Many-channel microscopic theory of resonance states and scattering processes in 9Be and 9B
Abstract
We present a many-channel microscopic model that extends the three-cluster model previously formulated in 2009NPA...V37. This extended model incorporates multiple three-cluster configurations, which are subsequently reduced to a comprehensive set of binary channels. These channels dictate the dynamics of various nuclear processes and the resonance structure of a compound nucleus across a broad energy spectrum. The application of this model focuses on investigating the nature of high-energy resonance states in 9Be and 9B, as well as the astrophysical S-factors for the reactions 7Li(d,n)αα and 7Be(d,p)αα, particularly pertinent to the cosmological lithium problem. Parameterization of resonance states is performed across a wide range of total angular momenta and includes states of both positive and negative parity. Dominant decay channels are identified for each resonance state. Detailed analysis of astrophysical S factors resulting from deuteron interactions with 7Li and 7Be is conducted within an energy range from zero to 2 MeV. Four exit channels in 9Be (8Be(0+)+n, 8Be(2+)+n, 5He(3/2-)+α, 5He(1/2-)+α) and four in 9B (8Be(0+)+p, 8Be(2+)+p, 5Li(3/2-)+α, 5Li(1/2-)+α) are considered. A clear hierarchy of reactions is established for the energy range 0≤ E<1.0 MeV. Notably, reactions 7Li+d=8Be(0+)+n and 7Be+d=8Be(0+)+p substantially dominate over all other reactions within this energy range. The model satisfactory describes the experimental astrophysical S factors for these reactions.
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