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Determination of the asymptotic normalization coefficient (nuclear vertex constant) for $α + d \to^{6} Li$ $α + d \to^{6} Li$ from the new direct measured $d {(α, γ)}^{6} Li$ $d {(α, γ)}^{6} Li$ data and its implication for extrapolating the $d {(α, γ)}^{6} Li$ $d {(α, γ)}^{6} Li$ astrophysical $S$ $S$ factor at Big Bang energies

K. I. Tursunmakhatov

Physical and Mathematical Department of Gulistan State University, Gulistan 120100, Uzbekistan

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and

R. Yarmukhamedov

Institute of Nuclear Physics, Uzbekistan Academy of Sciences, Tashkent 100214, Uzbekistan

E-mail Address: rakhim@inp.uz

Corresponding author.

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https://doi.org/10.1142/S2010194519600176Cited by:1 (Source: Crossref)

This article is part of the issue:

Proceedings of the International Workshop “New Aspects of the Hadron and Astro/Nuclear Physics” Tashkent, Uzbekistan, November 5–10, 2018;
Editors: Mirzayusuf Musakhanov and Ulugbek Yakhshiev

Abstract

The results of the analysis of the new experimental astrophysical S factors $S_{24}^{exp} (E)$ $S_{24}^{exp} (E)$ [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 $d {(α, γ)}^{6} Li$ $d {(α, γ)}^{6} Li$ reaction directly measured at extremely low energies $E$ $E$ , which is derived within the modified two-body potential method, are presented. New estimates and their uncertainties have been obtained for values of the asymptotic normalization coefficient for $α + d \to^{6} Li$ $α + d \to^{6} Li$ and for the direct astrophysical $S$ $S$ factors at Big Bang energies.

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Published: 25 July 2019

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