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NSR database version of April 27, 2024.

Search: Author = W.S.Rodney

Found 14 matches.

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1999JU06      Nucl.Phys. B(Proc.Supp.) S70, 382 (1999)

M.Junker, C.Arpesella, E.Bellotti, C.Broggini, P.Corvisiero, A.D'Alessandro, G.Fiorentini, A.Fubini, G.Gervino, U.Greife, C.Gustavino, J.Lambert, P.Prati, W.S.Rodney, C.Rolfs, H.P.Trautvetter, S.Zavatarelli, for the LUNA Collaboration

The cross section of 3He(3He, 2p)4He measured at solar energies

NUCLEAR REACTIONS 3He(3He, 2p)4He, E(cm)=25 keV; measured reaction products, Ep, Ip, Eα, Iα; deduced S-factors, σ. Comparison with available data.

doi: 10.1016/s0920-5632(98)00458-7
Citations: PlumX Metrics

1998JU03      Phys.Rev. C57, 2700 (1998)

M.Junker, A.D'Alessandro, S.Zavatarelli, C.Arpesella, E.Bellotti, C.Broggini, P.Corvisiero, G.Fiorentini, A.Fubini, G.Gervino, U.Greife, C.Gustavino, J.Lambert, P.Prati, W.S.Rodney, C.Rolfs, F.Strieder, H.P.Trautvetter, D.Zahnow, and the Luna Collaboration

Cross Section of 3He(3He, 2p)4He Measured at Solar Energies

NUCLEAR REACTIONS 3He(3He, 2p), E=20.76-91.70 keV; measured σ; deduced astrophysical S factor, electron screening effect, no evidence for low-energy resonance.

doi: 10.1103/PhysRevC.57.2700
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0110.

1997GR11      Nucl.Phys. A621, 603c (1997)

U.Greife, C.Arpesella, E.Bellotti, K.Brand, C.Broggini, L.Campajola, P.Corvisiero, A.D'Onofrio, G.Fiorentini, A.Fubini, G.Gervino, L.Gialanella, C.Gustavino, E.Huttel, M.Junker, R.W.Kavanagh, R.Kubat, J.Lambert, G.Oliviero, P.Prati, H.Rebel, V.Roca, W.S.Rodney, C.Rolfs, M.Romano, M.Romoli, S.Schmidt, W.H.Schulte, F.Strieder, F.Terrasi, H.P.Trautvetter, D.Zahnow, S.Zavatarelli

Further Direct Approaches to the Nuclear Reactions in the Sun

doi: 10.1016/S0375-9474(97)00312-6
Citations: PlumX Metrics

1996AR16      Phys.Lett. 389B, 452 (1996)

C.Arpesella, E.Bellotti, C.Broggini, P.Corvisiero, G.Fiorentini, A.Fubini, G.Gervino, U.Greife, C.Gustavino, M.Junker, J.Lambert, P.Prati, W.S.Rodney, C.Rolfs, H.P.Trautvetter, D.Zahnow, S.Zavatarelli

Measurement of the 3He(3He, 2p)4He Cross Section within the Solar Gamow Peak

NUCLEAR REACTIONS, ICPND 3He(3He, 2p), E=20.7-91.7 keV; measured astrophysical S-factor vs E; deduced no evidence for hypothetical resonance.

doi: 10.1016/S0370-2693(96)01326-3
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0110.

1994GR33      Nucl.Instrum.Methods Phys.Res. A350, 327 (1994)

U.Greife, C.Arpesella, C.A.Barnes, F.Bartolucci, E.Bellotti, C.Broggini, P.Corvisiero, G.Fiorentini, A.Fubini, G.Gervino, F.Gorris, C.Gustavino, M.Junker, R.W.Kavanagh, A.Lanza, G.Mezzorani, P.Prati, P.Quarati, W.S.Rodney, C.Rolfs, W.H.Schulte, H.P.Trautvetter, D.Zahnow

Laboratory for Underground Nuclear Astrophysics (LUNA)

NUCLEAR REACTIONS, ICPND 2H(d, n), (d, p), E=10 keV; 2H(3He, p), E=70 keV; measured spectra. 2H(3He, p), E ≤ 40 keV; 3He(3He, 2p), E ≤ 160 keV; measured astrophysical S-factor vs E. Windowless gas target system, close geometry detector telescopes.

doi: 10.1016/0168-9002(94)91182-7
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.

1987RO25      Rep.Prog.Phys. 50, 233 (1987)

C.Rolfs, H.P.Trautvetter, W.S.Rodney

Current Status of Nuclear Astrophysics

doi: 10.1088/0034-4885/50/3/001
Citations: PlumX Metrics

1983SC10      Z.Phys. A310, 243 (1983)

P.Schmalbrock, H.W.Becker, L.Buchmann, J.Gorres, C.Rolfs, H.P.Trautvetter, W.S.Rodney

Search for γ-Ray Transitions within the 5Li Groundstate

NUCLEAR REACTIONS 4He(p, p'γ), E=1.5-7 MeV; measured σ(Ep'), Eγ, Iγ; deduced no 5Li decay.

doi: 10.1007/BF01415229
Citations: PlumX Metrics

1982KR05      Z.Phys. A304, 307 (1982)

H.Krawinkel, H.W.Becker, L.Buchmann, J.Gorres, K.U.Kettner, W.E.Kieser, R.Santo, P.Schmalbrock, H.P.Trautvetter, A.Vlieks, C.Rolfs, J.W.Hammer, R.E.Azuma, W.S.Rodney

The 3He(α, γ)7Be Reaction and the Solar Neutrino Problem

NUCLEAR REACTIONS 3He(α, γ), E(cm)=107-1266 keV; measured σ(E, Eγ, θγ), σ(absolute). 3He(α, α), E=0.2-3 MeV; measured yield vs E; deduced astrophysical S-factor vs E. Ge(Li) detectors, extended, quasipoint jet gas targets.

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA1205.

1979LO01      Nucl.Phys. A313, 346 (1979)

H.Lorenz-Wirzba, P.Schmalbrock, H.P.Trautvetter, M.Wiescher, C.Rolfs, W.S.Rodney

The 18O(p, α)15N Reaction at Stellar Energies

NUCLEAR REACTIONS 18O(p, α), E=72-935 keV; measured Ep, Eα, Iα, Iα(θ). 19F deduced resonances, resonance strength, Γ, J, π, astrophysical reaction rate. Enriched 18O solid targets. Windowless, recirculating gas target.

doi: 10.1016/0375-9474(79)90505-0
Citations: PlumX Metrics

1975RO05      Nucl.Phys. A240, 221 (1975)

C.Rolfs, W.S.Rodney, S.Durrance, H.Winkler

A New Method for Measurement of Proton Beam Energies

NUCLEAR REACTIONS 16,17O(p, γ), E=0.9-1.9 MeV; measured σ(E); deduced Q-values, Ep. 18F deduced resonances, level-width. Natural, enriched targets.

doi: 10.1016/0375-9474(75)90327-9
Citations: PlumX Metrics

1975RO08      Nucl.Phys. A241, 460 (1975)

C.Rolfs, W.S.Rodney, M.H.Shapiro, H.Winkler

Hydrogen Burning of 20Ne and 22Ne in Stars

NUCLEAR REACTIONS 20,22Ne(p, γ), E=0.37-2.10 MeV; measured σ(E, Eγ, θ); deduced Q. 21,23Na deduced resonances, strengths, branching ratios, L, S, astrophysical S. Natural Ne gas target, Ne implanted target.

doi: 10.1016/0375-9474(75)90398-X
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC0626.

1975RO20      Nucl.Phys. A250, 295 (1975)

C.Rolfs, W.S.Rodney

Hydrogen Burning of 17O in the CNO Cycle

NUCLEAR REACTIONS 17O(p, γ), E=1.36-1.65 MeV; measured σ(E), Eγ, Iγ. 18F levels, deduced spectroscopic, astrophysical S-factors. Enriched targets.

doi: 10.1016/0375-9474(75)90260-2
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC2616.

1974RO37      Nucl.Phys. A235, 450 (1974)

C.Rolfs, W.S.Rodney

Proton Capture by 15N at Stellar Energies

NUCLEAR REACTIONS 15N(p, γ), (p, αγ), E=150-2500 keV; measured σ(E, Eγ, θ). 16O levels deduced spectroscopic, astrophysical S-factors. Enriched target.

doi: 10.1016/0375-9474(74)90205-X
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetC0647.

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