On the existence of super-heavy elements near Z = 114 and N = 184 in meteorites

Details On the existence of super-heavy elements near Z = 114 and N = 184 in meteorites On the existence of super-heavy elements near Z = 114 and N = 184 in meteorites

Jan 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970nupha.140...69r&link_type=abstract

Nuclear Physics A, Volume 140, Issue 1, p. 69-73.

Physics

Nuclear Physics

13

Scientific paper

The observed excess abundance of 136Xe and 86Kr in
primitive chondritic meteorites can be attributed to spontaneous fission
of the super-heavy elements (near Z = 114 and N = 184) decaying through
symmetric and asymmetric fission modes respectively.

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