Astrophys.J. 941, 96 (2022)

M.La Cognata, S.Palmerini, P.Adsley, F.Hammache, A.Di Pietro, P.Figuera, F.Dell'Agli, R.Alba, S.Cherubini, G.L.Guardo, M.Gulino, L.Lamia, D.Lattuada, C.Maiolino, A.Oliva, R.G.Pizzone, P.M.Prajapati, G.G.Rapisarda, S.Romano, D.Santonocito, R.Sparta, M.L.Sergi, A.Tumino, P.Ventura

A New Reaction Rate of the ²⁷Al(p/α)²⁴Mg Reaction Based on Indirect Measurements at Astrophysical Energies and Implications for ²⁷Al Yields of Intermediate-mass Stars

NUCLEAR REACTIONS ²H(²⁷Al, α²⁴Mg), E=80 MeV; measured reaction products. ²⁸Si, ²⁴Mg; deduced σ(θ), σ(θ, E), resonance strengths. Comparison with Monte Carlo code RatesMC. Indirect Trojan Horse Method (THM), the INFN-LNS Tandem (Catania, Italy).

doi: 10.3847/1538-4357/ac9c5e