A Study on the Emission of 1, 2 Proton Halo Nuclei from Parent with Z = 121–128 in the Superheavy Nuclei via Cluster Radioactivity

2020 ◽  
Vol 50 (3) ◽  
pp. 298-316
Author(s):  
K. P. Anjali ◽  
K. Prathapan ◽  
R. K. Biju
1997 ◽  
Vol 616 (1-2) ◽  
pp. 247-253 ◽  
Author(s):  
Yu.E. Penionzhkevich
Keyword(s):  

2014 ◽  
Vol 89 (2) ◽  
Author(s):  
Raj Kumar ◽  
J. A. Lay ◽  
A. Vitturi
Keyword(s):  

2004 ◽  
Vol 154 ◽  
pp. 85-91 ◽  
Author(s):  
Takashi Nakatsukasa ◽  
Kazuhiro Yabana ◽  
Makoto Ito ◽  
Minoru Kobayashi ◽  
Manabu Ueda

Author(s):  
H. C. Manjunatha ◽  
S. Alfred Cecil Raj ◽  
A. M. Nagaraja ◽  
N. Sowmya

Cluster radioactivity is an intermediate between alpha decay and spontaneous fission. It is also an exotic decay obtained in superheavy nuclei. When a cluster decay is detected in superheavy nuclei, the daughter nuclei is having near or equal to doubly magic nuclei. We have investigated cluster decay of isotopes of He, Li, Be, Ne, N, Mg, Si, P, S, Cl, Ar and Ca in the superhaevy nuclei region 299-306122. We have also compared the logarithmic half-lives of cluster decay with that of other models such as Univ [1], NRDX [2], UDL [3] and Horoi [4]. From this study it is concluded that  cluster decay of 4He, 22Ne, 26Mg, 28Si 30Si, 34S, 40Ca and 46Ca are having shorter logarithmic half-lives compared to exotic cluster decay modes.


2014 ◽  
Vol 89 (6) ◽  
Author(s):  
Xiao Jun Bao ◽  
Hai Fei Zhang ◽  
Jian Min Dong ◽  
Jun Qing Li ◽  
Hong Fei Zhang

2016 ◽  
Vol 367 ◽  
pp. 13-32 ◽  
Author(s):  
Emil Ryberg ◽  
Christian Forssén ◽  
H.-W. Hammer ◽  
Lucas Platter
Keyword(s):  

2004 ◽  
Vol 19 (32) ◽  
pp. 2437-2443 ◽  
Author(s):  
HUA GUO ◽  
YINHUA LIANG ◽  
XIGUO LI ◽  
YUXIN LIU ◽  
BO LIU

The results for the nuclear-matter properties in a chiral hadronic model have been compared with those in the nonlinear Walecka model. It has been found that the scalar and the vector potentials and binding energies per nucleon for nuclear matter in the chiral hadronic model are very close to those of the RBHF. Two-proton halo in 27 S and one-proton halo in 26 P are predicted when the chiral hadronic model is extended to study proton halos in light proton-rich nuclei. Comparison between the results obtained in the chiral hadronic model and in the nonlinear Walecka model has been made, it has been shown that the chiral hadronic model can also be used to describe the properties of light proton-rich nuclei.


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