Abstract:A formula for the relationship between the α-decay energies (Q values) of superheavy nuclei (SHN) is presented, which is composed of the effects of Coulomb energy and symmetry energy. It can be employed not only to validate the experimental observations and measurements to a large extent, but also to predict the Q values of heaviest SHN with a high accuracy generally which will be very useful for future experiments. Furthermore, the shell closures in superheavy region and the effect of the symmetry energy on t… Show more
“…2 present a linear decreasing trend for N=158-162 and N=164-166 and an increasing trend for N=162-164. Such a complicated trend was attributed [19] to the large symmetry energy that lowers the Q α -value at the magic shells ( Fig. 1 and Fig.…”
Section: Resultsmentioning
confidence: 99%
“…To estimate the unknown Q α -values from the measured ones we employ the method [19], which takes into the account the effects of Coulomb energy and symmetry energy and validates not only the experimental measurements, but also predicts the Q α -values with a high accuracy. Once the parent or daughter nuclei have neutron or proton magic numbers ( Fig.…”
Abstract. The α-decay and spontaneous fission half-lives of nuclei around 270 Hs are calculated with formulas derived from an in-depth analysis of the available experimental data and of results of theoretical models. The parameters of these formulas result from the fit of half-lives with respect to the reaction energies, the height of the SF barrier and the fissionability. The calculated partial and total half-lives are compared with the experimental data and results of other approximations. Half-life predictions are made for many unknown nuclei.
“…2 present a linear decreasing trend for N=158-162 and N=164-166 and an increasing trend for N=162-164. Such a complicated trend was attributed [19] to the large symmetry energy that lowers the Q α -value at the magic shells ( Fig. 1 and Fig.…”
Section: Resultsmentioning
confidence: 99%
“…To estimate the unknown Q α -values from the measured ones we employ the method [19], which takes into the account the effects of Coulomb energy and symmetry energy and validates not only the experimental measurements, but also predicts the Q α -values with a high accuracy. Once the parent or daughter nuclei have neutron or proton magic numbers ( Fig.…”
Abstract. The α-decay and spontaneous fission half-lives of nuclei around 270 Hs are calculated with formulas derived from an in-depth analysis of the available experimental data and of results of theoretical models. The parameters of these formulas result from the fit of half-lives with respect to the reaction energies, the height of the SF barrier and the fissionability. The calculated partial and total half-lives are compared with the experimental data and results of other approximations. Half-life predictions are made for many unknown nuclei.
“…Bottom part includes the results of our calculations for decay modes, branching ratios and total half-life for the known and many unknown nuclei. [13].…”
“…We have calculated Q α [19,20,21,22,23,24,25], total half-lives, alpha half-lives, spontaneous fission halflives and branching ratio (alpha and SF) of nuclei with Z=104-112 and N=158-166. The agreement to the results of Refs.…”
Abstract. Simple relationships derived from the systematics of experimental and calculated α-decay and spontaneous fission halflives are used to predict half-lives for many undiscovered nuclides around 270 Hs. α half-lives are calculated within the shell model rate theory in terms of the formation and reaction amplitudes. Estimations for spontaneous fission half-lives are performed within a dynamical approach defined essentially by the shape, the height of fission barrier and nuclear deformations. Systematic trends in evolution of the decay properties with Z, N and the valence proton and neutron numbers are illustrated and discussed.
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