The detection of the neutrinos produced in the p− p chain and in the CNO cycle can be used
to test the Standard Solar Model. The 3 He (α, γ) 7 Be reaction is the first reaction of the 2nd …

Background: The Li 6 (p, γ) Be 7 cross section influences a variety of astrophysical
scenarios, including big-bang and stellar nucleosynthesis. In recent years, conflicting results …

Background: The production of Be 7 and Li 7 nuclei plays an important role in primordial
nucleosynthesis, nuclear astrophysics, and fusion energy generation. The He 3 (α, γ) Be 7 …

In the present review work, the main methods of the determination of asymptotic
normalization coefficients (or respective nuclear vertex constants) for the A+ x→ B channel …

We treat low-energy 3 He–α elastic scattering in an effective field theory (EFT) that exploits
the separation of scales in this reaction. We compute the amplitude up to next-to-next-to …

A new algorithm for the asymptotic nuclear coefficients calculation, which we call the Δ
method, is proved and developed. This method was proposed by Ramírez Suárez and …

The astrophysical He 3 (α, γ) Be 7 and H 3 (α, γ) Li 7 direct capture processes are studied in
the framework of the two-body model with potentials of a simple Gaussian form, which …

We describe bound states, resonances, and elastic scattering of light ions using a δ-shell
potential. Focusing on low-energy data such as energies of bound states and resonances …

A microscopic approach to description of radiative capture reactions based on a multiscale
algebraic version of the resonating group model is developed. The main idea of the …

The observation of neutrinos emitted in the p− p chain and in the CNO cycle can be
employed to test the Standard Solar Model. The 3 He (α, γ) 7 Be reaction is the first reaction …