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arXiv · 2401.04281

Comments to the paper "Detailed study of the astrophysical direct capture reaction $^6$Li($p,\gamma$)$^7$Be in a potential model approach" by E. M. Tursunov, S. A. Turakulov, and K. I. Tursunmakhatov, PHYSICAL REVIEW C 108, 065801 (2023)

S. B. Dubovichenko·A. S. Tkachenko·R. Ya. Kezerashvili
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Abstract

We explicitly present the comparison of the results for the astrophysical S-factor and reaction rate for the $^6$Li($p,\gamma$)$^7$Be capture process at astrophysical energies, presented in Phys. Rev. Phys. Rev. C 105, 065806 (2022) and Phys. Rev. C 108. 065801 (2023) obtained within the famework of potential models. We demonstrate that both potential model approaches describe successfully the astrophysical S-factor and reaction rate simultaneously and reproduce the LUNA Collaboration [Phys. Rev. C 102, 052802(R) (2020)] results.

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S. B. Dubovichenko, A. S. Tkachenko, R. Ya. Kezerashvili. 2024-01-08. Comments to the paper "Detailed study of the astrophysical direct capture reaction $^6$Li($p,\gamma$)$^7$Be in a potential model approach" by E. M. Tursunov, S. A. Turakulov, and K. I. Tursunmakhatov, PHYSICAL REVIEW C 108, 065801 (2023). https://arxiv.org/abs/2401.04281

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