In the present work, the results of the analysis of the experimental astrophysical $S$ factors (AS) $S^{\exp}(E)$ [1,2] for the nuclear-astrophysical $d(\alpha,\gamma){}^6{\rm Li}$ reaction directly measured at extremely low energies E are presented. One notes that the $d(\alpha,\gamma){}^6{\rm Li}$ reaction is of great interest as one of the sources of the 6Li creation in the early...
One of the most interesting problems in heavy-ion physics is an identification of the reactions which are called deep-inelastic collisions, quasifission and fusion-fission. These reactions are called binary reactions and their mechanisms are in competition to synthesis of superheavy elements in the different stages of formation of evaporation residue which is considered as a superheavy...
The astrophysical S-factor and reaction rates of the direct capture processes $^3$He(α, γ)$^7$Be and $^3$H(α, γ)$^7$Li, as well as the abundance of the $^7$Li/H element are studied in the framework of the two-body model with potentials of a simple Gaussian form, which describe correctly the phase shifts in the s, p, d, and f waves, as well as the binding energy and the asymptotic normalization...
