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

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

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..390s&link_type=abstract

THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1

Astronomy and Astrophysics

Astrophysics

Nucleosynthesis, Stellar Evolution, Particle Accelerators, Normalising, Origin, Formation, And Abundances Of The Elements, Black Holes, Electrostatic Accelerators, Spectroscopic Factors And Asymptotic Normalization Coefficients

Scientific paper

Astrophysical S-factors of (p, n) reactions on 99Ru, 100Ru, 101Ru, and 102Ru 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.

Affiliated with

Also associated with

No associations

Rating

Astrophysical S-Factors and Reaction Rates of Threshold (p, n)-Reactions on 99-102Ru does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Astrophysical S-Factors and Reaction Rates of Threshold (p, n)-Reactions on 99-102Ru, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Astrophysical S-Factors and Reaction Rates of Threshold (p, n)-Reactions on 99-102Ru will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1862721