistical theory predictions of the observable quantities are similar to 2 times smaller at near threshold energies and have better agreement at higher energies. | en |
| dc.format.extent | 3 | |
| dc.format.extent | 124543 | |
| dc.language.iso | eng | |
| dc.publisher | EDP Sciences | |
| dc.relation.ispartof | Int Conf on Nuclear Data for Science and Technology | |
| dc.subject | ISOTOPES | |
| dc.title | Astrophysical S-factors and reaction rates of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn | en |
| dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
| rioxxterms.versionofrecord | 10.1051/ndata:07216 | |
| rioxxterms.type | Other | |
| herts.preservation.rarelyaccessed | true | |
