NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = P.G.Prada Moroni Found 7 matches. 2015LA20 Astrophys.J. 811, 99 (2015) L.Lamia, C.Spitaleri, E.Tognelli, S.Degl'Innocenti, R.G.Pizzone, P.G.Prada Moroni Astrophysical impact of the updated 9Be (p, α)6Li and 10B(p, α)7Be reaction rates as deduced by THM NUCLEAR REACTIONS 9Be, 10B(p, α), E(cm)<0.5 MeV; calculated σ, S-factors, reaction rates using Trojan Horse Method. Comparison with NACRE library.
doi: 10.1088/0004-637X/811/2/99
2014TU03 Astrophys.J. 785, 96 (2014) A.Tumino, R.Sparta, C.Spitaleri, A.M.Mukhamedzhanov, S.Typel, R.G.Pizzone, E.Tognelli, S.Degl'Innocenti, V.Burjan, V.Kroha, Z.Hons, M.La Cognata, L.Lamia, J.Mrazek, S.Piskor, P.G.Prada Moroni, G.G.Rapisarda, S.Romano, M.L.Sergi New Determination of the 2H(d, p)3H and 2H(d, n)3He Reaction Rates at Astrophysical Energies NUCLEAR REACTIONS 2H(3He, pt), E=17 MeV;2H(3He, n3He), E=18 MeV; measured reaction products, Ep, Ip; deduced σ(θ), S-factors, reaction rates, inputs for FRANEC evolutionary code. Comparison with available data.
doi: 10.1088/0004-637X/785/2/96
2013LA13 Astrophys.J. 768, 65 (2013) L.Lamia, C.Spitaleri, R.G.Pizzone, E.Tognelli, A.Tumino, S.Degl'Innocenti, P.G.Prada Moroni, M.La Cognata, L.Pappalardo, M.L.Sergi An Updated 6Li(p, α)3He Reaction Rate at Astrophysical Energies with the Trojan Horse Method NUCLEAR REACTIONS 6Li(p, α), E(cm)<1 MeV; analyzed available S-factors, reaction rates; deduced importance of this reaction for 6Li destruction in astrophysical environment.
doi: 10.1088/0004-637X/768/1/65
2001GA40 Nucl.Phys. A688, 530c (2001) D.Galli, P.G.Prada Moroni, S.Zavatarelli, F.Ferrini, F.Palla Astrophysical Implications of the New Measurements of the 3He(3He, 2p)4He Cross Section NUCLEAR REACTIONS 3He(3He, 2p), E=low; compiled, surveyed σ data, star abundance data, 3He abundance discussed.
doi: 10.1016/S0375-9474(01)00778-3
2001PR12 Nucl.Phys. A688, 572c (2001) P.G.Prada Moroni, S.Zavatarelli The Effects on Stellar Evolution of a Low Energy Resonance in the 3He + 3He Reaction NUCLEAR REACTIONS 3He(3He, 2p), E=low; surveyed σ data, calculated σ assuming hypothetical low-energy resonances, effects on solar neutrino flux and on 3He galactic abundance discussed.
doi: 10.1016/S0375-9474(01)00791-6
2001ZA07 Nucl.Phys. A688, 514c (2001) S.Zavatarelli, P.Corvisiero, H.Costantini, P.G.Prada Moroni, P.Prati, R.Bonetti, A.Guglielmetti, C.Broggini, L.Campajola, A.Formicola, L.Gialanella, G.Imbriani, A.Ordine, V.Roca, M.Romano, A.D'Onofrio, F.Terrasi, G.Gervino, C.Gustavino, M.Junker, D.Rogalla, C.Rolfs, F.Schumann, F.Strieder, H.P.Trautvetter The D(3He, p)4He Fusion Reaction: Electron screening effect and astrophysical S(E) factor at low energies NUCLEAR REACTIONS 2H(3He, p), E=4.2-13.8 keV; measured σ, S-factor. Comparison with earlier data and with calculations that include electron screening effects.
doi: 10.1016/S0375-9474(01)00773-4
2000CO17 Phys.Lett. 482B, 43 (2000) H.Costantini, A.Formicola, M.Junker, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, A.D'Onofrio, A.Fubini, G.Gervino, L.Gialanella, U.Greife, A.Guglielmetti, C.Gustavino, G.Imbriani, A.Ordine, P.G.Prada Moroni, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, F.Schumann, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli Stopping Power, Electron Screening and the Astrophysical S(E) Factor of d(3He, p)4He NUCLEAR REACTIONS 2H(3He, p), E=11-35 keV; measured σ; deduced electron screening effect, stopping power, astrophysical S factor. Gas target.
doi: 10.1016/S0370-2693(00)00513-X
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