Astrophysical S-factors and reaction rates of (p,n)-reactions on (117)Sn, (118)Sn, (122)Sn, and (124)Sn

Ye Skakun, T. Rauscher

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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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.

Original languageEnglish
Title of host publicationInt Conf on Nuclear Data for Science and Technology
EditorsO. Bersillon, F. Gunsing, E. Bauge, R. Jacqmin, S. Leray
Place of PublicationCEDEX A
PublisherEDP Sciences
Pages1325-1327
Number of pages3
Volume2
ISBN (Print)978-2-7598-0091-9
DOIs
Publication statusPublished - 2008
EventInternational Conference on Nuclear Data for Science and Technology - Nice, France
Duration: 22 Apr 200727 Apr 2007

Conference

ConferenceInternational Conference on Nuclear Data for Science and Technology
Country/TerritoryFrance
CityNice
Period22/04/0727/04/07

Keywords

  • ISOTOPES

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