Asymptotic normalization coefficient for α+d →<sup>6</sup>Li from the peripheral direct capture d(α,γ)<sup>6</sup>reaction and the astrophysical<i>S</i>factor at Big Bang energies
K. I. TursunmakhatovDepartment of Physics and Mathematics of Gulistan State University, 120100 Gulistan, UzbekistanR. YarmukhamedovInstitute of Nuclear Physics, 100214 Tashkent, UzbekistanS. B. IgamovInstitute of Nuclear Physics, 100214 Tashkent, Uzbekistan
ABI
Annotatsiya
The results of the analysis of the new experimental astrophysical S factors S exp 24 (E) [D. Trezzi, et al., Astropart. Phys. 89 , 57 (2017)] and those measured earlier [R. G. Robertson, et al., Phys. Rev. Lett. 47 , 1867 (1981)] for the nuclear-astrophysical d(α,γ) 6 Li reaction directly measured at extremely low energies E , are presented. New estimates and their uncertainties have been obtained for values of the asymptotic normalization coefficient for α + γ → 6 Li and for the direct astrophysical S factors at Big Bang energies.
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