Stellar reaction rate of 20Ne(α, γ)24Mg

Details Stellar reaction rate of 20Ne(α, γ)24Mg Stellar reaction rate of 20Ne(α, γ)24Mg

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nupha.398..279s&link_type=abstract

Nuclear Physics A, Volume 398, Issue 2, p. 279-307.

Physics

Nuclear Physics

30

Nuclear Reactions

Scientific paper

The reaction 20Ne(α, γ)24Mg has been investigated at Eα(lab) = 0.55-3.20 MeV. Neon gas enriched to 99.95% in 20Ne was recirculated in differentially pumped gas target systems of the extended and quasipoint jet types. New resonances were found at Eα(lab) = 958, 1226, 1260, 1704 and 2277 keV, which correspond to known states in 24Mg. Excitation energies, γ-ray decay schemes, γ-ray angular distributions, resonance widths and strengths as well as Jπ and T-assignments are reported for all the resonances. Information on low-lying states in 24Mg is also obtained. The nuclear and astrophysical aspects of the results are discussed.
Travel and other support has been given by the Natural Sciences and Engineering Research Council of Canada.

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