NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = N.P.Bateman Found 9 matches. 2002CH61 Phys.Rev. C 66, 064316 (2002) J.C.Chow, J.D.King, N.P.T.Bateman, R.N.Boyd, L.Buchmann, J.M.D'Auria, T.Davinson, M.Dombsky, E.Gete, U.Giesen, C.Iliadis, K.P.Jackson, A.C.Morton, J.Powell, A.Shotter β-delayed particle decay of 17Ne into p+α+12C through the isobaric analog state in 17F RADIOACTIVITY 17Ne(β+α), (β+p); measured Ep, Eα pα(12C)-coin following decay of intermediate IAS state; deduced branching ratios. 17F deduced branching ratios for particle decay from IAS.
doi: 10.1103/PhysRevC.66.064316
2002MO19 Nucl.Phys. A706, 15 (2002) A.C.Morton, J.C.Chow, J.D.King, R.N.Boyd, N.P.T.Bateman, L.Buchmann, J.M.D'Auria, T.Davinson, M.Dombsky, W.Galster, E.Gete, U.Giesen, C.Iliadis, K.P.Jackson, J.Powell, G.Roy, A.Shotter Beta-Delayed Particle Decay of 17Ne RADIOACTIVITY 17Ne(β+p), (β+α); measured Ep, Eα, pγ-coin, angular correlations; deduced log ft, Gamow-Teller strength. 17F deduced levels, J, π, particle decay branching ratios.
doi: 10.1016/S0375-9474(02)00862-X
1999YI01 Phys.Rev. C60, 028801 (1999) K.O.Yildiz, N.P.T.Bateman, Y.M.Butt, A.A.Chen, K.B.Swartz, P.D.Parker Thick Target Yields of 26Alg.s. from the 16O(16O, x)26Alg.s. and 16O(14N, x)26Alg.s. Reactions NUCLEAR REACTIONS 16O(16O, X)26Al, E=80-150 MeV; 16O(14N, X)26Al, E=115 MeV; measured thick target yields; deduced production of 26Al in proto-solar nebula. Previous measurements included in analysis. Comparison with model predictions.
doi: 10.1103/PhysRevC.60.028801
1998BA19 Phys.Rev. C57, 2022 (1998) N.P.T.Bateman, D.W.Bardayan, Y.M.Butt, A.A.Chen, K.O.Yildiz, B.M.Young, P.D.Parker Thick Target Yield of 26Al from the 12C(16O, x)26Al(g.s.) Reaction NUCLEAR REACTIONS 12C(16O, X)26Al, E=45, 65, 140 MeV; measured thick target yield; deduced σ. Activation method.
doi: 10.1103/PhysRevC.57.2022
1998UT02 Phys.Rev. C57, 2731 (1998); Erratum Phys.Rev. C58, 1354 (1998) S.Utku, J.G.Ross, N.P.T.Bateman, D.W.Bardayan, A.A.Chen, J.Gorres, A.J.Howard, C.Iliadis, P.D.Parker, M.S.Smith, R.B.Vogelaar, M.Wiescher, K.Yildiz Breakout from the Hot CNO Cycle: The 18F(p, γ) vs 18F(p, α) branching ratio NUCLEAR REACTIONS 19F(3He, t), (3He, tα), (3He, pt), E=29.8 MeV; 16O(6Li, t), (6Li, 3He), E=32 MeV; measured particle spectra, tp-, tα-coin; deduced reaction rates for 18F + p. 19F deduced levels, resonance features. Astrophysical implications.
doi: 10.1103/PhysRevC.57.2731
1997BA51 Nucl.Phys. A621, 60c (1997) N.P.T.Bateman, D.W.Bardayan, Y.M.Butt, A.A.Chen, K.O.Yildiz, B.M.Young, P.D.Parker, A.E.Champagne The Production of 26Al in the Early Solar System by Oxygen Rich Cosmic Rays NUCLEAR REACTIONS 12C(16O, X)26Al, E=45, 65, 140 MeV; measured residual decay associated βγ(t); deduced residual yield, astrophysical consequences.
doi: 10.1016/S0375-9474(97)00213-3
1995HO25 Nucl.Instrum.Methods Phys.Res. B99, 346 (1995) M.A.Hofstee, J.C.Blackmon, A.E.Champagne, N.P.T.Bateman, P.D.Parker, K.Yildiz, B.M.Young, R.B.Vogelaar, M.S.Smith, A.J.Howard Investigating the Astrophysically Important E(x) = 2.646 MeV State in 20Na NUCLEAR REACTIONS 20Ne(3He, t), E=27 MeV; measured triton spectra, tγ-coin. 20Na level deduced Γγ/Γ.
doi: 10.1016/0168-583X(95)00307-X
1995LU01 Phys.Rev. C51, 635 (1995) B.J.Lund, N.P.T.Bateman, S.Utku, D.J.Horen, G.R.Satchler Isospin Character of Transitions to the 2+1 and 3-1 States of 90,92,94,96Zr NUCLEAR REACTIONS 90,92,94,96Zr(α, α), (α, α'), E=35.4 MeV; measured σ(θ); deduced model parameters. 90,92,94,96Zr levels deduced B(λ), deformation length, transition densities, isospin mixing features. Deformed optical, folding model analyses.
doi: 10.1103/PhysRevC.51.635
1995RO22 Phys.Rev. C52, 1681 (1995) J.G.Ross, J.Gorres, C.Iliadis, S.Vouzoukas, M.Wiescher, R.B.Vogelaar, S.Utku, N.P.T.Bateman, P.D.Parker Indirect Study of Low-Energy Resonances in 31P(p, α)28Si and 35Cl(p, α)32S NUCLEAR REACTIONS 31P, 35Cl(3He, d), E=25 MeV; measured particle spectra, γd-, (particle)d-coin; deduced (p, γ), (p, α) reaction rates for 31P, 35Cl. 36Ar deduced levels Γ, J, π, T. 32S deduced levels Γ, J, π, T, resonance strength.
doi: 10.1103/PhysRevC.52.1681
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