Modeling the Production of Be-7, Be-10, and Al-26 by Spallation Reactions in the Early Solar System

Details Modeling the Production of Be-7, Be-10, and Al-26 by Spallation Reactions in the Early Solar System Modeling the Production of Be-7, Be-10, and Al-26 by Spallation Reactions in the Early Solar System

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1268l&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1268

Physics

1

Scientific paper

Modeled production rates for 7Be,10Be, and
26Al in CAIs from the early solar system are presented. The
new results simultaneously describe the measured data and are therefore
strong indications of a spallogenic origin for these isotopes.

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