Thick target yields of 26Alg.s. from the 16O(16O,x)26Alg.s. and 16O(14N,x)26Alg.s. reactions

Details Thick target yields of 26Alg.s. from the 16O(16O,x)26Alg.s. and 16O(14N,x)26Alg.s. reactions Thick target yields of 26Alg.s. from the 16O(16O,x)26Alg.s. and 16O(14N,x)26Alg.s. reactions

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999phrvc..60b8801y&link_type=abstract

Physical Review C (Nuclear Physics), Volume 60, Issue 2, August 1999, id. 028801

Physics

Nuclear Physics

Cosmic Ray Nucleosynthesis, Compound Nucleus, General, Solar Nebula, Cosmogony, Origin, Formation, And Abundances Of The Elements

Scientific paper

Extending the earlier work of Bateman et al., we have measured the energy-integrated yield of 26Alg.s. from the 16O(16O,x)26Alg.s. and 16O(14N,x)26Alg.s. reactions. We find that although the yield from the 16O(16O,x)26Alg.s. reaction is several times larger than from the 12C(16O,x)26Alg.s. reaction, the abundance of fossil 26Alg.s. observed in carbonaceous chondrite meteorites could be produced by oxygen-rich cosmic rays via the 16O(16O,x)26Alg.s. reaction only under the improbable scenario that more than 40% of the solar system oxygen was injected into the protosolar nebula as cosmic rays.

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