Effects of partial deconvolution of the UHCRE data on the inferred r-process contribution to cosmic ray abundances for 74 <= Z <= 86

Details Effects of partial deconvolution of the UHCRE data on the inferred r-process contribution to cosmic ray abundances for 74 <= Z <= 86 Effects of partial deconvolution of the UHCRE data on the inferred r-process contribution to cosmic ray abundances for 74 <= Z <= 86

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995nimpa.361..342b&link_type=abstract

Nuclear Instruments and Methods in Physics Research Section A, v. 361, p. 342-348

Physics

1

Scientific paper

A ratio between the relative abundances of the groups of platinum (75 <= Z <= 79) and lead (80 <= Z <= 83) has been extracted from a published sample of 270 galactic cosmic rays from the Ultra Heavy Cosmic Ray Experiment after carrying out a process of partial deconvolution. The ratio obtained is compared with the ratio corresponding to a solar system-like source composition and found to be significantly higher. This result, compatible with previous experiments, suggests a contribution of the r-process to cosmic ray abundances.

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