Effects of bulk composition on production rates of cosmogenic nuclides in meteorites

Details Effects of bulk composition on production rates of cosmogenic nuclides in meteorites Effects of bulk composition on production rates of cosmogenic nuclides in meteorites

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lpi....24..937m&link_type=abstract

In Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 2: G-M p 937-938 (SEE N94-16173 03-91)

Computer Science

Argon Isotopes, Chemical Composition, Flux (Rate), Isotopic Enrichment, Meteorites, Meteoritic Composition, Neon Isotopes, Nuclides, Computerized Simulation, Galactic Cosmic Rays, Monte Carlo Method

Scientific paper

The bulk chemical composition of meteorites has been suggested as a main factor influencing the production of cosmogenic nuclides. Numerical simulations with Los Alamos Monte Carlo production and transport codes were done for Ne-21/Ne-22 ratios and Ar-38 production rates in meteorites with a wide range of compositions. The calculations show that an enhanced flux of low-energy secondary particles in metal-rich phases is the essential key for the explanation of experimentally observed differences in nuclide production processes in various meteorite classes.

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