Synthesis of element 105
Dubnium “In 1968 experiments were conducted at the Laboratory of Nuclear Reactions of the Joint Institute for Nuclear Research in order to produce a new chemical element with atomic number 105 [1]. In the case of the irradiation of Am243 with accelerated Ne22 ions with a very small cross section, the formation of short-lived emitters of α – particles with an energy of 9.4-9.7 MeV was observed. |
However, on the basis of an analysis of the decay schemes of the known α-radioactive nuclei with an odd number of nucleons, it may be assumed that the bulk of the α-decay of the isotopes with Z = 105 corresponds to the excited levels of the daughter nuclei (Z = 103), and the most intense α-lines belonging to the isotopes 105260 and 105261 should be sought in the softer part of the α-spectrum (Eα-< 9.1 MeV). Unfortunately, the energy interval 8.8-9.0 MeV includes the α – particles of isotopes (Z < 92) formed as a result of nuclear reactions on trace impurities of lead in the americium target [2]. Therefore, despite extensive work on the purification of the target from lead, the analysis of this part of the spectrum was greatly hindered in [1]. Nonetheless, the synthesis of element 105 can also be approached from the other side…” From “THE SYNTHESIS OF ELEMENT 105”. G.N.Flerov, Yu.Ts.Oganessian, Yu.V.Lobanov, Yu.A.Lazarev, S.P.Tret’yakova, I.V.Kolesov, and V.M.Plotko download: [ pdf ] (767Kb) |
Dmitriev S.N. et al. Results of the Experiment on Chemical Identification of Db as a Decay Product of Element 115 Preprint of the JINR. Dubna, 2003.
download: [ pdf ] (347Kb)
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