Abstract:The α decay half-lives of the recently produced isotopes of the 112, 114, 116 and 118 nuclei and decay products have been calculated in the quasi-molecular shape path using the experimental Q α value and a Generalized Liquid Drop Model including the proximity effects between nucleons in the neck or the gap between the nascent fragments. Reasonable estimates are obtained for the observed α decay half-lives. The results are compared with calculations using the Density-Dependent M3Y effective interaction and the … Show more
“…The GLDM allows to describe the processes of fusion, fission, light nucleus and α emission [9,10,11,12,13,14,15,16,17]. The macroscopic energy includes the volume, surface, Coulomb and proximity energies:…”
The proton radioactivity half-lives of spherical proton emitters are investigated theoretically. The potential barriers preventing the emission of proton are determined in the quasimolecular shape path within a generalized liquid drop model (GLDM) including the proximity effects between nuclei in a neck and the mass and charge asymmetry. The penetrability is calculated in the WKB approximation. The spectroscopic factor has been taken into account in half-life calculation, which is obtained by employing the relativistic mean field (RMF) theory combined with the BCS method with the force NL3. The half-lives within the GLDM are compared with the experimental data and other theoretical values. GLDM works quite well for spherical proton emitters when the spectroscopic factors are considered, indicating the necessity of introducing the spectroscopic factor and the success of the GLDM for proton emission. Finally, we present two formulae for proton emission half-life similar to the Viola-Seaborg formulae and Royer's formulae of α-decay.
“…The GLDM allows to describe the processes of fusion, fission, light nucleus and α emission [9,10,11,12,13,14,15,16,17]. The macroscopic energy includes the volume, surface, Coulomb and proximity energies:…”
The proton radioactivity half-lives of spherical proton emitters are investigated theoretically. The potential barriers preventing the emission of proton are determined in the quasimolecular shape path within a generalized liquid drop model (GLDM) including the proximity effects between nuclei in a neck and the mass and charge asymmetry. The penetrability is calculated in the WKB approximation. The spectroscopic factor has been taken into account in half-life calculation, which is obtained by employing the relativistic mean field (RMF) theory combined with the BCS method with the force NL3. The half-lives within the GLDM are compared with the experimental data and other theoretical values. GLDM works quite well for spherical proton emitters when the spectroscopic factors are considered, indicating the necessity of introducing the spectroscopic factor and the success of the GLDM for proton emission. Finally, we present two formulae for proton emission half-life similar to the Viola-Seaborg formulae and Royer's formulae of α-decay.
“…Refs. [43,56,68,72,73,76,[80][81][82]). In the analysis of the decay chains, however, effects of the single-particle structure of the nuclei have been usually disregarded.…”
Superheavy nuclei and elements / Nuclear mass / α-Decay energy / α-Decay half-life / Single-particle spectra / α-Decay chains Summary. A short review of the studies of superheavy nuclei (SHN), done recently in our theoretical group of Warsaw, is presented. Main attention is given to description of the properties of SHN. The description is performed by macroscopic-microscopic methods. Such properties as mass, α-decay energy and α-decay half-life are considered. Special attention is devoted to the analysis of the half-life. Although mainly treated in a phenomenological way, the role of the microscopic structure of a nucleus in this quantity is tested. It is found that this structure may significantly change the half-life of nuclei with the odd nucleon (or nucleons).
“…As known, in this case the probability for the decay (or the half-life T α ) is directly connected to the decay energy Q α and the atomic number of the nucleus. The Geiger-Nuttall relation [43], connecting these quantities (in the version of Viola-Seaborg [44] or any other version [45][46][47][48][49]), describes well all 65 known even-even nuclei heavier than Pb, for which both partial half-life and decay energies have been measured. The experimental values obtained earlier in hot and cold fusion reactions and belonging to the α-decay of even-even nuclei with 100 ≤ Z ≤ 110, are shown in Fig.…”
Summary. The observation of atomic numbers Z that are 40% larger than that of Bi, the heaviest stable element, is an impressive extension of nuclear survival. Although the super heavy nuclei (SHN) are at the limits of Coulomb stability, shell stabilization lowers the ground-state energy, creates a fission barrier, and thereby enables the SHE to exist. The fundamentals of the modern theory concerning the mass limits of nuclear matter have been experimentally verified.
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