NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = F.Gorris Found 4 matches. 1999BO29 Eur.Phys.J. A 5, 327 (1999) L.Borucki, H.W.Becker, F.Gorris, S.Kubsky, W.H.Schulte, C.Rolfs Hydrogen Doppler Spectroscopy using 15N Ions NUCLEAR REACTIONS 20,22Ne(p, γ), 4He(7Li, γ), (11B, γ), (14N, γ), (16O, γ), E not given; measured resonance γ-ray yields; deduced atomic, molecular beams energy spreads. 20Ne(p, p), (p, p'), E=3552 keV; measured proton spectra; deduced resonance features.
doi: 10.1007/s100500050291
1995GR07 Z.Phys. A351, 107 (1995) U.Greife, F.Gorris, M.Junker, C.Rolfs, D.Zahnow Oppenheimer-Phillips Effects and Electron Screening in d + d Fusion Reactions NUCLEAR REACTIONS, ICPND 2H(d, n), (d, p), E(cm)=1.6-130 keV; measured σ(E) ratio spectra, astrophysical S-factor vs E for 2H(d, p); deduced no Oppenheimer-Phillips effect evidence.
doi: 10.1007/BF01292792
1994GR33 Nucl.Instrum.Methods Phys.Res. A350, 327 (1994) U.Greife, C.Arpesella, C.A.Barnes, F.Bartolucci, E.Bellotti, C.Broggini, P.Corvisiero, G.Fiorentini, A.Fubini, G.Gervino, F.Gorris, C.Gustavino, M.Junker, R.W.Kavanagh, A.Lanza, G.Mezzorani, P.Prati, P.Quarati, W.S.Rodney, C.Rolfs, W.H.Schulte, H.P.Trautvetter, D.Zahnow Laboratory for Underground Nuclear Astrophysics (LUNA) NUCLEAR REACTIONS, ICPND 2H(d, n), (d, p), E=10 keV; 2H(3He, p), E=70 keV; measured spectra. 2H(3He, p), E ≤ 40 keV; 3He(3He, 2p), E ≤ 160 keV; measured astrophysical S-factor vs E. Windowless gas target system, close geometry detector telescopes.
doi: 10.1016/0168-9002(94)91182-7
1994PR09 Z.Phys. A350, 171 (1994) P.Prati, C.Arpesella, F.Bartolucci, H.W.Becker, E.Bellotti, C.Broggini, P.Corvisiero, G.Fiorentini, A.Fubini, G.Gervino, F.Gorris, U.Greife, C.Gustavino, M.Junker, C.Rolfs, W.H.Schulte, H.P.Trautvetter, D.Zahnow Electron Screening in the d + 3He Fusion Reaction NUCLEAR REACTIONS, ICPND 2H(3He, p), E(cm)=5.4-31.3 keV; measured spectra, astrophysical S-factor; deduced electron screening potential. Windowless gas target system.
doi: 10.1007/BF01290685
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