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NSR database version of April 24, 2024.

Search: Author = G.Roters

Found 6 matches.

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1999RO24      Eur.Phys.J. A 6, 451 (1999)

G.Roters, C.Rolfs, F.Strieder, H.P.Trautvetter

The E1 and E2 Capture Amplitudes in 12C(α, γ0)16O

NUCLEAR REACTIONS 4He(12C, γ), E=0.94-3.4 MeV; measured Eγ, Iγ, excitation function; deduced E1, E2 contributions.

doi: 10.1007/s100500050369
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0652.


1997TR07      Nucl.Phys. A621, 161c (1997)

H.P.Trautvetter, G.Roters, C.Rolfs, S.Schmidt, P.Descouvemont

The E2-Contribution to the 12C(α, γ)16O-Reaction

NUCLEAR REACTIONS, ICPND 4He(12C, γ), E=0.9-3.4 MeV; measured Eγ, Iγ; deduced astrophysical S-factors vs E for E1, E2 transitions. Other data considered.

doi: 10.1016/S0375-9474(97)00230-3
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0652.


1995BE29      Z.Phys. A351, 453 (1995)

H.W.Becker, M.Bahr, M.Berheide, L.Borucki, M.Buschmann, C.Rolfs, G.Roters, S.Schmidt, W.H.Schulte, G.E.Mitchell, J.S.Schweitzer

Hydrogen Depth Profiling using 18O Ions

NUCLEAR REACTIONS, ICPND 1H(15N, α), E=6.58 MeV; 1H(18O, α), E=2.9 MeV; measured spectra. 18O(p, α), E ≈ 140-160 keV; calculated astrophysical S-factor vs E. 1H(15N, α), E ≈ 6.525-6.625 MeV; 1H(18O, α), E ≈ 2.85-2.95 MeV; measured yield ratio Iα/I(H) vs E. 16O, 19F deduced more accurate resonance parameters. 1H(18O, α), E ≈ 2.68-2.78 MeV; measured α-yield vs E. 1H(15N, α), E ≈ 6.36-6.48 MeV; measured γ yield vs E. Single stage accelerator technique, depth profiling applications.

doi: 10.1007/BF01291151
Citations: PlumX Metrics


1994IL01      Nucl.Phys. A571, 132 (1994)

C.Iliadis, J.Gorres, J.G.Ross, K.W.Scheller, M.Wiescher, R.E.Azuma, G.Roters, H.P.Trautvetter, H.C.Evans

Explosive Hydrogen Burning of 35Cl

NUCLEAR REACTIONS 35Cl(3He, d), E=15 MeV; measured σ(θ), σ(Ed). 32S(6Li, d), E=32 MeV; measured σ(Ed). 32S(α, γ), E ≈ resonance; measured Eγ, Iγ. 35Cl(p, γ), E ≈ 200-800 keV; measured γ yield vs E , stellar rates. 35Cl(p, X), E=177 keV; measured particle spectra. 36Ar deduced levels, J, π, L, spectroscopic factors, γ-branching ratios, resonance strengths. Deduced no evidence for (p, α) reactions.

doi: 10.1016/0375-9474(94)90345-X
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC0908.


1992BE45      Nucl.Instrum.Methods Phys.Res. A321, 521 (1992)

M.Benjelloun, Th.Delbar, W.Galster, P.Leleux, E.Lienard, P.Lipnik, P.Duhamel, J.Vanhorenbeeck, C.Rolfs, G.Roters, H.P.Trautvetter, W.Rodney

Precise Measurement of the J(π) = 1- Resonance in 14N by 13C + p Elastic Scattering on a Thick Target

NUCLEAR REACTIONS 1H(13C, 13C), E=6.8-9.6 MeV; measured proton spectra. 14N deduced resonance energy, Γ. Proton, projectile energy loss, straggling considered correctly, thick CH2 target.

doi: 10.1016/0168-9002(92)90062-9
Citations: PlumX Metrics


1991GA22      Phys.Rev. C44, 2776 (1991)

W.Galster, P.Leleux, I.Licot, E.Lienard, P.Lipnik, D.Mertens, T.Delbar, J.Vervier, P.Decrock, M.Huyse, P.Van Duppen, P.Duhamel, J.Vanhorenbeeck, G.Roters, C.Rolfs, U.Schroeder, H.P.Trautvetter, K.Wolke, J.Lambert, W.S.Rodney

Target and Detection Techniques for the 13N(p, γ)14O Reaction Using Radioactive Ion Beams: 13C(p, γ)14N reaction as a test case

NUCLEAR REACTIONS, ICPND 1H(13C, 13C), (13C, γ), E(cm)=0.46-0.6 MeV; measured σ(E), thick target γ yield. 13C(p, γ), E=0.45-0.65 MeV; measured σ(E), thin targets. 14N deduced resonance, Γ, Γγ. Breit-Wigner analysis. Techniques for radioactive beams, gas, foil targets.

doi: 10.1103/PhysRevC.44.2776
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetF0562.


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