α-decay energy formula for superheavy nuclei based on the liquid-drop model

2010 ◽  
Vol 82 (3) ◽  
Author(s):  
Tiekuang Dong ◽  
Zhongzhou Ren
2006 ◽  
Vol 74 (1) ◽  
Author(s):  
Hongfei Zhang ◽  
Wei Zuo ◽  
Junqing Li ◽  
G. Royer

1971 ◽  
Vol 26 (4) ◽  
pp. 643-652 ◽  
Author(s):  
Jens Grumann ◽  
Tihomir Morovic ◽  
Walter Greiner

AbstractThe potential energy surface has been calculated by two methods which are compared with re­spect to spontaneous fission. In the first one essentially the sum of the single particle energies is computed as was done in a previous paper3 while in the second one the Strutinsky technique of renormalizing to a liquid drop model has been applied. Also the half-lives for electron capture are investigated together with the predictions of the half-lives for spontaneous fission and α-decay. The results support the existence of superheavy nuclei in the regions around Z = 114 and Z = 164.


2018 ◽  
Vol 98 (2) ◽  
Author(s):  
K. P. Santhosh ◽  
C. Nithya ◽  
H. Hassanabadi ◽  
Dashty T. Akrawy

2019 ◽  
Vol 28 (10) ◽  
pp. 1950089 ◽  
Author(s):  
Hong-Ming Liu ◽  
Jun-Yao Xu ◽  
Jun-Gang Deng ◽  
Biao He ◽  
Xiao-Hua Li

In this work, we systematically study the [Formula: see text] decay half-lives of 170 even–even nuclei with [Formula: see text] within the two-potential approach while the [Formula: see text] decay preformation factor [Formula: see text] is obtained by the cluster-formation model. The calculated results can well reproduce the experimental data. In addition, we extend this model to predict the [Formula: see text] decay half-lives of 64 even–even nuclei with [Formula: see text] whose [Formula: see text] decay is energetically allowed or observed but not yet quantified. For comparison, the two famous models i.e., SemFIS proposed by Poenaru et al. [Europhys. Lett. 77 (2007) 62001] and UDL proposed by Qi et al. [Phys. Rev. Lett. 103 (2009) 072501] are used. The predicted results of these models are basically consistent. At the same time, through analyzing the changing trend of [Formula: see text] decay energy [Formula: see text] of [Formula: see text] and 128 isotopes nuclei with the increasing of neutron number N and that of [Formula: see text] decay preformation factor [Formula: see text] of those isotopes even–even nuclei with the increasing of neutron number N, [Formula: see text] may be a new neutron magic number.


Author(s):  
Xiao Pan ◽  
Youtian Zou ◽  
Hong-Ming Liu ◽  
Biao He ◽  
Xiao-Hua Li ◽  
...  

2020 ◽  
Vol 101 (6) ◽  
Author(s):  
K. P. Santhosh ◽  
Dashty T. Akrawy ◽  
H. Hassanabadi ◽  
Ali H. Ahmed ◽  
Tinu Ann Jose

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