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

Skakun, Ye and Rauscher, T. (2010) Astrophysical S-Factors and Reaction Rates of Threshold (p,n)-Reactions on (99-102)Ru. American Institute of Physics (AIP).
Copy

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.
Item Type Other
Keywords p-process; MODEL; PROCESS NUCLEOSYNTHESIS; CAPTURE CROSS-SECTIONS; statistical model; RELEVANT; (p,n) reactions; reaction rates; GAMMA-PROCESSES; NUCLEAR ASTROPHYSICS; nucleosynthesis; P-PROCESS
Date Deposited 29 May 2025 09:15
Last Modified 29 May 2025 09:15

Explore Further

Full text not available from this repository.

Atom BibTeX OpenURL ContextObject in Span OpenURL ContextObject Dublin Core MPEG-21 DIDL Data Cite XML EndNote HTML Citation METS MODS RIOXX2 XML Reference Manager Refer ASCII Citation
Export

Downloads