Speaker
Description
The nuclear $^4$He + $^2$H system is of great importance to nuclear astrophysics. Radiative capture proceeding in this system is responsible for production of the $^6$Li nuclei during the primordial nucleosynthesis. In this work, the $^4$He + $^2$H radiative capture is considered from the microscopic viewpoint within a developed approach [1, 2] based on clustering aspects of nuclear structure and dynamics and formalism of expansions over the oscillator basis. The cross section in terms of the astrophysical $S$ factor for the reaction are calculated. The low-energy dependence of the astrophysical $S$ factor serves as a source of information useful for the so-called second “lithium puzzle”. A comparison of the calculated results with experimental data is performed.
- A.S. Solovyev and S.Yu. Igashov, Phys. Rev. C 96, 064605 (2017).
- A.S. Solovyev and S.Yu. Igashov, Phys. Rev. C 99, 054618 (2019).