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Title: Predicting the production rates of cosmogenic nuclides in extraterrestrial matter

Conference ·

The production rates of nuclides made by the galactic and solar cosmic rays are important in the interpretations of measurements made with lunar samples, meteorites, and cosmic spherules. Production rates of cosmogenic nuclides have been predicted by a variety of methods that are reviewed in this paper, ranging from systematic studies of one or a group of meteorites to purely theoretical calculations. Production rates can vary with the chemical composition and the preatmospheric depth of the sample and with the size and shape of the object. While the production systematics for cosmogenic nuclides are fairly well known, our ability to predict their production rates can be improved, with a corresponding increase in the scientific return. Additional detailed studies of cosmogenic nuclides in extraterrestrial objects are needed, especially for fairly small and very large objects. Nuclides made in simulation experiments and cross sections for many major nuclear reactions should be measured. Such studies are especially needed for the long-lived radionuclides that have only recently become readily measurable by accelerator mass spectrometry. 34 refs., 5 figs.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
DOE Contract Number:
W-7405-ENG-36
OSTI ID:
6542744
Report Number(s):
LA-UR-87-1397; CONF-8704112-1; ON: DE87009008
Resource Relation:
Journal Volume: 29; Journal Issue: 1-2; Conference: 4. international symposium on accelerator mass spectrometry, Ontario, Canada, 27 Apr 1987; Other Information: Portions of this document are illegible in microfiche products
Country of Publication:
United States
Language:
English