University of Hertfordshire

By the same authors

Astrophysical S-Factors and Reaction Rates of Threshold (p,n)-Reactions on (99-102)Ru

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

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Original languageEnglish
Title of host publication10th Int Symposium on Origin of Matter and Evolution of Galaxies
Subtitle of host publicationOMEG-2010
EditorsI. Tanihara
PublisherAmerican Institute of Physics
Pages390-393
Number of pages4
ISBN (Print)978-0-7354-0819-7
DOIs
Publication statusPublished - 2010
Event10th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG10) - Osaka, Japan
Duration: 8 Mar 201010 Mar 2010

Publication series

NameAIP Conf Procs
Volume1269
ISSN (Print)0094-243X

Conference

Conference10th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG10)
CountryJapan
CityOsaka
Period8/03/1010/03/10

Abstract

Astrophysical S-factors of (p,n) reactions on (99)Ru, (100)Ru, (101)Ru, and (102)Ru were derived from the sum of experimental isomeric and ground states cross sections measured in the incident proton energy range of 5-9 MeV. They were compared with Hauser-Feshbach statistical model predictions of the NON-SMOKER code. Good agreement was found in the majority of cases. Reaction rates were derived up to 8.7 GK stellar temperature by combining experiment and theory.

ID: 1620026