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NSR database version of May 10, 2024.

Search: Author = C.Funck

Found 7 matches.

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1989FU01      Z.Phys. A332, 109 (1989)

C.Funck, B.Grund, K.Langanke

Improved Study of the ¹⁴O(α, p)¹⁷F Reaction at Stellar Energies

NUCLEAR REACTIONS, ICPND ¹⁴O(α, p), E ≈ 0.5-4.5 MeV; calculated astrophysical S-factor vs E. Generator coordinate method.

1989FU06      Astrophys.J. 344, 46 (1989)

C.Funck, K.Langanke

The ¹⁴C(α, γ)¹⁸O Reaction at Astrophysical Energies

NUCLEAR REACTIONS, ICPND ¹⁴C(α, γ), E=astrophysical region; calculated reaction rate vs temperature.

doi: 10.1086/167775
Citations: PlumX Metrics

1989FU08      Z.Phys. A334, 1 (1989)

C.Funck, B.Grund, K.Langanke

Microscopic Multichannel Calculation of the Molecular Dipole Degree of Freedom in the ¹⁸O Nucleus

NUCLEAR STRUCTURE ¹⁸O; calculated continuum level energy surfaces, B(λ). Microscopic multi-channel calculation, dimolecular α+¹⁴C rotator.

1988FU02      Nucl.Phys. A480, 188 (1988)

C.Funck, K.Langanke

Microscopic Study of the ¹⁴O(α, p)¹⁷F Reaction at Stellar Energies

NUCLEAR REACTIONS, ICPND ¹⁴O(α, p), E ≈ 0.5-4 MeV; calculated reaction rate, reaction σ, astrophysical S-factor vs E. ¹⁸Ne deduced resonances. Generator coordinate method, multi-channels.

doi: 10.1016/0375-9474(88)90392-2
Citations: PlumX Metrics

1987FU02      Nucl.Phys. A464, 90 (1987)

C.Funck, K.Langanke

Study of the ¹³N(p, γ)¹⁴O Reaction at Stellar Energies in a Microscopic Coupled-Channel Approach

NUCLEAR REACTIONS, ICPND ¹³N(p, γ), E=low; calculated astrophysical S-factor vs E, capture σ, Γγ, reaction rate vs temperature. ¹⁴O deduced 1^- resonance Γγ, reaction role. Microscopic coupled channels approach.

doi: 10.1016/0375-9474(87)90424-6
Citations: PlumX Metrics

1987KR03      Phys.Rev. C35, 1631 (1987)

D.Krolle, H.J.Assenbaum, C.Funck, K.Langanke

Possible Experiments to Distinguish between Different Methods of Treating the Pauli Principle in Nuclear Potential Models

NUCLEAR REACTIONS ⁴He(α, αγ), E ≤ 15 MeV; calculated bremsstrahlung σ(E), σ(θ₁, θ₂), phase shifts. Finite Pauli repulsion model.

doi: 10.1103/PhysRevC.35.1631
Citations: PlumX Metrics

1985FU04      Phys.Lett. 152B, 11 (1985)

C.Funck, K.Langanke, A.Weiguny

The E2 Contribution to the ¹²C(α, γ)¹⁶O Reaction at Stellar Energies in a Coupled Channel Approach

NUCLEAR REACTIONS, ICPND ¹²C(α, γ), E ≈ 0.1-3.5 MeV; calculated E2 capture σ, S-factor vs E; deduced astrophysical S(E2).

doi: 10.1016/0370-2693(85)91129-3
Citations: PlumX Metrics