NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = J.Vise Found 8 matches. 1994GI01 Nucl.Phys. A567, 146 (1994) U.Giesen, C.P.Browne, J.Gorres, J.G.Ross, M.Wiescher, R.E.Azuma, J.D.King, J.B.Vise, M.Buckby The Influence of Low-Energy Resonances on the Reaction Rate of 18O(α, γ)22Ne NUCLEAR REACTIONS, ICPND 18O(6Li, 6Li), (6Li, d), E=32 MeV; measured σ(θ); deduced model parameters. 18O(α, γ), E < 1 MeV; measured γ(θ). 18O(p, γ), E ≈ resonance; measured thick target yield curve. 22Ne deduced resonances, J, π, spectroscopic factors, role in 18O(α, γ) reaction rate.
doi: 10.1016/0375-9474(94)90731-5
1994KI02 Nucl.Phys. A567, 354 (1994) J.D.King, R.E.Azuma, J.B.Vise, J.Gorres, C.Rolfs, H.P.Trautvetter, A.E.Vlieks Cross Section and Astrophysical S-Factor for the 13C(p, γ)14N Reaction NUCLEAR REACTIONS, ICPND 13C(p, γ), E=120-950 keV; measured γ-ray yield 14N. 13C(p, γ), E=120-950 keV; calculated astrophysical S-factor, thermonuclear reaction rate. 14N deduced resonance parameters, branching ratios, direct capture contributions, spectroscopic factors for proton-bound states.
doi: 10.1016/0375-9474(94)90154-6
1990GR04 Nucl.Phys. A510, 346 (1990) S.Graff, J.Gorres, M.Wiescher, R.E.Azuma, J.King, J.Vise, G.Hardie T.R.Wang Proton Capture on 28Si and Its Astrophysical Implications NUCLEAR REACTIONS, ICPND 28Si(p, γ), E=0.37-2.95 MeV; measured σ(E); deduced astrophysical S-factor, total reaction rate. 29P deduced resonances, resonance strengths, Γ, spectroscopic factors.
doi: 10.1016/0375-9474(90)90244-G
1987MA31 Nucl.Phys. A470, 206 (1987) P.V.Magnus, M.S.Smith, P.D.Parker, R.E.Azuma, C.Campbell, J.D.King, J.Vise Measurement of the 15N(α, γ)19F Resonances at E(cm)=536 keV and 542 keV NUCLEAR REACTIONS 15N(α, γ), E(cm)=536, 542 keV; measured Eγ, Iγ. 19F resonances deduced γ transition strength.
doi: 10.1016/0375-9474(87)90128-X
1987SC10 Nucl.Phys. A467, 240 (1987) U.Schroder, H.W.Becker, G.Bogaert, J.Gorres, C.Rolfs, H.P.Trautvetter, R.E.Azuma, C.Campbell, J.D.King, J.Vise Stellar Reaction Rate of 14N(p, γ)15O and Hydrogen Burning in Massive Stars NUCLEAR REACTIONS, ICPND 14N(p, γ), E=0.2-3.6 MeV; measured σ(E, E(γ), θ(γ)); deduced astrophysical S-factor, capture σ . 15O deduced levels, J, π, Γ, spectroscopic factors. Windowless gas, implanted 14N targets. Ge(Li) detectors.
doi: 10.1016/0375-9474(87)90528-8
1963VI06 Phys.Rev. 132, 2573 (1963) Electron-Neutrino Angular Correlation in the Decay of He6 NUCLEAR STRUCTURE 6He; measured not abstracted; deduced nuclear properties.
doi: 10.1103/PhysRev.132.2573
1961VI06 Cu(Pnpl)-213, p.17 (1961) Beta-Neutrino Angular Correlation in He6 NUCLEAR STRUCTURE 6He; measured not abstracted; deduced nuclear properties.
1958BE80 Phys.Rev. 109, 85 (1958) N.Benczer-Koller, A.Schwarzschild, J.B.Vise, C.S.Wu Determination of Electron Polarization by Electron-Electron Scattering: Y90 and Au198
doi: 10.1103/PhysRev.109.85
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