NSR Query Results
Output year order : Descending NSR database version of April 29, 2024. Search: Author = A.Vlieks Found 9 matches. 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
1986SC21 Nucl.Phys. A457, 182 (1986) P.Schmalbrock, T.R.Donoghue, M.Wiescher, V.Wijekumar, C.P.Browne, A.A.Rollefson, C.Rolfs, A.Vlieks Proton Threshold State in 27Si and Their Implications on Hydrogen Burning of 26Al NUCLEAR REACTIONS, ICPND 28Si(3He, α), E=15 MeV; measured σ(Eα), σ(θ); deduced 26A(p, γ)27Si stellar capture σ reaction rates. 27Si deduced levels. Natural targets, magnetic spectrograph, position sensitive detectors, photographic plates.
doi: 10.1016/0375-9474(86)90526-9
1983GO21 Nucl.Phys. A408, 372 (1983) J.Gorres, H.W.Becker, L.Buchmann, C.Rolfs, P.Schmalbrock, H.P.Trautvetter, A.Vlieks, J.W.Hammer, T.R.Donoghue Proton-Induced Direct Capture on 21Ne and 22Ne NUCLEAR REACTIONS, ICPND 22Ne(p, p), E=0.6-1.6 MeV; measured σ(θ=145°)/σ(Rutherford) vs E. 21,22Ne(p, γ), E=0.3-1.6 MeV; measured Eγ, Iγ, σ(E, θγ); deduced direct capture σ, astrophysical reaction rates. 22Na resonances deduced γ transition strength. 23Na levels deduced spectroscopic factors, γ transition strength. Extended quasipoint jet gas targets, Ge(Li) detectors.
doi: 10.1016/0375-9474(83)90588-2
1983WI09 Phys.Rev. C28, 1431 (1983) M.Wiescher, R.N.Boyd, S.L.Blatt, L.J.Rybarcyk, J.A.Spizuoco, R.E.Azuma, E.T.H.Clifford, J.D.King, J.Gorres, C.Rolfs, A.Vlieks 11C Level Structure via the 10B(p, γ) Reaction NUCLEAR REACTIONS, ICPND 10B(p, γ), E=0.07-2.2 MeV; measured Eγ, Iγ, γ yield, capture σ vs E, γ(θ); deduced direct capture contributions. 11C deduced resonances, J, π, Γ, γ-branching ratios, Γγ/Γ.
doi: 10.1103/PhysRevC.28.1431
1982KE10 Z.Phys. A308, 73 (1982) K.U.Kettner, H.W.Becker, L.Buchmann, J.Gorres, H.Krawinkel, C.Rolfs, P.Schmalbrock, H.P.Trautvetter, A.Vlieks The 4He(12C, γ)16O Reaction at Stellar Energies NUCLEAR REACTIONS, ICPND 4He(12C, 12C), E=5.6-13.7 MeV; measured σ(E, θ). 16O resonance deduced parameters. 4He(12C, γ), E(cm)=1.44-3.38 MeV; measured capture σ, σ(E, E(γ)), Eγ, Iγ; deduced astrophysical S-factor, reaction mechanism. 16O resonances deduced Γγ, α-reduced widths.
doi: 10.1007/BF01415851
1982KR05 Z.Phys. A304, 307 (1982) H.Krawinkel, H.W.Becker, L.Buchmann, J.Gorres, K.U.Kettner, W.E.Kieser, R.Santo, P.Schmalbrock, H.P.Trautvetter, A.Vlieks, C.Rolfs, J.W.Hammer, R.E.Azuma, W.S.Rodney The 3He(α, γ)7Be Reaction and the Solar Neutrino Problem NUCLEAR REACTIONS 3He(α, γ), E(cm)=107-1266 keV; measured σ(E, Eγ, θγ), σ(absolute). 3He(α, α), E=0.2-3 MeV; measured yield vs E; deduced astrophysical S-factor vs E. Ge(Li) detectors, extended, quasipoint jet gas targets. Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA1205. 1980VL02 Helv.Phys.Acta 53, 318 (1980) Precision Measurement of Proton-Proton Scattering above 1.0 MeV NUCLEAR REACTIONS 1H(p, p), E=1.397, 1.855, 2.425, 3.037 MeV; measured σ(E); deduced systematic, statistical uncertainities. Precision measurements.
1978VL02 Nucl.Phys. A309, 506 (1978) A.E.Vlieks, C.W.Cheng, J.D.King Cross Section and Stellar Reaction Rates for the 42Ca(p, γ) Reaction NUCLEAR REACTIONS 42Ca(p, γ), E=0.7-5.5 MeV; measured σ(E); deduced reaction rates for stellar nucleosynthesis.
doi: 10.1016/0375-9474(78)90492-X
1974VL01 Nucl.Phys. A224, 492 (1974) A.E.Vlieks, J.F.Morgan, S.L.Blatt Total Cross Sections for Some (α, n) and (α, p) Reactions in Medium-Weight Nuclei NUCLEAR REACTIONS 45Sc, 46Ti, 50Cr, 51V, 54Fe(α, n), 58Ni(α, p); measured σ(Eα); deduced astrophysical reaction rates n(A) < σ(ν) > . Separated targets.
doi: 10.1016/0375-9474(74)90551-X
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