NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = D.Zahnow Found 16 matches. 1998JU03 Phys.Rev. C57, 2700 (1998) M.Junker, A.D'Alessandro, S.Zavatarelli, C.Arpesella, E.Bellotti, C.Broggini, P.Corvisiero, G.Fiorentini, A.Fubini, G.Gervino, U.Greife, C.Gustavino, J.Lambert, P.Prati, W.S.Rodney, C.Rolfs, F.Strieder, H.P.Trautvetter, D.Zahnow, and the Luna Collaboration Cross Section of 3He(3He, 2p)4He Measured at Solar Energies NUCLEAR REACTIONS 3He(3He, 2p), E=20.76-91.70 keV; measured σ; deduced astrophysical S factor, electron screening effect, no evidence for low-energy resonance.
doi: 10.1103/PhysRevC.57.2700
1997GR11 Nucl.Phys. A621, 603c (1997) U.Greife, C.Arpesella, E.Bellotti, K.Brand, C.Broggini, L.Campajola, P.Corvisiero, A.D'Onofrio, G.Fiorentini, A.Fubini, G.Gervino, L.Gialanella, C.Gustavino, E.Huttel, M.Junker, R.W.Kavanagh, R.Kubat, J.Lambert, G.Oliviero, P.Prati, H.Rebel, V.Roca, W.S.Rodney, C.Rolfs, M.Romano, M.Romoli, S.Schmidt, W.H.Schulte, F.Strieder, F.Terrasi, H.P.Trautvetter, D.Zahnow, S.Zavatarelli Further Direct Approaches to the Nuclear Reactions in the Sun
doi: 10.1016/S0375-9474(97)00312-6
1997ST19 Nucl.Phys. A621, 123c (1997) F.Strieder, L.Campajola, A.D'Onofrio, L.Gialanella, U.Greife, V.Roca, C.Rolfs, M.Romano, M.Romoli, S.Schmidt, W.H.Schulte, H.P.Trautvetter, D.Zahnow The d(7Li, p)8Li Cross Section Near E(cm) = 0.61 MeV NUCLEAR REACTIONS, ICPND 2H(7Li, 8Li), E=0.47-4 MeV; measured recoil β-delayed α-decay spectra; deduced σ.
doi: 10.1016/S0375-9474(97)00222-4
1997ZA06 Z.Phys. A359, 211 (1997) D.Zahnow, C.Rolfs, S.Schmidt, H.P.Trautvetter Low-Energy S(E) Factor of 9Be(p, α)6Li and 9Be(p, d)8Be NUCLEAR REACTIONS, ICPND 9Be(p, α), (p, d), E=16-390 keV; measured astrophysical S-factors, σ(θ). 10B deduced resonances E, Γ.
doi: 10.1007/s002180050389
1996AR16 Phys.Lett. 389B, 452 (1996) C.Arpesella, E.Bellotti, C.Broggini, P.Corvisiero, G.Fiorentini, A.Fubini, G.Gervino, U.Greife, C.Gustavino, M.Junker, J.Lambert, P.Prati, W.S.Rodney, C.Rolfs, H.P.Trautvetter, D.Zahnow, S.Zavatarelli Measurement of the 3He(3He, 2p)4He Cross Section within the Solar Gamow Peak NUCLEAR REACTIONS, ICPND 3He(3He, 2p), E=20.7-91.7 keV; measured astrophysical S-factor vs E; deduced no evidence for hypothetical resonance.
doi: 10.1016/S0370-2693(96)01326-3
1996AR23 Nucl.Phys. B(Proc.Suppl.) S48, 375 (1996) C.Arpesella, F.Bartolucci, E.Bellotti, C.Broggini, P.Corvisiero, G.Fiorentini, A.Fubini, G.Gervino, U.Greife, C.Gustavino, M.Junker, P.Prati, C.Rolfs, H.P.Trautvetter, D.Zahnow, S.Zavatarelli Status of the LUNA Experiment
doi: 10.1016/0920-5632(96)00275-7
1996CA43 Z.Phys. A356, 107 (1996) L.Campajola, L.Gialanella, K.Brand, A.D'Onofrio, U.Greife, E.Huttel, R.Kubat, G.Oliviero, H.Rebel, V.Roca, C.Rolfs, M.Romano, M.Romoli, S.Schmidt, W.H.Schulte, F.Strieder, F.Terrasi, H.-P.Trautvetter, D.Zahnow Production of an 8.0 MeV 7Be Ion Beam at the Naples TTT-3 Accelerator NUCLEAR REACTIONS 1H(7Be, γ), E=8 MeV; measured residual nuclei production. Radioactive beam from 7Li(p, n) reaction.
doi: 10.1007/s002180050154
1996GI11 Nucl.Instrum.Methods Phys.Res. A376, 174 (1996) L.Gialanella, F.Strieder, K.Brand, L.Campajola, A.D'Onofrio, U.Greife, E.Huttel, F.Petrazzuolo, V.Roca, C.Rolfs, M.Romano, M.Romoli, S.Schmidt, W.H.Schulte, F.Terrasi, H.P.Trautvetter, D.Zahnow A Recoil Separator for the Measurement of Radiative Capture Reactions NUCLEAR REACTIONS 1H(12C, γ), E=2, 11 MeV; measured Eγ, Iγ; deduced absolute reaction σ. Recoil separator plus windowless gas target.
doi: 10.1016/0168-9002(96)00264-1
1996ST18 Z.Phys. A355, 209 (1996) F.Strieder, L.Gialanella, U.Greife, C.Rolfs, S.Schmidt, W.H.Schulte, H.P.Trautvetter, D.Zahnow, F.Terrasi, L.Campajola, A.D'Onofrio, V.Roca, M.Romano, M.Romoli The d(7Li, p)8Li Cross Section Near E(cm) = 0.61 MeV NUCLEAR REACTIONS, ICPND 2H(7Li, p), E(cm) ≈ 0.61 MeV; measured proton yield, β-delayed α-activity of residual 8Li. 2H(7Li, p), E(cm)=0.5-0.75 MeV; measured σ(θ); deduced absolute σ(E), consequences for expected flux of high energy solar neutrinos.
doi: 10.1007/s002180050100
1995AR31 Nucl.Instrum.Methods Phys.Res. A360, 607 (1995) C.Arpesella, E.Bellotti, C.Broggini, P.Corvisiero, A.Fubini, G.Gervino, U.Greife, C.Gustavino, M.Junker, A.Lanza, P.Prati, C.Rolfs, D.Zahnow, S.Zavatarelli A Monte Carlo Code for Nuclear Astrophysics Experiments NUCLEAR REACTIONS 3He(d, p), (3He, 2p), E=153 keV; 2H(d, X), 9Be(p, X), E not given; analyzed spectra. Monte Carlo code for astrophysical applications, ion energy, angular straggling, Doppler broadening effects accurately evaluated.
doi: 10.1016/0168-9002(95)00038-0
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
1995ZA03 Z.Phys. A351, 229 (1995) D.Zahnow, C.Angulo, C.Rolfs, S.Schmidt, W.H.Schulte, E.Somorjai The S(E) Factor of 7Li(p, γ)8Be and Consequences for S(E) Extrapolation in 7Be(p, γ0)8B NUCLEAR REACTIONS, ICPND 7Li(p, γ), E=100-1500 keV; measured Eγ, Iγ(θ) ratios; deduced σ(E), astrophysical S-factor vs E, capture mechanism. 8Be deduced resonance energy, Γ.
doi: 10.1007/BF01289534
1995ZA04 Nucl.Phys. A589, 95 (1995) D.Zahnow, C.Angulo, M.Junker, C.Rolfs, S.Schmidt, W.H.Schulte, E.Somorjai Thermonuclear Reaction Rates of 9Be(p, γ)10B NUCLEAR REACTIONS, ICPND 9Be(p, γ), E=75-1800 keV; measured Eγ, Iγ; deduced σ(E), thermonuclear reaction rates, astrophysical S-factor.
doi: 10.1016/0375-9474(95)00077-E
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
1993AN09 Z.Phys. A345, 333 (1993) C.Angulo, W.H.Schulte, D.Zahnow, G.Raimann, C.Rolfs Astrophysical S(E) Factor of 10B(p, α1)7Be at Low Energies NUCLEAR REACTIONS, ICPND 10B(p, α), E(cm)=48-159 keV; measured absolute fusion σ, astrophysical S-factor vs E. γ-spectroscopic techniques.
doi: 10.1007/BF01280844
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