Mass asymmetric fission and the termination of the astrophysical r-process

Details Mass asymmetric fission and the termination of the astrophysical r-process Mass asymmetric fission and the termination of the astrophysical r-process

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975phlb...55..281b&link_type=abstract

Physics Letters B, Volume 55, Issue 3, p. 281-285.

Physics

5

Scientific paper

We use a recent calculation of the mass-asymmetric fission barriers for heavy neutron-rich nuclei to estimate the heavy to light mass fragment ratio (MH/ML) resulting from fission at the termination of the astrophysical r-process. The fragments due to mass-asymmetric fission at the termination of the r-process may account for the solar system abundance distribution of neutron-rich nuclei in the mass region 150 <~ A <~ 170.

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