New perspectives in superheavy element chemistry and nuclear spectroscopy. First investigation of seaborgium hexacarbonyl
Julia Even
Helmholtz-Institut Mainz, Germany
Jeudi 04/09/2014, 11:00
Bat 703, p 45, CEA Saclay, Orme des Merisiers

SuperHeavy Elements (SHE) provide unique possiblities to study the influence
 of relativistic effects on the electronic structure. However, until
 recently, only a limited number of thermally stable, inorganic compounds
 of SHEs have been accessible due to technical restrictions [1]. Thanks to
 the approach of physical preseparation [2], many limitations could be
 overcome. We have developed in experiments at the TRIGA reactor in Mainz
 and at the TASCA separator at GSI a method to synthesize carbonyl
 complexes of short-lived isotopes [3]. This method has now been
 successfully applied at the GARIS separator at RIKEN to synthesize for the
 first time a carbonyl complex of a superheavy element - Seaborgium
 hexacarbonyl [4].

 265Sg was synthesized in the reaction 248Cm(22Ne,5n), separated from the
 primary beam, and was thermalized in a He/CO mixture behind GARIS. This
 way it formed a volatile complex and was transported in the gas stream to
 a COMPACT gas-chromatography detector[6], where its adsorption on SiO2 was
 studied. The chemical properties of seaborgium were compared to its
 lighter homologs molybdenum and tungsten. The combination of physical and
 chemical separation allowed studying the decay of 265Sg  under background-
 free conditions. Our results indicate the observation of Sg(CO)6 and
 provide new information on the nuclear properties of 265Sg.

Experimental details and results will be presented in the seminar. An
 outlook on future applications of CO chemistry in superheavy element
 research and as a new tool for background-free decay spectroscopy will be
 given.

[1] A. Tuerler and V. Pershina, Chem. Rev. 113, 1237-1312 (2013).

[2] Ch.E. Duellmann et al., Nucl. Instr. Meth. A 551, 528539 (2005).

[3] J. Even et al., Inorg.Chem. 51, 6431-6422 (2012).

[4] J. Even et al, accepted for publication in Science (2014).

[5] H. Haba et al., Phys. Rev. C 85, 024611(2012).

[6] A. Yakushev et al., Inorg. Chem. 53, 1624 (2014).

 

 

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