NSR Query Results
Output year order : Descending NSR database version of May 6, 2024. Search: Author = A.A.Wolters Found 12 matches. 1993PO11 Z.Phys. A346, 11 (1993) N.A.F.M.Poppelier, A.A.Wolters, P.W.M.Glaudemans Properties of Exotic Light Nuclei NUCLEAR STRUCTURE 4,5,6,7,8,9,10,11He; calculated levels. 5,7,9,11He, 6,8,10,7,9,11Li, 5,7,9,11,13,15,6,8,10,12,14B, 5,7,9,11,13,15B; 7,9,11,13,15,17C, 7,8,9,10,11,12,13,14,15,16,17,19N, 9,10,11,12,13,14,15,16,17,18,19,20F; calculated μ. 6,7,8,9,10,11Li; calculated levels, rms charge, matter radii. 12,13,14,15,16,17,18,19,20,21,22,23,24C, 15,16,17,18,19,20,21,22,23,24,25,26,27N, 16,17,18,19,20,21,22,23,24,25,26,27,28O, 18,19,20,21,22,23,24,25,26,27,28,29F; calculated binding energies. Shell model.
doi: 10.1007/BF01290776
1992WO01 Phys.Rev. C45, 477 (1992) A.A.Wolters, A.G.M.van Hees, P.W.M.Glaudemans Reply to ' Comment on ' p-Shell Nuclei in a (0+2)(h-bar x Omega) Model Space. I. Method ' and on ' p-Shell Nuclei in a (0+2)(h-bar x Omega) Model Space. II. Results ' '
doi: 10.1103/PhysRevC.45.477
1991PA18 Phys.Lett. 271B, 1 (1991) V.Paar, D.Vorkapic, K.Heyde, A.G.M.van Hees, A.A.Wolters Broken Isospin Symmetry in the Shell Model and Chaotic Behavior NUCLEAR STRUCTURE A=22; calculated nearest neighbor spacing distribution with, without Coulomb interaction, Δ3 statistics; deduced isospin symmetry breaking effect on quantum chaos. Realistic shell model.
doi: 10.1016/0370-2693(91)91267-Y
1990EN02 Nucl.Phys. A510, 209 (1990) P.M.Endt, C.Alderliesten, F.Zijderhand, A.A.Wolters, A.G.M.van Hees Spectroscopic Information on 24Mg and 28Si from Proton Capture NUCLEAR REACTIONS 23Na(p, γ), E=1020, 1318, 1417 keV; measured Eγ, Iγ, σ(E, Eγ). 24Mg deduced levels, γ-branching, J, π, T. 27Al(p, γ), E=655, 760, 767, 992, 1317 keV; measured Eγ, Iγ, σ(E, Eγ). 28Si deduced levels, γ-branching, T1/2, J, π, T. Ge detectors with, without Compton suppression.
doi: 10.1016/0375-9474(90)90237-G
1990KI07 Nucl.Phys. A512, 425 (1990) S.W.Kikstra, C.van der Leun, P.M.Endt, J.G.L.Booten, A.G.M.van Hees, A.A.Wolters The 40Ca Level Scheme Investigated with the 39K(p, γ)40Ca Reaction NUCLEAR REACTIONS, ICPND 39K(p, γ), E=0.3-2.9 MeV; measured σ(E, Eγ), γ yield; deduced Q. 40Ca deduced levels, resonance strengths, γ-branchings, T1/2, J, π, T. Enriched targets, Ge detectors. Shell-model calculations.
doi: 10.1016/0375-9474(90)90080-6
1990WO09 Phys.Rev. C42, 2053 (1990) A.A.Wolters, A.G.M.van Hees, P.W.M.Glaudemans p-Shell Nuclei in a (0 + 2)(h-bar x Omega) Model Space. I. Method NUCLEAR STRUCTURE 8Be; calculated levels. 4He, 12,14C, 16O, 14N, 8Be; calculated Coulomb energies, radial excitation strengths. Empirical effective interaction, complete (0+2) (h-bar x omega) space.
doi: 10.1103/PhysRevC.42.2053
1990WO10 Phys.Rev. C42, 2062 (1990) A.A.Wolters, A.G.M.van Hees, P.W.M.Glaudemans p-Shell Nuclei in a (0 + 2)(h-bar x Omega) Model Space. II. Results NUCLEAR STRUCTURE 6,4,5,7,8He; 7,8,9Li, 9,10,11,12Be, 10,11,12,13B, 15,12,13,14C, 14,15,16N, 16O; calculated levels. Effective interactions, (0+2)(h-bar x omega) space. NUCLEAR REACTIONS 4He, 7Li, 13C(e, e'), E not given; calculated form factors. Effective interactions, (0+2)(h-bar x omega) space.
doi: 10.1103/PhysRevC.42.2062
1989TA26 Nucl.Phys. A504, 167 (1989) M.Takahara, M.Hino, T.Oda, K.Muto, A.A.Wolters, P.W.M.Glaudemans, K.Sato Microscopic Calculation of the Rates of Electron Captures which Induce the Collapse of O + Ne + Mg Cores NUCLEAR STRUCTURE 20Ne, 20F, 24Mg, 24Na; calculated Gamow-Teller transition log ft, electron capture rates; deduced O+Ne+Mg core evolution consequences. Shell model.
doi: 10.1016/0375-9474(89)90288-1
1988KR02 Nucl.Phys. A477, 55 (1988) G.J.Kramer, H.P.Blok, J.F.A.van Hienen, S.Brandenburg, M.N.Harakeh, S.Y.van der Werf, P.W.M.Glaudemans, A.A.Wolters Spectroscopic Factors from the 51V(d, 3He)50Ti Reaction NUCLEAR REACTIONS, MECPD 51V(d, 3He), E=52.9 MeV; measured σ(E(3He), θ). 50Ti deduced levels, L, spectroscopic factors.
doi: 10.1016/0375-9474(88)90360-0
1988VA03 Nucl.Phys. A476, 61 (1988) A.G.M.van Hees, A.A.Wolters, P.W.M.Glaudemans Static Moments and Phenomenological Interactions NUCLEAR STRUCTURE 9,6,7,8Li, 8,10,11,12,13B, 9Be, 11,13,14,15C, 12,13,14,15,16N, 15,16O; calculated μ. Phenomenological interactions.
doi: 10.1016/0375-9474(88)90373-9
1988WO04 Europhys.Lett. 5, 7 (1988) A.A.Wolters, A.G.M.van Hees, P.W.M.Glaudemans An Expansion of the Shell-Model Space for Light Nuclei NUCLEAR STRUCTURE 4He, 6,7Li, 10,11B, 9Be, 12,13,14C, 14,15N, 16O; calculated ground state wave functions, rms charge radii, quadrupole moments. Shell model, phenomenological interaction.
doi: 10.1209/0295-5075/5/1/002
1987VA26 Phys.Lett. 196B, 19 (1987) A.G.M.van Hees, A.A.Wolters, P.W.M.Glaudemans An Effective Interaction Derived from Spectra and Static Moments NUCLEAR STRUCTURE 8Li, 11Be, 8,12,14B, 14,15C, 12,16N; calculated magnetic dipole moments. Phenomenological interaction.
doi: 10.1016/0370-2693(87)91668-6
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