The fusion-fission reaction mechanism leading to the massive nucleus format
ion is studied. We investigate the superheavy nucleus formation in heavy-io
n induced reactions by analysing the evaporation residue (ER) production in
order to study the fusion dynamics and the decay properties of nuclei clos
e to the stability island at Z = 114. We consider the Ni-64 + Pb-208, Ca-48
+ U-238 and Ca-48 + Pu-244 reactions that lead to the Z = 110, 112 and 114
superheavy elements respectively.
By using the dinuclear system (DNS) concept of the two interacting nuclei w
e calculate the quasifission-fusion competition in the entrance channel and
the fission-evaporation competition along the de-excitation cascade of the
compound nucleus. The dynamics of the entrance channel allows us to determ
ine the beam energy window which is favorable to the fusion, while the dyna
mic evolution of the compound nucleus on the shell correction to the fissio
n barrier and the dissipative effects influence the fission-evaporation com
petition in order to obtain the residue nuclei from the superheavy nucleus
formation. We also calculate the Gamma(n)/Gamma(tot) ratio at each step of
the de-excitation cascade of the compound nucleus and we present a systemat
ics of Gamma(n)/Gamma(tot) (at first step of the cascade) for many reaction
s that lead to nuclei with Z = 102-114.