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NSR database version of April 27, 2024.

Search: Author = S.Ramano

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2022LA01      Phys.Lett. B 826, 136917 (2022)

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

Exploring the astrophysical energy range of the ²⁷Al(p, α)²⁴Mg reaction: A new recommended reaction rate

NUCLEAR REACTIONS ²H(²⁷Al, α²⁴Mg)¹NN, E<1.5 MeV; measured reaction products. ²⁸Si, ²⁴Mg; deduced σ(θ, E), strengths of the levels, astrophysical reaction rates. The indirect Trojan Horse method (THM), INFN-LNS Tandem accelerator (Catania, Italy).

doi: 10.1016/j.physletb.2022.136917
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