NSR Query Results
Output year order : Descending NSR database version of May 3, 2024. Search: Author = R.Spanhoff Found 6 matches. 1983SP05 Hyperfine Interactions 15/16, 89 (1983) Nuclear Spins and Moments of the 182Re Isomers RADIOACTIVITY 182Re(EC), (β+); measured NMR, oriented nuclei. 182Re deduced isomer J, μ, Nilsson assignments. 182W levels deduced (G2) factors.
doi: 10.1007/BF02159723
1981SP06 Hyperfine Interactions 9, 99 (1981) Nuclear Orientation of 184Ir, 185Ir and 186Ir RADIOACTIVITY 184,185,186Ir; measured NMR, γ(θ, T), oriented nuclei. 185,184,186Ir level deduced μ, configuration. 185Os deduced levels, J, π, ICC. 186Os transitions deduced δ. Recoil implantation in Fe.
doi: 10.1007/BF01020905
1980BI06 Nucl.Phys. A344, 207 (1980) R.Bijker, A.E.L.Dieperink, O.Scholten, R.Spanhoff Description of the Pt and Os Isotopes in the Interacting Boson Model NUCLEAR STRUCTURE 196,194,192,190,188,186Pt, 194,192,190,188,186,184Os; calculated levels, B(E2), quadrupole moments, isomer shifts. Interacting boson model.
doi: 10.1016/0375-9474(80)90673-9
1980DE22 Hyperfine Interactions 7, 465 (1980) J.de Jong, H.Postma, R.Spanhoff The Nuclear Magnetic Moment of 182Ta NUCLEAR MOMENTS 182Ta; measured NMR, oriented nuclei; deduced μ.
doi: 10.1007/BF01021529
1980SP01 Phys.Rev. C21, 361 (1980) R.Spanhoff, M.J.Canty, H.Postma, G.Mennenga Nuclear Orientation Study of 182W in the Decay of 182Re Isomers RADIOACTIVITY 182mRe [from Ta(α, 3n), E=40 MeV]; measured γγ-coin, Iγ(θ), oriented nuclei. 182Re levels deduced μ, Nilsson assignments. 182W levels deduced J, π, δ, two-quasiparticle character.
doi: 10.1103/PhysRevC.21.361
1978SP05 Phys.Rev. C18, 493 (1978) R.Spanhoff, H.Postma, M.J.Canty 186Os Studied in the Decay of 15.8-h 186Ir and by the 186W(α, 4n)186Os Reaction RADIOACTIVITY 186mIr; measured Iγ(θ) oriented nuclei, γγ-coin, I(ce); deduced log ft, ICC. 186Ir deduced μ, Nilsson assignment. 186Os deduced levels, J, π, δ. NUCLEAR REACTIONS 186Os(α, 4n), E=47 MeV; measured Eγ, Iγ, γγ-coin, Iγ(θ), γ(t). 186Os deduced levels, J, π, T1/2.
doi: 10.1103/PhysRevC.18.493
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