NSR Query Results
Output year order : Descending NSR database version of May 9, 2024. Search: Author = K.W.Scheller Found 5 matches. 1995SC03 Nucl.Phys. A582, 109 (1995) K.W.Scheller, J.Gorres, S.Vouzoukas, M.Wiescher, B.Pfeiffer, K.-L.Kratz, D.J.Morrissey, B.M.Sherrill, M.Steiner, M.Hellstrom, J.A.Winger Study of the β-Delayed Neutron Decay of 17C and 18C RADIOACTIVITY 17,18C(β-n) [from 9Be(22Ne, X), E=69 MeV/nucleon]; measured β-decay curves, neutron spectra; deduced T1/2, log ft. 17,18N levels deduced branching ratios.
doi: 10.1016/0375-9474(94)00465-Y
1994GO16 Phys.Rev. C50, R1270 (1994) J.Gorres, J.Meissner, J.G.Ross, K.W.Scheller, S.Vouzoukas, M.Wiescher, J.D.Hinnefeld Lifetimes of Levels in 20F NUCLEAR REACTIONS 19F(d, p), E=2 MeV; measured pγ-coin, Eγ, DSA. 20F levels deduced T1/2.
doi: 10.1103/PhysRevC.50.R1270
1994IL01 Nucl.Phys. A571, 132 (1994) C.Iliadis, J.Gorres, J.G.Ross, K.W.Scheller, M.Wiescher, R.E.Azuma, G.Roters, H.P.Trautvetter, H.C.Evans Explosive Hydrogen Burning of 35Cl NUCLEAR REACTIONS 35Cl(3He, d), E=15 MeV; measured σ(θ), σ(Ed). 32S(6Li, d), E=32 MeV; measured σ(Ed). 32S(α, γ), E ≈ resonance; measured Eγ, Iγ. 35Cl(p, γ), E ≈ 200-800 keV; measured γ yield vs E , stellar rates. 35Cl(p, X), E=177 keV; measured particle spectra. 36Ar deduced levels, J, π, L, spectroscopic factors, γ-branching ratios, resonance strengths. Deduced no evidence for (p, α) reactions.
doi: 10.1016/0375-9474(94)90345-X
1994SC01 Phys.Rev. C49, 46 (1994) K.W.Scheller, J.Gorres, J.G.Ross, M.Wiescher, R.Harkewicz, D.J.Morrissey, B.M.Sherrill, M.Steiner, N.A.Orr, J.A.Winger Study of the β-Delayed Neutron Decay of 18N RADIOACTIVITY 18N(β-) [from 9Be(22Ne, X), E=75 MeV/nucleon]; measured β-delayed neutron spectra, T1/2; deduced log ft. 18O deduced levels, J, π, total branching ratio.
doi: 10.1103/PhysRevC.49.46
1993IL01 Nucl.Phys. A559, 83 (1993) C.Iliadis, J.Gorres, J.G.Ross, K.W.Scheller, M.Wiescher, C.Grama, Th.Schange, H.P.Trautvetter, H.C.Evans Explosive Hydrogen Burning of 31P NUCLEAR REACTIONS, ICPND 31P(p, γ), (p, α), E=160-370 keV; 28Si(α, γ), E=2.4-2.6 MeV; measured γ yield vs E; deduced stellar reaction rates, temperature dependence. 32S deduced proton thershold state features.
doi: 10.1016/0375-9474(93)90181-V
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