On the production of l36Cl by high energy protons in thin and thick targets

Details On the production of l36Cl by high energy protons in thin and thick targets On the production of l36Cl by high energy protons in thin and thick targets

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nimpb.113..484h&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section B, v. 113, p. 484-489.

Physics

11

Scientific paper

Model calculations for the production of cosmogenic nuclides are a versatile tool for the interpretation of the abundances of cosmogenic nuclides, in dependence of the irradiation history in extraterrestrial matter, and the properties of the cosmic particle rays. Such a modelling requires integral excitation functions for the production of these nuclides by the most propagating primary and secondary particles of the cosmic radiation. Although many investigations on l36Cl in meteorites and lunar samples were made, the cross section data base for this nuclide was still insufficient. Here we report on cross section measurements for the proton-induced production of l36Cl from most relevant target elements and on the depth dependent production in thick targets. Our new nuclear data will be applied to the production of l36Cl in a lunar drill core and the meteorite Knyahinya.

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