NSR Query Results
Output year order : Descending NSR database version of April 25, 2024. Search: Author = J.W.Hammer Found 51 matches. 2013HA03 Phys.Rev. C 87, 025806 (2013) S.Harissopulos, A.Spyrou, A.Lagoyannis, M.Axiotis, P.Demetriou, J.W.Hammer, R.Kunz, H.-W.Becker Cross section measurements of proton capture reactions relevant to the p process: The case of 89Y(p, γ)90Zr and 121, 123Sb(p, γ)122, 124Te NUCLEAR REACTIONS 89Y, 121,123Sb(p, γ)90Zr/122Te/124Te, E=16-3.4 MeV; measured Eγ, Iγ, γ(θ), total σ(E), primary and secondary γ; deduced astrophysical S(E) factors, reaction rates, isomeric cross section ratios. 90Zr; deduced levels, J, π. 89Y(p, γ)90Zr, E=2, 3, 4, 4.8 MeV; measured Eγ, integrated σ(E) by 4π-summing method. Comparison with TALYS code calculations, and with previous studies.
doi: 10.1103/PhysRevC.87.025806
2010CO12 Phys.Rev. C 82, 035802 (2010) H.Costantini, R.J.de Boer, R.E.Azuma, M.Couder, J.Gorres, J.W.Hammer, P.J.LeBlanc, H.Y.Lee, S.O'Brien, A.Palumbo, E.C.Simpson, E.Stech, W.Tan, E.Uberseder, M.Wiescher 16O(α, γ)20Ne S factor: Measurements and R-matrix analysis NUCLEAR REACTIONS 16O(α, γ), E=2.5 MeV; measured Eγ, Iγ, γγ-coin, Eα, Iα. 20Ne; deduced levels, J, π, resonances, width, yields, branching ratios, S factors, reaction rates. R-matrix analysis.
doi: 10.1103/PhysRevC.82.035802
2006AS02 Phys.Rev. C 73, 055801 (2006) M.Assuncao, M.Fey, A.Lefebvre-Schuhl, J.Kiener, V.Tatischeff, J.W.Hammer, C.Beck, C.Boukari-Pelissie, A.Coc, J.J.Correia, S.Courtin, F.Fleurot, E.Galanopoulos, C.Grama, F.Haas, F.Hammache, F.Hannachi, S.Harissopulos, A.Korichi, R.Kunz, D.LeDu, A.Lopez-Martens, D.Malcherek, R.Meunier, Th.Paradellis, M.Rousseau, N.Rowley, G.Staudt, S.Szilner, J.P.Thibaud, J.L.Weil E1 and E2 S factors of 12C(α, γ0)160 from γ-ray angular distributions with a 4π-detector array NUCLEAR REACTIONS 12C(α, γ), E(cm)=1.30-2.78 MeV; measured Eγ, Iγ(θ); deduced E1 and E2 astrophysical S-factors.
doi: 10.1103/PhysRevC.73.055801
2005HA16 Nucl.Phys. A752, 514c (2005) J.W.Hammer, M.Fey, R.Kunz, J.Kiener, V.Tatischeff, F.Haas, J.L.Weil, M.Assuncao, C.Beck, C.Boukari-Pelissie, A.Coc, J.J.Correia, S.Courtin, F.Fleurot, E.Galanopoulos, C.Grama, F.Hammache, S.Harissopulos, A.Korichi, E.Krmpotic, D.Le Du, A.Lopez-Martens, D.Malcherek, R.Meunier, P.Papka, T.Paradellis, M.Rousseau, N.Rowley, G.Staudt, S.Szilner New determination of the 12C(α, γ)16O reaction rate from γ-ray angular distribution measurements NUCLEAR REACTIONS 12C(α, γ), E(cm)=0.89-2.8 MeV; measured σ(θ), S-factors; deduced astrophysical reaction rate.
doi: 10.1016/j.nuclphysa.2005.02.056
2005HA48 Nucl.Phys. A758, 363c (2005) J.W.Hammer, M.Fey, R.Kunz, J.Kiener, V.Tatischeff, F.Haas, J.L.Weil, M.Assuncao, C.Beck, C.Boukari-Pelissie, A.Coc, J.J.Correia, S.Courtin, F.Fleurot, E.Galanopoulos, C.Grama, F.Hammache, S.Harissopulos, A.Korichi, E.Krmpotic, D.Le Du, A.Lopez-Martens, D.Malcherek, R.Meunier, P.Papka, T.Paradellis, M.Rousseau, N.Rowley, G.Staudt, S.Szilner E1 and E2 capture cross section and astrophysical reaction rate of the key reaction 12C(α, γ)16O NUCLEAR REACTIONS 12C(α, γ), E(cm)=0.89-2.8 MeV; measured Eγ, Iγ, angular distributions; deduced S-factors for E1 and E2 capture. Eurogam and Gandi arrays, astrophysical implications discussed.
doi: 10.1016/j.nuclphysa.2005.05.066
2005HA49 Nucl.Phys. A758, 505c (2005) S.Harissopulos, A.Spyrou, A.Lagoyannis, Ch.Zarkadas, H.-W.Becker, C.Rolfs, F.Strieder, J.W.Hammer, A.Dewald, K.-O.Zell, P.von Brentano, R.Julin, P.Demetriou, S.Goriely Systematic measurements of proton- and alpha-capture cross sections relevant to the modelling of the p process NUCLEAR REACTIONS 92Mo(α, γ), E=9 MeV; 91Zr(α, γ), E=10.5 MeV; 118Sn(α, γ), E=11.5 MeV; measured Eγ, Iγ. 91Zr, 118Sn(α, γ), E(cm) ≈ 9-11 MeV; measured σ. Comparison with model predictions.
doi: 10.1016/j.nuclphysa.2005.05.092
2005HA56 J.Phys.(London) G31, S1417 (2005) S.Harissopulos, A.Lagoyannis, A.Spyrou, Ch.Zarkadas, S.Galanopoulos, G.Perdikakis, H.-W.Becker, C.Rolfs, F.Strieder, R.Kunz, M.Fey, J.W.Hammer, A.Dewald, K.-O.Zell, P.von Brentano, R.Julin, P.Demetriou Proton and alpha-particle capture reactions at sub-Coulomb energies relevant to the p process NUCLEAR REACTIONS 104Pd(p, γ), E(cm)=2-8 MeV; 118Sn(α, γ), E(cm)=10-11 MeV; measured Eγ, Iγ, σ. Comparison with model predictions.
doi: 10.1088/0954-3899/31/10/006
2005HA69 Phys.Rev. C 72, 062801 (2005) S.Harissopulos, H.W.Becker, J.W.Hammer, A.Lagoyannis, C.Rolfs, F.Strieder Cross section of the 13C(α, n)16O reaction: A background for the measurement of geo-neutrinos NUCLEAR REACTIONS 13C(α, n), E=0.8-8.0 MeV; measured σ, neutron yields.
doi: 10.1103/PhysRevC.72.062801
2003FE04 Nucl.Phys. A718, 131c (2003) M.Fey, R.Kunz, J.W.Hammer, M.Jaeger, A.Mayer, E.Krmpotic, C.Bauer, C.Meyer, S.Harissopulos, T.Paradellis, G.Staudt, F.Haas, P.Papka, K.-L.Kratz, B.Pfeiffer The Key Reactions in Stellar Helium Burning: 12C(α, γ)16O and 22Ne(α, n)25Mg NUCLEAR REACTIONS 12C(α, γ), E ≈ 1-2.8 MeV; measured Eγ, Iγ(θ); deduced S-factor components. 22Ne(α, n), E=0.57-1.47 MeV; measured excitation function.
doi: 10.1016/S0375-9474(03)00690-0
2003GA01 Phys.Rev. C 67, 015801 (2003) S.Galanopoulos, P.Demetriou, M.Kokkoris, S.Harissopulos, R.Kunz, M.Fey, J.W.Hammer, Gy.Gyurky, Zs.Fulop, E.Somorjai, S.Goriely The 88Sr(p, γ)89Y reaction at astrophysically relevant energies NUCLEAR REACTIONS 88Sr(p, γ), E=1.4-5 MeV; measured Eγ, Iγ, angular distributions, total σ; deduced astrophysical S-factors, reaction rates. Comparison with model predictions.
doi: 10.1103/PhysRevC.67.015801
2003HA32 Nucl.Phys. A719, 115c (2003) S.Harissopulos, S.Galanopoulos, P.Demetriou, A.Spyrou, G.Kriembardis, M.Kokkoris, A.G.Karydas, Ch.Zarkadas, R.Kunz, M.Fey, J.W.Hammer, G.Gyurky, Zs.Fulop, E.Somorjai, A.Dewald, K.O.Zell, P.von Brentano, R.Julin, S.Goriely A systematic study of proton capture reactions in the Se-Sb region at energies relevant to the p process NUCLEAR REACTIONS 80Se, 86Sr, 93Nb, 103Rh(p, γ), E(cm) ≈ 1.5-4.5 MeV; measured Eγ, σ; deduced astrophysical S-factors.
doi: 10.1016/S0375-9474(03)00978-3
2002KU16 Astrophys.J. 567, 643 (2002) R.Kunz, M.Fey, M.Jaeger, A.Mayer, J.W.Hammer, G.Staudt, S.Harissopulos, T.Paradellis Astrophysical Reaction Rate of 12C(α, γ)16O NUCLEAR REACTIONS 12C(α, γ), E(cm) < 10 MeV; calculated S-factors, astrophysical reaction rates.
doi: 10.1086/338384
2002WI18 Phys.Rev. C 66, 065802 (2002) S.Wilmes, V.Wilmes, G.Staudt, P.Mohr, J.W.Hammer The 15N(α, γ)19F reaction and nucleosynthesis of 19F NUCLEAR REACTIONS 15N(α, γ), E=461-2642 keV; measured Eγ, Iγ; deduced resonance energies, strengths, widths, and branching ratios, astrophysical reaction rates. 19F deduced levels.
doi: 10.1103/PhysRevC.66.065802
2001HA31 Prog.Part.Nucl.Phys. 46, 43 (2001) Key Reactions in the Helium Burning Phase of Stars NUCLEAR REACTIONS 12C(α, γ), E(cm)=0.95-2.78 MeV; measured σ(θ); deduced S-factors. 22Ne(α, n), E=570-1400 keV; measured σ; deduced resonance parameters.
doi: 10.1016/S0146-6410(01)00106-5
2001HA38 Nucl.Phys. A688, 421c (2001) S.Harissopulos, S.Galanopoulos, P.Tsagari, P.Demetriou, G.Kuburas, T.Paradellis, R.Kunz, J.W.Hammer, G.Gyurky, E.Somorjai, S.Goriely, S.Kasemann, A.Dewald, K.O.Zell Cross Sections of (p, γ) Reactions of N = 50 Nuclei Relevant to p-Process NUCLEAR REACTIONS 88Sr, 89Y(p, γ), E=1.5-3.5 MeV; measured Eγ, σ. Comparison with Statistical Model calculations and with neighboring nuclei.
doi: 10.1016/S0375-9474(01)00743-6
2001HA60 Phys.Rev. C64, 055804 (2001) S.Harissopulos, E.Skreti, P.Tsagari, G.Souliotis, P.Demetriou, T.Paradellis, J.W.Hammer, R.Kunz, C.Angulo, S.Goriely, T.Rauscher Cross Section Measurements of the 93Nb(p, γ)94Mo Reaction at Ep = 1.4-4.9 MeV Relevant to the Nucleosynthetic p Process NUCLEAR REACTIONS 93Nb(p, γ), E=1.4-4.9 MeV; measured Eγ, Iγ, total σ; deduced astrophysical reaction rates. Comparison with model predictions.
doi: 10.1103/PhysRevC.64.055804
2001JA15 Phys.Rev.Lett. 87, 202501 (2001) M.Jaeger, R.Kunz, A.Mayer, J.W.Hammer, G.Staudt, K.L.Kratz, B.Pfeiffer 22Ne(α, n)25Mg: The key neutron source in massive stars NUCLEAR REACTIONS 22Ne(α, n), E=570-1450 keV; measured σ; deduced resonance parameters, astrophysical reaction rates.
doi: 10.1103/PhysRevLett.87.202501
2001KU09 Phys.Rev.Lett. 86, 3244 (2001) R.Kunz, M.Jaeger, A.Mayer, J.W.Hammer, G.Staudt, S.Harissopulos, T.Paradellis 12C(α, γ)16O: The key reaction in stellar nucleosynthesis NUCLEAR REACTIONS 12C(α, γ), E(cm)=0.95-2.8 MeV; measured Eγ, Iγ(θ); deduced astrophysical S-factors.
doi: 10.1103/PhysRevLett.86.3244
2000JA08 Trans.Bulg.Nucl.Soc. 5, 183 (2000) M.Jaeger, R.Kunz, I.Busching, A.Mayer, J.W.Hammer The Reaction 22Ne(α, n)25Mg as a Neutron Source for the Astrophysical s-Process NUCLEAR REACTIONS 22Ne(α, n), E=0.59-1.5 MeV; measured σ, resonance features.
2000TS05 Trans.Bulg.Nucl.Soc. 5, 195 (2000) P.Tsagari, E.Skreti, G.A.Souliotis, P.Demetriou, S.Harissopulos, T.Paradellis, J.W.Hammer, R.Kunz, C.Angulo, S.Goriely, T.Rauscher Cross Section Measurements of the 89Y(p, γ)90Zr Reaction in the Energy Range Ep = 1.6-2.4 MeV NUCLEAR REACTIONS 89Y(p, γ), E=1.6-2.4 MeV; measured Eγ, Iγ, total σ. 90Zr deduced levels, J, π. Comparison with statistical model.
1999AN35 Nucl.Phys. A656, 3 (1999) C.Angulo, M.Arnould, M.Rayet, P.Descouvemont, D.Baye, C.Leclercq-Willain, A.Coc, S.Barhoumi, P.Aguer, C.Rolfs, R.Kunz, J.W.Hammer, A.Mayer, T.Paradellis, S.Kossionides, C.Chronidou, K.Spyrou, S.Degl'Innocenti, G.Fiorentini, B.Ricci, S.Zavatarelli, C.Providencia, H.Wolters, J.Soares, C.Grama, J.Rahighi, A.Shotter, M.Lamehi-Rachti A Compilation of Charged-Particle Induced Thermonuclear Reaction Rates COMPILATION 1H(p, e+ν), 2H, 6,7Li, 7,9Be, 10,11B, 12,13C, 13,14,15N, 16,17,18O, 19F, 20,21,22Ne, 22,23Na, 24,25,26Mg, 26,27Al, 28Si(p, γ), 2H(d, γ), (d, p), 2,3H(d, n), 2,3H, 3He, 7Li, 7Be, 12C, 14,15N, 16,18O, 20,22Ne(α, γ), 3He(3He, 2p), 6,7Li, 9Be, 10,11B, 14,15N, 17,18O, 19F, 20Ne, 23Na, 24Mg, 27Al(p, α), 7Li, 9Be, 13C, 14N, 17,18O, 21,22Ne, 23Na, 25,26Mg, 27Al(α, n), 9Be, 11B, 13C, 14,15N, 19F, 23Na(p, n), 9Be(p, d), E < 10 MeV; compiled, analyzed σ, S-factors; calculated astrophysical reaction rates vs T9. Analytical approximations.
doi: 10.1016/S0375-9474(99)00030-5
1999KO34 Nucl.Instrum.Methods Phys.Res. A431, 160 (1999) V.Kolle, U.Kolle, S.E.Braitmayer, P.Mohr, S.Wilmes, G.Staudt, J.W.Hammer, M.Jaeger, H.Knee, R.Kunz, A.Mayer Capture Reactions at Astrophysically Relevant Energies: Extended gas target experiments and GEANT simulations NUCLEAR REACTIONS 20Ne(α, γ), E=0.45-3.50 MeV; measured Eγ, Iγ, yield curves; deduced resonant capture features, gas target density effects. GEANT simulations.
doi: 10.1016/S0168-9002(99)00247-8
1998BU13 Phys.Rev. C58, R10 (1998) Y.M.Butt, J.W.Hammer, M.Jaeger, R.Kunz, A.Mayer, P.D.Parker, R.Schreiter, G.Staudt Measurement of the Properties of the Astrophysically Interesting 3/2+ State at 7.101 MeV in 19F NUCLEAR REACTIONS 15N(α, γ), E=2.60-3.93 MeV; measured Eγ, Iγ. 19F deduced resonance E, Γ, ωγ. Astrophysical implications.
doi: 10.1103/PhysRevC.58.R10
1997KU18 Nucl.Phys. A621, 149c (1997) R.Kunz, A.Mayer, K.-D.Joos, H.Knee, A.Muller, J.Nickel, Ch.Plettner, J.W.Hammer, D.Baye, P.Descouvemont, M.Jaeger, V.Kolle, S.Wilmes, G.Staudt, P.Mohr, Ch.Chronidou, S.Harissopulos, K.Spyrou, Th.Paradellis Capture Reactions in the Helium Burning of Stars NUCLEAR REACTIONS, ICPND 12C(α, γ), E(cm)=0.9-3 MeV; measured Iγ(θ), preliminary results; analyzed astrophysical S-factors vs E, reaction rates vs T9. 16O(α, γ), E not given; analyzed Eγ, Iγ. Astrophysical implications.
doi: 10.1016/S0375-9474(97)00228-5
1997MO27 Phys.Rev.Lett. 79, 3837 (1997) R.Morlock, R.Kunz, A.Mayer, M.Jaeger, A.Muller, J.W.Hammer, P.Mohr, H.Oberhummer, G.Staudt, V.Kolle Halo Properties of the First (1/2)+ State in 17F from the 16O(p, γ)17F Reaction NUCLEAR REACTIONS, ICPND 16O(p, p), (p, γ), E(cm)=200-3750 keV; measured Eγ, Iγ, elastic, capture σ(E). 17F deduced halo state properties. Direct capture model.
doi: 10.1103/PhysRevLett.79.3837
1997WI12 Nucl.Phys. A621, 145c (1997) S.Wilmes, V.Kolle, U.Kolle, G.Staudt, P.Mohr, J.W.Hammer, A.Mayer The Capture Reactions 15N(α, γ)19F and 20Ne(α, γ)24Mg at Astrophysically Relevant Energies NUCLEAR REACTIONS 15N(α, γ), E=0.65-2.65 MeV; measured Eγ, Iγ; deduced resonance strengths. 20Ne(α, γ), E=1.64-2.65 MeV; measured Eγ, Iγ; deduced primary transitions yield vs E.
doi: 10.1016/S0375-9474(97)00227-3
1996KU07 Phys.Rev. C53, 2486 (1996) R.Kunz, S.Barth, A.Denker, H.W.Drotleff, J.W.Hammer, H.Knee, A.Mayer Determination of the 9Be(α, n)12C Reaction Rate NUCLEAR REACTIONS, ICPND 9Be(α, n), E=0.5-3.5 MeV; measured yield, σ(E); deduced astrophysical S-factor vs E, reaction rate. 13C deduced resonances, Γ.
doi: 10.1103/PhysRevC.53.2486
1995WI26 Phys.Rev. C52, R2823 (1995) S.Wilmes, P.Mohr, U.Atzrott, V.Kolle, G.Staudt, A.Mayer, J.W.Hammer Low Energy Resonances in 15N(α, γ)19F and 15O(α, γ)19Ne NUCLEAR REACTIONS 15N(α, γ), E=0.67-0.69 MeV; measured Eγ, Iγ; deduced resonance strength. 19Ne, 19F deduced resonance parameters. Gas target, hyperpure Ge detector. Realistic folding potential model. Other data input.
doi: 10.1103/PhysRevC.52.R2823
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
1993DR08 Astrophys.J. 414, 735 (1993) H.W.Drotleff, A.Denker, H.Knee, M.Soine, G.Wolf, J.W.Hammer, U.Greife, C.Rolfs, H.P.Trautvetter Reaction Rates of the s-Process Neutron Sources 22Ne(α, n)25Mg and 13C(α, n)16O NUCLEAR REACTIONS, ICPND 13C(α, n), E(cm) ≈ 275-1075 keV; 22Ne(α, n), E=0.57-2.3 MeV; measured σ(E); deduced astrophysical S-factor, reaction rates at helium burning temperatures.
doi: 10.1086/173119
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
1991DR01 Z.Phys. A338, 367 (1991) H.W.Drotleff, A.Denker, J.W.Hammer, H.Knee, S.Kuchler, D.Streit, C.Rolfs, H.P.Trautvetter New 22Ne(α, n)25Mg-Resonances at Very Low Energies Relevant for the Astrophysical s-Process NUCLEAR REACTIONS, ICPND 22Ne(α, n), E ≈ 550-2100 keV; measured σ(E); deduced resonance structure relevant to s-process. Windowless gas target system, 4π neutron detector.
doi: 10.1007/BF01288203
1990WE10 Nucl.Instrum.Methods Phys.Res. A292, 359 (1990) W.Weiss, W.Grum, J.W.Hammer, M.Koch, G.Schreder Polarization Measurement of Fast Neutrons from the 9Be(α, n)12C and the 13C(α, n)16O Reaction using a High-Pressure 4He-Polarimeter in a New Design NUCLEAR REACTIONS 9Be(α, n), E=1.9-3.1 MeV; 13C(α, n), E=2.406-3.308 MeV; measured σ(θ), polarization. New design high pressure 4He-polarimeter.
doi: 10.1016/0168-9002(90)90392-J
1989DA07 Phys.Rev. C39, 1768 (1989) G.Dagge, W.Grum, J.W.Hammer, K.-W.Hoffmann, G.Schreder Optical Model Analysis of Polarized Neutron Scattering from Aluminum, Copper, and Chromium NUCLEAR REACTIONS 27Al(polarized n, n), (polarized n, n'), E=7.62 MeV; Cr, Cu(polarized n, n), (polarized n, n'), E=7.75 MeV; measured σ(θ), analyzing power vs θ; deduced optical model parameters, spin orbit parameters. Coupled channels, optical model, weak-coupling model analyses.
doi: 10.1103/PhysRevC.39.1768
1989SC07 Phys.Rev. C39, 1774 (1989) G.Schreder, W.Grum, J.W.Hammer, K.-W.Hoffmann, G.Schleussner Optical Model Analysis of Polarized Neutron Scattering from Yttrium, Lanthanum, and Thulium NUCLEAR REACTIONS 89Y, 139La, 169Tm(polarized n, n), E=7.75 MeV; measured σ(θ), analyzing power vs θ; deduced optical model parameters, spin-orbit parameters.
doi: 10.1103/PhysRevC.39.1774
1989WO09 Z.Phys. A334, 491 (1989) K.Wolke, V.Harms, H.W.Becker, J.W.Hammer, K.L.Kratz, C.Rolfs, U.Schroder, H.P.Trautvetter, M.Wiescher, A.Wohr Helium Buring of 22Ne NUCLEAR REACTIONS, ICPND 22Ne(α, γ), (α, nγ), E=0.71-2.25 MeV; measured σ(Eγ, E), γ yields, σ(En); deduced reaction rates. 26Mg deduced resonances, γ-branching ratios, J, π, transition strengths. Enriched gas target. Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1122. 1988HI06 Z.Phys. A329, 243 (1988) M.Hilgemeier, H.W.Becker, C.Rolfs, H.P.Trautvetter, J.W.Hammer Absolute Cross Section of the 3He(α, γ)7Be Reaction NUCLEAR REACTIONS, ICPND 3He(α, γ), E(cm)=195-686 keV; measured σ(E); deduced astrophysical S(E) factor. Windowless gas targets, beam calorimeter, Ge detectors. Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA1289. 1987RE02 Nucl.Phys. A462, 385 (1987) A.Redder, H.W.Becker, C.Rolfs, H.P.Trautvetter, T.R.Donoghue, T.C.Rinckel, J.W.Hammer, K.Langanke The 12C(α, γ)16O Cross Section at Stellar Energies NUCLEAR REACTIONS, ICPND 12C(α, γ), E=0.94-2.84 MeV; measured Eγ, Iγ, σ(E), σ(E, E(γ), θ); deduced astrophysical S-factor. Implanted 12C targets, NaI(Tl), Ge detectors.
doi: 10.1016/0375-9474(87)90555-0
1986HA25 Nucl.Instrum.Methods Phys.Res. A244, 455 (1986) J.W.Hammer, G.Bulski, W.Grum, W.Kratschmer, H.Postner, G.Schleussner SCORPION, The Stuttgart Scattering Facility for Fast Polarized Neutrons NUCLEAR REACTIONS 12C(n, n), (polarized n, n), E=7.55-8.8 MeV; measured σ(θ), analyzing power vs θ.
doi: 10.1016/0168-9002(86)91069-7
1985RE09 Phys.Rev.Lett. 55, 1262 (1985) A.Redder, H.W.Becker, J.Gorres, M.Hilgemeier, A.Krauss, C.Rolfs, U.Schroder, H.P.Trautvetter, K.Wolke, T.R.Donoghue, T.C.Rinckel, J.W.Hammer Capture Amplitudes in the Reaction 12C(α, γ)16O at Stellar Energies NUCLEAR REACTIONS 12C(α, γ), E(cm)=1.7-2.8 MeV; measured Eγ, Iγ, γ(θ); deduced nonnegligible E2 contribution to reaction rate at stellar energies, capture σ(E1)/σ(E2).
doi: 10.1103/PhysRevLett.55.1262
1983GO21 Nucl.Phys. A408, 372 (1983) J.Gorres, H.W.Becker, L.Buchmann, C.Rolfs, P.Schmalbrock, H.P.Trautvetter, A.Vlieks, J.W.Hammer, T.R.Donoghue Proton-Induced Direct Capture on 21Ne and 22Ne NUCLEAR REACTIONS, ICPND 22Ne(p, p), E=0.6-1.6 MeV; measured σ(θ=145°)/σ(Rutherford) vs E. 21,22Ne(p, γ), E=0.3-1.6 MeV; measured Eγ, Iγ, σ(E, θγ); deduced direct capture σ, astrophysical reaction rates. 22Na resonances deduced γ transition strength. 23Na levels deduced spectroscopic factors, γ transition strength. Extended quasipoint jet gas targets, Ge(Li) detectors.
doi: 10.1016/0375-9474(83)90588-2
1983SC17 Nucl.Phys. A398, 279 (1983) P.Schmalbrock, H.W.Becker, L.Buchmann, J.Gorres, K.U.Kettner, W.E.Kieser, H.Krawinkel, C.Rolfs, H.P.Trautvetter, J.W.Hammer, R.E.Azuma Stellar Reaction Rate of 20Ne(α, γ)24Mg NUCLEAR REACTIONS, ICPND 20Ne(α, γ), E=0.55-3.2 MeV; measured Eγ, Iγ(E, θ); deduced astrophysical reaction rate, S-factor of capture σ. 24Mg deduced levels, absolute γ-transition strengths, Γ, J, π, T, δ, γ-branching ratios. Windowless gas targets of the extended and jet type, enriched 20Ne gas, Ge(Li) detectors.
doi: 10.1016/0375-9474(83)90488-8
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. 1980WI17 Nucl.Phys. A349, 165 (1980) M.Wiescher, H.W.Becker, J.Gorres, K.-U.Kettner, H.P.Trautvetter, W.E.Kieser, C.Rolfs, R.E.Azuma, K.P.Jackson, J.W.Hammer Nuclear and Astrophysical Aspects of 18O(p, γ)19F NUCLEAR REACTIONS 18O(p, γ), E=80-2200 keV; measured Ep, Eγ, Iγ(E, θ). 19F deduced levels, absolute γ-transition strength, Γ, J, π, δ, γ-branching ratios, S, astrophysical reaction rate. Enriched target, Ge(Li) detectors.
doi: 10.1016/0375-9474(80)90451-0
1978TR05 Nucl.Phys. A297, 489 (1978) H.P.Trautvetter, M.Wiescher, K.-U.Kettner, C.Rolfs, J.W.Hammer Helium Burning of 18O NUCLEAR REACTIONS 18O(α, γ), E=0.6-2.3 MeV; measured Eγ, Iγ, Iγ(θ), Iγ(E); deduced astrophysical reaction rate. 22Ne deduced resonances, resonance strength, Γ, J, π, δ, γ-ray branching ratios. Enriched 18O targets. Ge(Li) detector.
doi: 10.1016/0375-9474(78)90156-2
1976HA36 Z.Phys. A278, 183 (1976) Die K-Elektroneneinfangwahrscheinlichkeit P(k) beim Zerfall von 139Ce RADIOACTIVITY 139Ce; measured K-shell EC probability.
doi: 10.1007/BF01437774
1976HA61 Z.Phys. A279, 135 (1976) The K-Fluorescence Yield of Germanium RADIOACTIVITY 74As; measured γγ-coin, T1/2, K X-rays; deduced EC, β-branching. 74Ge deduced K-fluorescence yield P(K)w(K).
doi: 10.1007/BF01437868
1975AL23 Z.Phys. A273, 405 (1975) Die K-Fluoreszenzausbeute von Titan und der Zerfall des 48Vanadium RADIOACTIVITY 48V; measured T1/2, I X-ray, Iγ, γ(X-ray)-coin; deduced branching. 48Ti deduced K-fluorescence yield.
doi: 10.1007/BF01435584
1971GE10 Z.Phys. 246, 376 (1971) V.Gehrling, J.W.Hammer, K.-W.Hoffmann Der Zerfall des 84Rb und die Fluoreszenzausbeute von Krypton RADIOACTIVITY 84Rb; measured T1/2, Eγ, Iγ, Xγ-coin, γγγ-triple coin; deduced branching ratios. Kr deduced K-shell fluorescence yield.
doi: 10.1007/BF02115802
1969GR12 Z.Physik 225, 293 (1969) H.-H.Grotheer, J.W.Hammer, K.-W.Hoffmann Experimentelle Untersuchungen am Elektroneneinfang des 85Strontium und 88Yttrium RADIOACTIVITY 85Sr; measured X(K)γ-coin; deduced K-capture rate. 85Rb level deduced T1/2. 88Y; measured X(K)γ-coin; deduced EC/β+ branching ratio. ATOMIC PHYSICS Rb, Sr; deduced K-fluorescence yield.
doi: 10.1007/BF01395011
1968HA47 Z.Physik 216, 355 (1968) Experimentelle Untersuchungen am Elektroneneinfang des Mangan 54 und Zink 65 RADIOACTIVITY 54Mn, 65Zn; measured T1/2, Eγ, Xγ-coin; deduced electron subshell capture rates, γ/β. Ge(Li) detector.
doi: 10.1007/BF01391530
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