Calculation of cosmogenic nuclides in stony meteorites

Details Calculation of cosmogenic nuclides in stony meteorites Calculation of cosmogenic nuclides in stony meteorites

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aipc..183..392d&link_type=abstract

Cosmic abundances of matter. AIP Conference Proceedings, Volume 183, pp. 392-393 (1989).

Physics

Scientific paper

In our calcuations, use is made of Monte Carlo techniques for identifying nuclear collisions and specific nuclear reactions as well as establishing the transport of the incident nucleon and its generated nucleons. It is possible to use an integrated calculational approach in predicting the cosmogenic nuclide production rate and depth dependence. In particular, the High Energy intranuclear and internuclear Cascade Transport Code, HETC, (developed by Armstrong et al.) is used to calculate directly the nuclide production rate due to spallation. When the neutron source spectrum generated with HETC is linked to the low energy neutron transport code, MORSE, the neutron induced cosmogenic nuclide profiles can be calculated without the resort to extrapolation of excitations functions.

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