Nur Mohammad¹, Md. Rabiul Islam¹, Hajera Sultana², Md. Abdul Khan^2
1Department of Physics, Raiganj University, Raiganj, Uttar Dinajpur, WB-733134, India
²Department of Physics, Aliah University, IIA/27, Newtown, Kolkata-700160, India

Abstract. Nuclear fusion reactions at sub-barrier energies play crucial roles in many aspects of primordial nucleosynthesis in stellar objects. One of the primary aspects that plays a pivotal role in understanding the relationship between stellar evolution and nuclear reaction dynamics is the energy dependence of astronuclear observables, such as the fusion cross-section σ. This paper presents the results of a few ³He-induced nuclear fusion reactions-³He(³He,2p)⁴He, ⁶Li(³He,d)⁷Be and ¹⁰B(³He,n)¹²N which are investigated adopting the single-step selective resonant tunnelling model (SRTM). As an improvement over earlier works, the authors have used a microscopically derived density-dependent double-folding potential model, invoking the M3Y-Reid NN interactions, for the numerical computation of the astrophysical S-factor, S(E), and the fusion cross-section, σ. The results of the calculations have been compared with those found in the literature. The results obtained in the present studies agree fairly with the experimentally observed results found in the literature.

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