Radiative capture in the $^{4}$He + $^{2}$H system in the framework of a microscopic approach

Not scheduled
25m
Online

Online

Oral report Section 2. Experimental and theoretical studies of nuclear reactions. Will not participate

Speaker

Dr Alexander Solovyev (Dukhov Automatics Research Institute (VNIIA))

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 cluster aspects of nuclear structure and dynamics and formalism of expansions over the oscillator basis. Cross section and astrophysical S factor of the reaction are calculated. Low-energy dependence of these quantities serves as a source of information that can be useful for the so-called second “lithium puzzle”. A comparison of the calculated results with experimental data is performed.

  1. A.S. Solovyev and S.Yu. Igashov, Phys. Rev. C 96, 064605 (2017).
  2. A.S. Solovyev and S.Yu. Igashov, Phys. Rev. C 99, 054618 (2019).

Primary author

Dr Alexander Solovyev (Dukhov Automatics Research Institute (VNIIA))

Presentation materials

There are no materials yet.