Synthesis of Superheavy Elements

Details Synthesis of Superheavy Elements Synthesis of Superheavy Elements

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005omeg.conf..266m&link_type=abstract

ORIGIN OF MATTER AND EVOLUTION OF GALAXIES 2003. Held 17-19 November 2003 in RIKEN, Wako, Saitama, Japan. Edited by M Terasawa,

Astronomy and Astrophysics

Astronomy

Scientific paper

In RIKEN (The Institute of Physical and Chemical Research) productions and decays of isotopes 271110 and 272111 were studied using a gas-filled recoil ion separator GARIS. The isotopes were produced by 208Pb + 64Ni ¤271110 + n and 209Bi + 64Ni ¤272111+ n reactions, respectively. Fourteen α-decay chains have been assigned to be the decays originating from the isotope 271110. We have observed 14 α-decay chains that can be assigned to subsequent decays from 272111. The results have provided good confirmations of productions and decays of both the 271110 and 272111 reported by GSI group.

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