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NSR database version of May 3, 2024.

Search: Author = H.Krauss

Found 7 matches.

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1994MO17      Phys.Rev. C50, 1543 (1994)

P.Mohr, V.Kolle, S.Wilmes, U.Atzrott, G.Staudt, J.W.Hammer, H.Krauss, H.Oberhummer

Direct Capture in the 3⁺ Resonance of ²H(α, γ)⁶Li

NUCLEAR REACTIONS, ICPND ²H(α, γ), E=2-2.5 MeV; measured Eγ, Iγ; deduced σ(E), folding potential parameters.

doi: 10.1103/PhysRevC.50.1543
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0540.

1994MO27      Z.Phys. A349, 339 (1994)

P.Mohr, H.Abele, V.Kolle, G.Staudt, H.Oberhummer, H.Krauss

Properties of ⁸Be and ¹²C Deduced from the Folding-Potential Model

NUCLEAR REACTIONS, ICPND ⁴He(α, α), E ≈ 7-35 MeV; analyzed σ(θ); deduced model potential parameters. ⁴He(α, γ), E(cm)=1.5-3.5 MeV; ⁸Be(α, γ), E not given; calculated σ(E), astrophysical S-factor, Γγ. Double-folded potential.

NUCLEAR STRUCTURE ⁸Be, ¹²C; calculated levels, B(λ). α-cluster states, double-folded potential.

doi: 10.1007/BF01288987
Citations: PlumX Metrics

1994OB03      Z.Phys. A349, 241 (1994)

H.Oberhummer, H.Krauss, K.Grun, T.Rauscher, H.Abele, P.Mohr, G.Staudt

Alpha Clustering and the Stellar Nucleosynthesis of Carbon

NUCLEAR REACTIONS ¹²C(γ, α), E=low; calculated triple-α process reaction rate. Direct capture, α-clustering.

doi: 10.1007/BF01288967
Citations: PlumX Metrics

1993KR18      Ann.Phys.(Leipzig) 2, 258 (1993)

H.Krauss, K.Grun, T.Rauscher, H.Oberhummer

The Astrophysical S-Factor of the Reaction ⁷Be(p, γ)⁸B in the Direct Capture Model

NUCLEAR REACTIONS, ICPND ⁷Be(p, γ), E(cm) ≤ 2 MeV; calculated σ(E), astrophysical S-factor vs E. ⁷Li(n, γ), E(cm) ≤ 1 MeV; calculated σ(E). Direct capture model.

doi: 10.1002/andp.19935050304
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1993MO11      Phys.Rev. C48, 1420 (1993)

P.Mohr, H.Abele, R.Zwiebel, G.Staudt, H.Krauss, H.Oberhummer, A.Denker, J.W.Hammer, G.Wolf

Alpha Scattering and Capture Reactions in the A = 7 System at Low Energies

NUCLEAR REACTIONS, ICPND ⁴He(³He, ³He), E=1.2-3 MeV; measured σ(θ). ⁴He(³He, ³He), (t, t), E ≤ 10 MeV; analyzed phase shifts data. ³H, ³He(α, γ), E(cm) ≤ 1 MeV; calculated astrophysical S-factor vs E; deduced multipole contributions.

doi: 10.1103/PhysRevC.48.1420
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetD0147.

1992RA04      Phys.Rev. C45, 1996 (1992)

T.Rauscher, K.Grun, H.Krauss, H.Oberhummer, E.Kwasniewicz

Analysis of ⁸Li(α, n)¹¹B Below the Coulomb Barrier in the Potential Model

NUCLEAR REACTIONS, ICPND ⁸Li(α, n), E(cm) ≤ 1 MeV; calculated astrophysical S-factor vs E, reaction rates. DWBA, folding potentials.

doi: 10.1103/PhysRevC.45.1996
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1992WI09      J.Phys.(London) G18, L147 (1992)

S.Winkler, H.Krauss, K.Grun, T.Rauscher, H.Oberhummer, H.Abele, G.Staudt

Calculation of the ³He(³He, 2p)⁴He and ³H(³H, 2n)⁴He Astrophysical S Factor at Low Energies

NUCLEAR REACTIONS, ICPND ³He(³He, 2p), E(cm) ≤ 1 MeV; analyzed astrophysical S-factor vs E. ³H(t, 2n), E ≤ 0.35 MeV; analyzed σ(E), astrophysical S-factor vs E. Potential model.

doi: 10.1088/0954-3899/18/8/004
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