Towards an ab initio description of the light-nuclei radiative captures
Abstract
The 3 He(α,γ)7 Be and 3 H(α,γ)7 Li astrophysical S factors are evaluated at low collision energies (less than 2.5 MeV in the centre-of-mass frame) within the no-core shell model with continuum approach using a renormalized chiral nucleon-nucleon interaction.
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