Relative yields of Al-26/g/ and Al-26/m/ from the Mg-25 /p, gamma/ reaction

Details Relative yields of Al-26/g/ and Al-26/m/ from the Mg-25 /p, gamma/ reaction Relative yields of Al-26/g/ and Al-26/m/ from the Mg-25 /p, gamma/ reaction

Jul 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...231..198n&link_type=abstract

Astrophysical Journal, Part 1, vol. 231, July 1, 1979, p. 189-200. Research supported by the U.S. Department of Energy.

Astronomy and Astrophysics

Astrophysics

3

Abundance, Aluminum 26, Magnesium Isotopes, Nuclear Fusion, Supernovae, Isotope Effect, Supermassive Stars, Tables (Data), Yield

Scientific paper

Relative yields of the Al-26 (5+) ground state, or Al-26(g), and the nearby 0(+) level, or Al-26(m), are derived from previous data on the Mg-25 (p, gamma) reaction for bombarding-proton energies of 0.3 to 1.72 MeV. When averaged over this energy range, the reaction yields are found to be in the ratio, Al-26(m)/Al-26(g) equals approximately 1/3. The significance of this yield ratio for nucleosynthesis in massive stars is briefly considered.

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