Heaviest elements (synthesis and decay properties)

For the 60 years that have passed after the discovery of the first artificial elements Np and Pu, the investigations of the properties of new elements have become one of the fundamental and quickly developing fields of nuclear physics and nuclear chemistry. The transition from the traditional method of producing transuranium elements, where continuous and pulsed neutron fluxes have been used, to nuclear reactions induced by heavy ions has made it possible to synthesize 12 new elements heavier than fermium (Z = 100). The theoretical description of the masses and fission barriers of the new nuclei led in the mid-1960s to the prediction of "islands of stability" for the very heavy and superheavy nuclides in the vicinity of the closed proton and neutron shells. The experimental data that demonstrate the enhanced stability of nuclei, close to the deformed shells Z = 108 and N = 162, relative to different decay modes and also the reactions of their synthesis are discussed from the point of view of advancing into an unexplored region of heavier (superheavy) and significantly longer-lived nuclides close to the spherical shells Z = 114 and N = 184. Experiments are described and first results are presented on the synthesis of superheavy nuclei in Ca-48-induced reactions. Presented are also the observed decay chains of individual atoms consisting of sequential a-decays and terminated by spontaneous fission The energies and half-lives are in agreement with the predictions of theoretical models describing the structure of heavy nuclei. They are considered as a first evidence of the existence of the hypothetical region of stability of superheavy elements. The experiments were carried out at the FLNR heavy ion accelerator in the framework of a large collaboration with LLNL (Livermore), GSI (Darmstadt), RIKEN (Saitama), the Institute of Physics and Department of Physics of the Comenius University (Bratislava) and the Department of Physics of the University in Messina.