Comment on detailed study of the astrophysical direct capture reaction Li 6 (p,γ) Be 7 in a potential model approach
Dubovichenko S.B. Tkachenko A.S. Kezerashvili R.Y.
November 2024American Physical Society
Physical Review C
2024#110Issue 5
We explicitly present the comparison of the results for the astrophysical S factor and reaction rate for the Li6(p,γ)Be7 capture process at astrophysical energies, presented by Dubovichenko et al. [Phys. Rev. C 105, 065806 (2022)2469-998510.1103/PhysRevC.105.065806] and Tursunov et al. [Phys. Rev. C 108, 065801 (2023)2469-998510.1103/PhysRevC.108.065801] obtained within the framework 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)10.1103/PhysRevC.102.052802] results.
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Fesenkov Astrophysical Institute, Almaty, 050020, Kazakhstan
New York City College of Technology, City University of New York, Brooklyn, 11201, NY, United States
Graduate School and University Center, City University of New York, New York, 10016, United States
Fesenkov Astrophysical Institute
New York City College of Technology
Graduate School and University Center
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