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Investigating the astrophysical22Ne(p,γ)23Na and22Mg(p,γ)23Al reactions with a multi-channel scattering formalism
EPJ Web of Conferences
The reaction 22 Ne(p, γ) 23 Na is key to the NeNa cycle of stellar nucleogenesis, and better understanding of the 22 Mg(p, γ) 23 Al reaction is needed to understand the 22 Na puzzle in ONe white dwarf novae. We aim to study these reactions using a multi-channel algebraic scattering (MCAS) formalism for low-energy nucleon-nucleus scattering, recently expanded to investigate radiative capture. As a first step towards this goal, we here calculate the energy levels of the mass-23 (Ne, Mg, Na, Al)doi:10.1051/epjconf/20146603030 fatcat:skciqnh5bjdd3cedznj76ybobu