arXiv · 1902.09767
$^{3}{\rm He}(α, γ)^{7}{\rm Be}$ and $^{3}{\rm H}(α,γ)^{7}{\rm Li}$ reaction rates and the implication for Big Bang nucleosynthesis in the potential model
Abstract
The reaction rates of the direct astrophysical capture processes $^{3}{\rm He}(α, γ)^{7}{\rm Be}$ and $^{3}{\rm H}(α,γ)^{7}{\rm Li}$, as well as the abundance of the $^{7}{\rm Li}$ element are estimated in the framework of a two-body potential model. The estimated $^{7}{\rm Li/H}$ abundance ratio of $^{7}{\rm Li/H}=(5.07\pm 0.14 )\times 10^{-10}$ is in a very good agreement with the recent measurement $^{7}{\rm Li/H}=(5.0\pm 0.3) \times 10^{-10}$ of the LUNA collaboration.
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S. A. Turakulov, E. M. Tursunov. 2019-02-26. $^{3}{\rm He}(α, γ)^{7}{\rm Be}$ and $^{3}{\rm H}(α,γ)^{7}{\rm Li}$ reaction rates and the implication for Big Bang nucleosynthesis in the potential model. https://doi.org/10.1142/s2010194519600140
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