NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = J.Humblet Found 10 matches. 2001HU14 Nucl.Phys. A688, 552c (2001) 12C(α, α)12C and 12C(α, γ)16O S-Factor NUCLEAR REACTIONS 12C(α, α), (α, γ), E=low; calculated S-factors for the radiative capture reaction following R-matrix fits to the elastic scattering data.
doi: 10.1016/S0375-9474(01)00785-0
1998HU18 Nucl.Phys. A638, 714 (1998) J.Humblet, A.Csoto, K.Langanke R-Matrix and K-Matrix Analysis of Elastic α-α Scattering NUCLEAR REACTIONS 4He(α, α), E(cm) < 40 MeV; analyzed phase shifts; deduced R-matrix, K-matrix parameters.
doi: 10.1016/S0375-9474(98)00419-9
1997BU12 Nucl.Phys. A621, 153c (1997) L.Buchmann, R.E.Azuma, C.A.Barnes, J.Humblet, K.Langanke Present Experimental Constraints on the Total S-Factor of 12C(α, γ)16O and Proposals for Future Experiments NUCLEAR REACTIONS, ICPND 12C(α, γ), E not given; analyzed data; deduced astrophysical S-factor limits for E1, E2 transitions, implications for future experiments.
doi: 10.1016/S0375-9474(97)00229-7
1996BU10 Phys.Rev. C54, 393 (1996) L.Buchmann, R.E.Azuma, C.A.Barnes, J.Humblet, K.Langanke Analysis of the Total 12C(α, γ)16O Cross Section Based on Available Angular Distributions and Other Primary Data NUCLEAR REACTIONS, ICPND 12C(α, γ), E=stellar; analyzed σ(E); deduced different multipoles associated astrophysical S-factor vs E. R-, K-matrix approaches.
doi: 10.1103/PhysRevC.54.393
1993HU07 Phys.Rev. C48, 2114 (1993) J.Humblet, B.W.Filippone, S.E.Koonin α Spectrum from 16N β Decay and the 12C(α, γ)16O Reaction NUCLEAR REACTIONS, ICPND 12C(α, γ), E(cm) ≤ 4.5 MeV; calculated astrophysical S-factor vs E. Input of 16N β-decay data. RADIOACTIVITY 16N(β-); analyzed Eα, Iα; deduced astrophysical S-factor vs E(cm) for 12C(α, γ) reaction.
doi: 10.1103/PhysRevC.48.2114
1991HU10 Phys.Rev. C44, 2530 (1991) J.Humblet, B.W.Filippone, S.E.Koonin Level Matrix, 16N β Decay, and the 12C(α, γ)16O Reaction RADIOACTIVITY 16N(β-); calculated α-spectra following β-decay; deduced 12C(α, γ)16O reaction astrophysical S-factor relevance. K-matrix approach.
doi: 10.1103/PhysRevC.44.2530
1990JI02 Phys.Rev. C41, 1736 (1990) X.Ji, B.W.Filippone, J.Humblet, S.E.Koonin Constraints on the 12C(α, γ)16O Astrophysical S Factor from the Beta-Delayed α Emission of 16N NUCLEAR REACTIONS, ICPND 12C(α, γ), E(cm)=1-4 MeV; calculated astrophysical S-factor vs E.
doi: 10.1103/PhysRevC.41.1736
1989FI08 Phys.Rev. C40, 515 (1989) B.W.Filippone, J.Humblet, K.Langanke K-Matrix Analysis of the 12C(α, γ) Reaction at Low Energy NUCLEAR REACTIONS, ICPND 12C(α, γ), E(cm)=0.3-3 MeV; calculated astrophysical S-factor vs E. K-matrix analysis.
doi: 10.1103/PhysRevC.40.515
1976HU10 Nucl.Phys. A271, 210 (1976) J.Humblet, P.Dyer, B.A.Zimmerman The K-Matrix Parametrization of the 12C(α, γ)16O Cross Section NUCLEAR REACTIONS 12C(α, γ); analyzed E1 σ. 12C(α, α); analyzed phase shift. Modified K-matrix calculations.
doi: 10.1016/0375-9474(76)90276-1
1972HU05 Nucl.Phys. A187, 65 (1972) Elastic Scattering and the K Matrix
doi: 10.1016/0375-9474(72)90076-0
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