Fusion and decay study of Cadmium nucleus formed in Calcium induced reaction at energies lying around the Coulomb barrier

The present investigation explores the fusion-fission phenomena in the field of nuclear physics, focusing particularly on their significance in astrophysical research, namely in the nucleosynthesis process occurring in the stars. The present work intends to investigate into the formations and fragmentation mechanisms of 104 Cd* system, populated in the interaction of 40 Ca and 64 Ni ions at energies spanning the mutual electrostatic repulsion. For analysing the formation processes in complete fusion of 40 Ca+ 64 Ni channel, the fusion excitation functions are estimated via statistical CCFULL approach along with the dynamical model named as EDWSP. The dynamical effects are included via energy dependence. The fusion models suggests that it is imperative to include energy dependence and coupling effects to harmonize the experimental data. Furthermore, the Dynamical Cluster-decay Model (DCM) framework is exploited to scrutinized the fragmentation mechanism defining the decay of 104 Cd*. The decay model suggests that the structure for evaporation residues and fission fragments gets altered by the incorporation of various angular momentum states. Other parameters such as nuclear deformations and neck-length parameter also pose influence on the structural aspects of decay profiles.