Abstract
Recently synthesized (t≲109 yr)r-process material has actinide elemental and isotopic abundance characteristics which can be used to distinguish it from ancientr-process material. The time-dependence of relative actinide abundances provides detailed chronometric information. Also it is shown that, ifN=184 is a neutron magic number as predicted by nuclear thery, the resultingr-process production peak atA∼281 will in turn yield, due to symmetric fission, a broad abundance peak aroundA∼135–140. The present results can be used to help verify or refute some current hypotheses concerning the origin of UH cosmic rays and some of the abundance anomalies in peculiar stars.
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Blake, J.B., Schramm, D.N. Recently synthesizedr-process nuclei: Ultra-heavy cosmic rays and peculiar stars. Astrophys Space Sci 30, 275–290 (1974). https://doi.org/10.1007/BF00648274
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DOI: https://doi.org/10.1007/BF00648274