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 …

We present new calculations of the astrophysical S factor and reaction rate for the Li 6 (p, γ)
Be 7 reaction at energies of 10 keV to 5 MeV in the framework of a modified potential cluster …

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 …

Extended tables are presented for spectroscopic factors, asymptotic normalization
coefficients and rms radii of one-nucleon overlap functions for 0 p-shell nuclei calculated in …

This work is aimed at clarifying the contribution of the proton direct radiative capture to the
12 C (p, γ) 13 N reaction by specifying the value of the asymptotic normalization coefficient …

The theoretical uncertainties of single proton transfer cross sections of the (3 He, d) and (d, 3
He) reactions, owing to the uncertainties of the entrance-and exit-channel optical model …

The proton transfer Be 7 (d, n) B 8 reaction at the energy of 4.5 MeV (center of mass) has
been analyzed within the modified distorted-wave Born approximation. New estimates and …

The angular distributions of^ 13 13 C elastically scattered by^ 9 9 Be nuclei were measured
at E_ Lab E Lab (^ 13 13 C)= 16.25 and 19.5 MeV. The measured angular distributions were …

The'lithium problem'in Big Bang nucleosynthesis (BBN) has recently focused on reactions
involving 7 Be. The 6 Li (${\rm {p}},{\rm {\gamma}} $) 7 Be reaction can provide us not only …

This paper reports on 4He elastic scattering by 6, 7 Li, 9Be and 1 1 B angular distributions
analyzed in the optical model (OM) context using Woods–Saxon (WS) potential form and …