Mg-26(p, n)Al-26 cross section measurements

Details Mg-26(p, n)Al-26 cross section measurements Mg-26(p, n)Al-26 cross section measurements

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983apj...271..404s&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 271, Aug. 1, 1983, p. 404-407. Research supported by the Ford Motor Company

Astronomy and Astrophysics

Astrophysics

13

Abundance, Aluminum 26, Magnesium Isotopes, Astrophysics, Cross Sections, Meteoritic Composition, Nuclear Reactions, Positrons, Supernovae

Scientific paper

Mg-26(p, n)Al-26-reaction total cross section measurements have been conducted, with separate measurements of the cross sections to the first two excited states of Al-26 from threshold to 5.6 MeV. For the case of the inverse reactions, Al-26(n, p)Mg-26, thermally averaged reaction rates are tabulated over the T9 = 0.1-10 temperature range (with the three lowest states of Al-26 as 'targets'), and compared with rates calculated on the basis of a statistical model.

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