Distribution of spontaneous fission fragments in nuclear astrophysical problems

Details Distribution of spontaneous fission fragments in nuclear astrophysical problems Distribution of spontaneous fission fragments in nuclear astrophysical problems

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..34..321o&link_type=abstract

Astrophysics and Space Science, vol. 34, May 1975, p. 321-345.

Astronomy and Astrophysics

Astrophysics

4

Abundance, Astrophysics, Fission Products, Nuclear Astrophysics, Nuclear Fission, A Stars, Heavy Nuclei, Mass Distribution, Mathematical Models, Meteoritic Composition, Neutron Emission, Solar System

Scientific paper

Empirical equations for calculating fission fragment yield are proposed which are applicable to all nuclides with an atomic mass below 208. An application of the equations to nuclear astrophysics indicates that the anomalously high abundance of medium weight elements observed in some peculiar A stars may be attributed to the accumulation of fission fragments from certain nuclei.

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