Abstract
Theoretical estimates for the astrophysical S-factor and the rate of the reaction d(α, γ)6Li were obtained on the basis of the two-body model involving an α−d potential that has a simple Gaussian form and which describes correctly S-, P-, and D-wave phase shifts, the binding energy, and the asymptotic normalization coefficient for the S-wave bound state. The wave functions for the bound and continuum channels were calculated with the aid of the highly precise Numerov algorithm. The results for the contributions of the E1 and E2 transition components reveal a good convergence as the upper limit in the effective integrals increases up to 40 fm. The results obtained for the astrophysical S-factor and the rate of the reaction d(α, γ)6Li in the temperature range of 106 K ≤ T ≤ 1010 K agree well with the results of the calculations performed by A.M. Mukhamedzhanov and his coauthors [Phys. Rev. C 83, 055805 (2011)] by using the known asymptotic form of the wave function at low energies and a complicated two-body potential at higher energies.
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Tursunov, E.M., Turakulov, S.A. & Descouvemont, P. Theoretical analysis of the astrophysical S-factor for the capture reaction α + d → 6Li + γ in the two-body model. Phys. Atom. Nuclei 78, 193–200 (2015). https://doi.org/10.1134/S1063778815010196
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DOI: https://doi.org/10.1134/S1063778815010196