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The 6Li(p, α)3He reaction important for nuclear astrophysics is studied in the framework of a microscopic approach based on a multichannel algebraic version of the resonating group model. Astrophysical S-factor for the reaction is calculated at low energies. The obtained result is compared with experimental data and other theoretical calculations

Microscopic Study of the 6Li(p, α)3He Reaction at Low Energies

Microscopic Study of the ⁶Li(p, α)³He Reaction at Low Energies