Synthesis of Superheavy Elements in the r-Process

Details Synthesis of Superheavy Elements in the r-Process Synthesis of Superheavy Elements in the r-Process

May 1971

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1971natur.231..103s&link_type=abstract

Nature, Volume 231, Issue 5298, pp. 103-106 (1971).

Physics

61

Scientific paper

Contrary to previous opinion, super-heavy elements can be produced in
the r-process in explosive stellar events. Calculations are based on
estimates of the fissionability of very neutron-rich superheavy nuclei
using currently accepted mass-law parameters. Certain consequences for
empirical cosmic ray abundance and galactic chronology are discussed.

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