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NSR database version of May 8, 2024.

Search: Author = G.Bluge

Found 7 matches.

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1991BL17      Few-Body Systems 11, 137 (1991)

G.Bluge, K.Langanke

Microscopic Study of the Low-Energy ³H(d, n)⁴He Reaction

NUCLEAR REACTIONS, ICPND ³H(d, n), E ≤ 80 keV; calculated astrophysical S-factor vs E. ⁴He(n, n), E ≤ 25 MeV; calculated phase shifts vs E.

1991TY01      Z.Phys. A339, 249 (1991)

S.Typel, G.Bluge, K.Langanke, W.A.Fowler

Microscopic Study of the Low-Energy ³He(³He, 2p)⁴He and ³H(³H, 2n)⁴He Fusion Cross Sections

NUCLEAR REACTIONS, ICPND ³He(³He, 2p), E ≤ 350 keV; ³H(t, 2n), E ≤ 300 keV; calculated fusion σ, astrophysical S-factor vs E. Microscopic multi-channel resonating group method.

doi: 10.1007/BF01284060
Citations: PlumX Metrics

1991TY02      Z.Phys. A339, 335 (1991)

S.Typel, G.Bluge, K.Langanke

The Low-Energy D(α, γ)⁶Li and ⁶Li + ²⁰⁸Pb → D + α + ²⁰⁸Pb Cross Sections

NUCLEAR REACTIONS, ICPND ²⁰⁸Pb(⁶Li, dα), E not given; calculated σ(θ, E(αd)). ²H(α, γ), E(cm) ≤ 2.5 MeV; calculated σ(θ), fusion σ(E). Multi-channel resonating group calculation.

doi: 10.1007/BF01560634
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1990BL02      Phys.Rev. C41, 1191 (1990)

G.Bluge, K.Langanke

Consistent Microscopic Study of the Low-Energy ⁵Li Spectrum

NUCLEAR REACTIONS, ICPND ³He(d, p), E ≈ 0.01-1 MeV; calculated astrophysical S-factor vs E. ³He(d, d), E ≤ 6 MeV; ¹H(α, α), E ≤ 16 MeV; calculated phase shift vs E. ⁵Li deduced levels. Multichannel microscopic cluster model.

doi: 10.1103/PhysRevC.41.1191
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1990BL08      Phys.Lett. 238B, 137 (1990)

G.Bluge, K.Langanke, M.Plagge, K.R.Nyga, H.Paetz gen.Schieck

The Low-nergy ³He(d, p)⁴He and ³H(d, n)⁴He Reactions with Polarized Deuterons

NUCLEAR REACTIONS ³He(polarized d, p), E ≤ 8 MeV; calculated T₂₀(θ). ³H(polarized d, n), E=107 keV; calculated iT₁₁(θ), T₂₀(θ), T₂₁(θ), T₂₂(θ). Data-independent approach.

doi: 10.1016/0370-2693(90)91709-K
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1989BL03      Z.Phys. A333, 219 (1989)

G.Bluge, K.Langanke, H.G.Reusch, C.Rolfs

The ³He(d, p)α Reaction at Astrophysical Energies

NUCLEAR REACTIONS, ICPND ³He(d, p), E ≈ 0.01-1 MeV; calculated astrophysical S-factor vs E. Resonating group model, effective nucleon-nucleon interactions.

1987BL12      Phys.Rev. C36, 21 (1987)

G.Bluge, H.J.Assenbaum, K.Langanke

Potential Model Analysis of Low Energy ²H(d, γ)⁴He Fusion Data

NUCLEAR REACTIONS, ICPND ²H(d, γ), E(cm)=0.010-10 MeV; calculated σ(Eγ, E), capture σ, astrophysical S-factor vs E, phase shifts vs E. ⁴He level deduced D-state admixture nucleus-nucleus potential dependence.

doi: 10.1103/PhysRevC.36.21
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