Autor: |
Skakun, E., Utenkov, S., Bondarenko, V., Goncharov, A., Mishchenko, V., Sukhostavets, V., Shebeko, K. |
Zdroj: |
Bulletin of the Russian Academy of Sciences: Physics; Mar2008, Vol. 72 Issue 3, p376-379, 4p |
Abstrakt: |
The excitation functions for the reactions of radiative proton capture, 64Zn(p,γ)65Ga and 66Zn(p,γ)67Ga, which are of interest for stellar nucleosynthesis, have been measured in the range of incidentproton energies from 1 to 2.8 MeV. The astrophysical S factor and reaction rates have been derived from the reaction cross sections. The experimental results are compared with the predictions of the Hauser-Feshbach statistical theory. [ABSTRACT FROM AUTHOR] |
Databáze: |
Complementary Index |
Externí odkaz: |
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