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NSR database version of May 10, 2024.

Search: Author = O.S.Van Roosmalen

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1987VA03      Phys.Rev. C35, 977 (1987)

O.S.van Roosmalen

Model-Independent Analysis of Heavy-Ion Elastic Scattering

NUCLEAR REACTIONS ²⁸Si(¹⁶O, ¹⁶O), E(cm)=21.1 MeV; calculated phase shifts.

doi: 10.1103/PhysRevC.35.977
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1985LA06      Nucl.Phys. A435, 657 (1985); Erratum Nucl.Phys. A446, 750 (1985)

K.Langanke, O.S.Van Roosmalen, W.A.Fowler

The ¹³N(p, γ)¹⁴O Reaction at Stellar Energies

NUCLEAR REACTIONS, ICPND ¹²C(p, γ), E ≈ 0.1-0.6 MeV; calculated σ(E). ¹³N(p, γ), E(cm) ≈ 0.0-2 MeV; calculated astrophysical factor S(E); deduced resonance effect. ¹⁴O deduced resonance Γp, Γγ. Microscopic potential model.

doi: 10.1016/0375-9474(85)90482-8
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1985LA14      Phys.Rev. C32, 163 (1985)

K.Langanke, O.S.van Roosmalen

Anomalous Projectile Fragments as Nuclear Molecules

NUCLEAR STRUCTURE ²⁴Mg, ³²S; calculated molecular state γ-decay T_1/2, B(E2); deduced no nuclear molecules, anomalous projectile fragments identity. Microscopic cluster model, ¹²C+¹²C, ¹⁶O+¹⁶O systems.

doi: 10.1103/PhysRevC.32.163
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1984LA08      Phys.Rev. C29, 1358 (1984)

K.Langanke, O.S.van Roosmalen

Intraband γ Transitions between ¹²C + ¹²C Molecular States

NUCLEAR REACTIONS ¹²C(¹²C, ¹²C), (¹²C, ¹²C'), E(cm) ≈ 25.5 MeV; analyzed γ-, particle-decay data. ²⁴Mg deduced molecular resonances, intraband transition quadrupole moment, B(E2), Γγ. Microscopic potential model.

doi: 10.1103/PhysRevC.29.1358
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