NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = M.Dessalvi Found 3 matches. 1999BO23 Phys.Rev.Lett. 82, 5205 (1999) R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, A.D'Alessandro, M.Dessalvi, A.D'Onofrio, A.Fubini, G.Gervino, L.Gialanella, U.Greife, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, P.Prati, V.Roca, C.Rolfs, M.Romano, F.Schuemann, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli, and the LUNA Collaboration First Measurement of the 3He(3He, 2p)4He Cross Section Down to the Lower Edge of the Solar Gamow Peak NUCLEAR REACTIONS 3He(3He, 2p), E(cm)=16.5-24.4 keV; measured σ, astrophysical S-factor; deduced electron screening effect, no narrow resonance.
doi: 10.1103/PhysRevLett.82.5205
1999PR12 Nucl.Phys. (Supplement) A654, 920c (1999) P.Prati, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, A.D'Alessandro, M.Dessalvi, A.D'Onofrio, A.Fubini, G.Gervino, L.Gialanella, U.Greife, A.Guglielmetti, C.Gustavino, M.Junker, A.Ordine, V.Roca, C.Rolfs, M.Romano, F.Schuemann, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli The LUNA Facility at the National Laboratory of Gran Sasso: Recent results and future activities NUCLEAR REACTIONS 3He(3He, 2p), E(cm)=16-25 keV; measured astrophysical S-factors, upper limits. Plans for future experiments discussed.
doi: 10.1016/S0375-9474(00)88573-5
1998ST20 Eur.Phys.J. A 3, 1 (1998) F.Strieder, F.Schumann, L.Gialanella, U.Greife, D.Rogalla, C.Rolfs, H.P.Trautvetter, Zs.Fulop, G.Gyurky, E.Somorjai, R.W.Kavanagh, L.Campajola, A.D'Onofrio, A.Ordine, V.Roca, M.Romano, F.Terrasi, C.Arpesella, A.D'Alessandro, C.Gustavino, M.Junker, O.Straniero, P.Corvisiero, M.Dessalvi, P.Prati, S.Zavatarelli, C.Broggini, G.Gervino, A.Fubini, E.Bellotti, R.Bonetti, A.Guglielmetti Loss of 8Li Recoil Nuclei in 7Li(d, p)8Li and Implications on the 7Be(p, γ)8B Cross Section NUCLEAR REACTIONS 7Li(d, p), E=0.4-1.8 MeV; measured yields; deduced recoil loss for several backing materials. 7Be(p, γ), E not given; deduced possible corrections to σ. Astrophysical implications.
doi: 10.1007/s100500050141
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