Low-energy $^{3}$He($\alpha,\gamma$)$^{7}$Be reaction within the Skyrme potential framework
Nguyen Le Anh, Nguyen Gia Huy, Dao Nhut Anh, Do Huy Tho, Hoang Thai An

TL;DR
This study employs a microscopic Skyrme Hartree-Fock potential model to accurately describe low-energy elastic scattering and compute the astrophysical S factor for the $^{3}$He($ alpha, gamma$)$^{7}$Be reaction, crucial in astrophysics.
Contribution
It introduces a unified microscopic potential framework derived from Skyrme HF calculations to model both scattering and radiative capture processes in light nuclei.
Findings
Reproduces low-energy phase shifts for p+α and $^{3}$He+α.
Calculates $S_{34}(0)$ in agreement with experimental data.
Shows moderate sensitivity of $S_{34}(0)$ to projectile density.
Abstract
\textbf{Background:} The He()Be reaction plays a crucial role in the proton-proton chain and Big Bang nucleosynthesis, affecting solar neutrino fluxes and primordial element abundances. Experimental data at astrophysical energies remain uncertain due to the extremely low cross sections. \\ \textbf{Purpose:} This work uses a microscopic potential-model approach to construct the He+ potential from the nucleon+ interaction, aiming to describe low-energy elastic scattering and to calculate the astrophysical factor of the He()Be reaction. \\ \textbf{Method:} The nucleon-nucleus potential is derived from self-consistent Skyrme Hartree-Fock (HF) calculations extended to the continuum. The He+ potential is then obtained by folding the HF potential with the He density. A small number of scaling…
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