194 research outputs found
Alpha decay chains study for the recently observed superheavy element Z=117 within the Isospin Cluster Model
The recently observed -decay chains were produced by
the fusion reactions with target and projectile at Dubna
in Russia. The reported cross-sections for the mentioned reaction are
pb and =1.3(+1.5,-0.6) at and
, respectively. The Q-values of -decay and the half-lives
(s) are calculated for the -decay chains of
nuclei, within the framework of Isospin Cluster Model (ICM). In
the ICM model the proximity energy is improved by using the isospin dependent
radius of parent, daughter and alpha particle. The binding energy (i=1,2) of any nucleus of mass number A and atomic number Z was
obtained from a phenomenological and more genaralized BW formula given by
\cite{samanta02}. The calculated results in ICM are compared with the
experimental results and other theoretical Macro-Microscopic(M-M), RMF(with NL3
and SFU Gold forces parameter) model calculations. The estimated values of
-decay half-lives are in good agreement with the recent data. The ICM
calculation is in favor of the persence of magic number at N=172
Superheavy Nuclei in the Relativistic Mean Field Theory
We have carried out a study of superheavy nuclei in the framework of the
Relativistic Mean-Field theory. Relativistic Hartree-Bogoliubov (RHB)
calculations have been performed for nuclei with large proton and neutron
numbers. A finite-range pairing force of Gogny type has been used in the RHB
calculations. The ground-state properties of very heavy nuclei with atomic
numbers Z=100-114 and neutron numbers N=154-190 have been obtained. The results
show that in addition to N=184 the neutron numbers N=160 and N=166 exhibit an
extra stability as compared to their neighbors. For the case of protons the
atomic number Z=106 is shown to demonstrate a closed-shell behavior in the
region of well deformed nuclei about N=160. The proton number Z=114 also
indicates a shell closure. Indications for a doubly magic character at Z=106
and N=160 are observed. Implications of shell closures on a possible synthesis
of superheavy nuclei are discussed.Comment: 29 pages Latex, 13 ps figures, to appear in Nucl. Phys.
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