NSR Query Results
Output year order : Descending NSR database version of April 25, 2024. Search: Author = H.P.Trautvetter Found 124 matches. Showing 1 to 100. [Next]2016WA11 Phys.Rev. C 93, 045803 (2016) A.Wallner, M.Bichler, K.Buczak, I.Dillmann, F.Kappeler, A.Karakas, C.Lederer, M.Lugaro, K.Mair, A.Mengoni, G.Schatzel, P.Steier, H.P.Trautvetter Accelerator mass spectrometry measurements of the 13C(n, γ)14C and 14N(n, p)14C cross sections NUCLEAR REACTIONS 13C(n, γ), 14N(n, p), E=123, 182 keV, and at kT=25 keV neutrons from TRIGA reactor of Atominstitut-Vienna and from Van de Graaff accelerator of Karlsruhe Institute of Technology; measured σ(E) and Maxwellian averaged σ(kT=5-100 keV) using accelerator mass spectrometry (AMS) technique at Vienna Environmental Research Accelerator (VERA) facility. Comparison with previous experimental σ(E), KADONIS compiled data, and JEFF-3.2 evaluated library. Impact of the new stellar cross sections on the s process in low-mass AGB stars using stellar models.
doi: 10.1103/PhysRevC.93.045803
2012ST02 Phys.Lett. B 707, 60 (2012) F.Strieder, B.Limata, A.Formicola, G.Imbriani, M.Junker, D.Bemmerer, A.Best, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, A.DiLeva, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, A.Lemut, M.Marta, C.Mazzocchi, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Terrasi, H.P.Trautvetter The 25Mg(p, γ)26Al reaction at low astrophysical energies NUCLEAR REACTIONS 25Mg(p, γ)26Al, E(cm) = 92, 189 keV; measured reaction products Eγ, Iγ; deduced energy levels, branching ratios, total resonance strength, screening effects.
doi: 10.1016/j.physletb.2011.12.029
2011AD03 Rev.Mod.Phys. 83, 195 (2011) E.G.Adelberger, A.Garcia, R.G.H.Robertson, K.A.Snover, A.B.Balantekin, K.Heeger, M.J.Ramsey-Musolf, A.B.Balantekin, K.Heeger, M.J.Ramsey-Musolf, D.Bemmerer, A.Junghans, D.Bemmerer, A.Junghans, C.A.Bertulani, K.-W.Chen, H.Costantini, P.Prati, M.Couder, E.Uberseder, M.Wiescher, R.Cyburt, B.Davids, S.J.Freedman, M.Gai, D.Gazit, L.Gialanella, G.Imbriani, U.Greife, M.Hass, W.C.Haxton, T.Itahashi, K.Kubodera, K.Langanke, D.Leitner, M.Leitner, P.Vetter, L.Winslow, L.E.Marcucci, T.Motobayashi, A.Mukhamedzhanov, R.E.Tribble, F.M.Nunes, T.-S.Park, R.Schiavilla, E.C.Simpson, C.Spitaleri, F.Strieder, H.-P.Trautvetter, K.Suemmerer, S.Typel Solar fusion cross sections. II. The pp chain and CNO cycles NUCLEAR REACTIONS 2H(p, γ), 3He(3He, 2p), (α, γ), (p, e), 7Be, 12C, 14N, 15N, 17O(p, γ), 15N, 16,17,18O(p, α), E<3 MeV; analyzed and evaluated experimental data; deduced recommended values and uncertainties.
doi: 10.1103/RevModPhys.83.195
2011MA25 Phys.Rev. C 83, 045804 (2011) M.Marta, A.Formicola, D.Bemmerer, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, A.Lemut, B.Limata, C.Mazzocchi, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, A.Vomiero, for the LUNA Collaboration The 14N( p, γ )15O reaction studied with a composite germanium detector NUCLEAR REACTIONS 14N(p, γ), E=359, 380, 399 keV; measured Eγ, Iγ, σ. 15O; deduced levels, J, π, branching ratios for four major resonances, corresponding astrophysical S factors. R-matrix analysis for capture to ground state. Relevance to (CNO) cycle of hydrogen burning.
doi: 10.1103/PhysRevC.83.045804
2010LE21 Phys.Rev. C 82, 055804 (2010), Erratum Phys.Rev. C 84, 019902 (2011) P.J.LeBlanc, G.Imbriani, J.Gorres, M.Junker, R.Azuma, M.Beard, D.Bemmerer, A.Best, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, M.Couder, R.deBoer, Z.Elekes, S.Falahat, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, F.Kappeler, A.Kontos, R.Kuntz, H.Leiste, A.Lemut Q.Li, B.Limata, M.Marta, C.Mazzocchi, R.Menegazzo, S.O'Brien, A.Palumbo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, E.Stech, O.Straniero, F.Strieder, W.Tan, F.Terrasi, H.P.Trautvetter, E.Uberseder, M.Wiescher Constraining the S factor of 15N(p, γ)16O at astrophysical energies NUCLEAR REACTIONS 15N(p, γ), E=130-1800 keV; measured Ep, Ip, Eγ, Iγ, σ(E), σ(θ); deduced resonances, branching ratios, astrophysical S factors and reaction rates. Multilevel R-matrix analysis. Implications for the first and second cycles of the CNO cycles.
doi: 10.1103/PhysRevC.82.055804
2010LI22 Phys.Rev. C 82, 015801 (2010) B.Limata, F.Strieder, A.Formicola, G.Imbriani, M.Junker, H.W.Becker, D.Bemmerer, A.Best, R.Bonetti, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, A.DiLeva, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, A.Lemut, M.Marta, C.Mazzocchi, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, C.Salvo, E.Somorjai, O.Straniero, F.Terrasi, H.-P.Trautvetter, for the LUNA Collaboration New experimental study of low-energy (p, γ) resonances in magnesium isotopes NUCLEAR REACTIONS 24Mg(p, γ)25Al, E=214 keV; 25Mg(p, γ)26Al, E=304 keV; 26Mg(p, γ)27Al, E=326 keV; measured Eγ, Iγ, resonance strengths and thick target yield curves at LUNA facility. 25,26,27Al; deduced levels, γ-ray branching ratios of primary γ rays from capture states.
doi: 10.1103/PhysRevC.82.015801
2010SZ04 Eur.Phys.J. A 44, 513 (2010) T.Szucs, D.Bemmerer, C.Broggini, A.Caciolli, F.Confortola, P.Corvisiero, Z.Elekes, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, A.Lemut, M.Marta, C.Mazzocchi, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, for the LUNA Collaboration An actively vetoed Clover γ-detector for nuclear astrophysics at LUNA NUCLEAR REACTIONS 24Mg(p, γ), E=223 keV; measured Eγ, Iγ. 25Al; deduced levels, J, π, branching ratios.
doi: 10.1140/epja/i2010-10967-1
2009CA05 Eur.Phys.J. A 39, 179 (2009) A.Caciolli, L.Agostino, D.Bemmerer, R.Bonetti, C.Broggini, F.Confortola, P.Corvisiero, H.Costantini, Z.Elekes, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, M.Laubenstein, A.Lemut, B.Limata, M.Marta, C.Mazzocchi, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, for the LUNA Collaboration Ultra-sensitive in-beam γ-ray spectroscopy for nuclear astrophysics at LUNA
doi: 10.1140/epja/i2008-10706-3
2008CO12 Nucl.Phys. A814, 144 (2008) H.Costantini, D.Bemmerer, F.Confortola, A.Formicola, Gy.Gyurky, P.Bezzon, R.Bonetti, C.Broggini, P.Corvisiero, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, M.Laubenstein, A.Lemut, B.Limata, V.Lozza, M.Marta, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter The 3He(α, γ)7Be S-factor at solar energies: The prompt γ experiment at LUNA NUCLEAR REACTIONS 3He(α, γ), E=220, 250, 400 keV; measured Eγ, Iγ, σ, branching ratio; deduced astrophysical S-factor. Prompt-γ technique, HPGe detector in the Gran Sasso underground laboratory. Comparison with other data.
doi: 10.1016/j.nuclphysa.2008.09.014
2008FO04 J.Phys.(London) G35, 014013 (2008) A.Formicola, A.Best, G.Imbriani, M.Junker, D.Bemmerer, R.Bonetti, C.Broggini, A.Caciolli, F.Confortola, P.Corvisiero, H.Costantini, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, G.Gyurky, C.Gustavino, A.Lemut, B.Limata, M.Marta, C.Mazzocchi, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter Measurement of 25Mg(p, γ)26Al resonance strengths via gamma spectrometry NUCLEAR REACTIONS 25Mg(p, γ), E not given;measured Eγ, Iγ; deduced resonance strengths.
doi: 10.1088/0954-3899/35/1/014013
2008GY01 J.Phys.(London) G35, 014002 (2008) G.Gyurky, D.Bemmerer, F.Confortola, H.Costantini, A.Formicola, R.Bonetti, C.Broggini, P.Corvisiero, Z.Elekes, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, M.Laubenstein, A.Lemut, B.Limata, V.Lozza, M.Marta, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter Comparison of the LUNA 3He(α, γ)7Be activation results with earlier measurements and model calculations NUCLEAR REACTIONS 3He(α, γ), E(cm)=92.9, 105.6, 105.7, 126.5, 147.7, 168.9, 169.5 keV; analyzed activation cross sections; calculated S-factor. Comparisons with previous experimental data.
doi: 10.1088/0954-3899/35/1/014002
2008MA36 Phys.Rev. C 78, 022802 (2008) M.Marta, A.Formicola, Gy.Gyurky, D.Bemmerer, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, R.Kunz, A.Lemut, B.Limata, C.Mazzocchi, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, M.Romano, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, A.Vomiero, for the LUNA Collaboration Precision study of ground state capture in the 14N(p, γ)15O reaction NUCLEAR REACTIONS 14N(p, γ), E=359, 380, 399 keV; measured Eγ, Iγ, σ ratios; deduced astrophysical S-factors. R-matrix analysis for capture to g.s. of 15O.
doi: 10.1103/PhysRevC.78.022802
2008SC08 Phys.Rev. C 77, 055803 (2008) D.Schurmann, R.Kunz, I.Lingner, C.Rolfs, F.Schumann, F.Strieder, H.-P.Trautvetter Lifetime measurement of the 6792 keV state in 15O, important for the astrophysical S factor extrapolation in 14N(p, γ)15O NUCLEAR REACTIONS 14N(p, γ), E=318 keV; measured Eγ, Iγ, γ∓coin, lifetimes using Doppler-shift attenuation method. 15O; deduced levels, J, π, astrophysical S factors. 19F(p, αγ), E=318 keV; measured Eγ, Iγ.
doi: 10.1103/PhysRevC.77.055803
2008TR03 J.Phys.(London) G35, 014019 (2008) H.P.Trautvetter, D.Bemmerer, R.Bonetti, C.Broggini, A.Caciolli, F.Confortola, P.Corvisiero, H.Costantini, Z.Elekes, A.Formicola, Z.Fulop, G.Gervino, A.Guglielmetti, G.Gyurky, C.Gustavino, G.Imbriani, M.Junker, A.Lemut, B.Limata, M.Marta, C.Mazzocchi, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, S.Vezzu, A.Vomiero, for the LUNA Collaboration Ground state capture in 14N(p, γ)15O studied above the 259 keV resonance at LUNA NUCLEAR REACTIONS 14N(p, γ), E=360, 380, 400 keV; measured Eγ, Iγ, cross sections; deduced astrophysical S-factor. Comparisons with existing data. R-matrix analysis.
doi: 10.1088/0954-3899/35/1/014019
2007CO17 Phys.Rev. C 75, 065803 (2007); Pub.Note: Phys.Rev. C 75, 069903 (2007) F.Confortola, D.Bemmerer, H.Costantini, A.Formicola, Gy.Gyurky, P.Bezzon, R.Bonetti, C.Broggini, P.Corvisiero, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, M.Laubenstein, A.Lemut, B.Limata, V.Lozza, M.Marta, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, and the LUNA Collaboration Astrophysical S factor of the 3He(α, γ)7Be reaction measured at low energy via detection of prompt and delayed γ rays NUCLEAR REACTIONS 3He(α, γ), E=220, 250, 400 keV; measured Eγ, Iγ. Deduced cross section and S-factor.
doi: 10.1103/PhysRevC.75.065803
2007GY01 Phys.Rev. C 75, 035805 (2007) Gy.Gyurky, F.Confortola, H.Costantini, A.Formicola, D.Bemmerer, R.Bonetti, C.Broggini, P.Corvisiero, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, M.Laubenstein, A.Lemut, B.Limata, V.Lozza, M.Marta, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, and the LUNA Collaboration 3He(α, γ)7Be cross section at low energies NUCLEAR REACTIONS 3He(α, γ), E=250, 300, 350, 400 keV; measured Eγ, Iγ, σ; deduced astrophysical S-factor.
doi: 10.1103/PhysRevC.75.035805
2006BE41 Phys.Rev.Lett. 97, 122502 (2006) D.Bemmerer, F.Confortola, H.Costantini, A.Formicola, Gy.Gyurky, R.Bonetti, C.Broggini, P.Corvisiero, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, M.Laubenstein, A.Lemut, B.Limata, V.Lozza, M.Marta, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, C.Rossi Alvarez, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, and the LUNA Collaboration Activation Measurement of the 3He(α, γ)7Be Cross Section at Low Energy NUCLEAR REACTIONS 3He(α, γ), E=300, 350, 400 keV; measured σ; deduced astrophysical S-factors. Activation technique.
doi: 10.1103/PhysRevLett.97.122502
2006BE44 Eur.Phys.J. A 27, Supplement 1, 161 (2006) D.Bemmerer, F.Confortola, A.Lemut, R.Bonetti, C.Broggini, P.Corvisiero, H.Costantini, J.Cruz, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, B.Limata, R.Menegazzo, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, and the LUNA Collaboration CNO hydrogen burning studied deep underground
doi: 10.1140/epja/i2006-08-024-7
2006BE50 Nucl.Phys. A779, 297 (2006) D.Bemmerer, F.Confortola, A.Lemut, R.Bonetti, C.Broggini, P.Corvisiero, H.Costantini, J.Cruz, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, A.Jesus, M.Junker, B.Limata, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, D.Rogalla, M.Romano, C.Rossi-Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, and the LUNA Collaboration Low energy measurement of the 14N(p, γ)15O total cross section at the LUNA underground facility NUCLEAR REACTIONS 14N(p, γ), E=70-228 keV; measured Eγ, σ; deduced astrophysical S-factor, resonance strength.
doi: 10.1016/j.nuclphysa.2006.09.001
2006CO13 Eur.Phys.J. A 27, Supplement 1, 177 (2006) H.Costantini, D.Bemmerer, P.Bezzon, R.Bonetti, C.Broggini, M.L.Casanova, F.Confortola, P.Corvisiero, J.Cruz, Z.Elekes, A.Formicola, Zs.Fulop, G.Gervino, C.Gustavino, A.Guglielmetti, Gy.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, A.Lemut, M.Marta, R.Menegazzo, P.Prati, E.Roca, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter Towards a high-precision measurement of the 3He(α, γ)7Be cross section at LUNA NUCLEAR REACTIONS 3He(α, γ), E=280, 327, 373 keV; calculated expected counting rate for activation experiment.
doi: 10.1140/epja/i2006-08-026-5
2006LE13 Phys.Lett. B 634, 483 (2006) A.Lemut, D.Bemmerer, F.Confortola, R.Bonetti, C.Broggini, P.Corvisiero, H.Costantini, J.Cruz, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, B.Limata, R.Menegazzo, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, and the LUNA Collaboration First measurement of the 14N(p, γ)15O cross section down to 70 keV NUCLEAR REACTIONS 14N(p, γ), E=70-228 keV; measured Eγ, Iγ, σ; deduced astrophysical S-factor and thermonuclear reaction rate. 14N(p, γ), E=259 keV; measured Eγ, Iγ; deduced resonance strength. Comparison with other data, discussed astrophysical consequences.
doi: 10.1016/j.physletb.2006.02.021
2005AN22 Nucl.Phys. A758, 391c (2005) C.Angulo, A.E.Champagne, H.-P.Trautvetter R-matrix analysis of the 14N(p, γ)15O astrophysical S-factor NUCLEAR REACTIONS 14N(p, γ), E(cm) ≈ 0-1500 keV; analyzed data; deduced S-factors, astrophysical reaction rate. R-matrix analysis.
doi: 10.1016/j.nuclphysa.2005.05.070
2005BE28 Eur.Phys.J. A 24, 313 (2005) D.Bemmerer, F.Confortola, A.Lemut, R.Bonetti, C.Broggini, P.Corvisiero, H.Costantini, J.Cruz, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, B.Limata, R.Menegazzo, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, A.Vomiero Feasibility of low-energy radiative-capture experiments at the LUNA underground accelerator facility
doi: 10.1140/epja/i2004-10135-4
2005CO16 Nucl.Phys. A758, 383c (2005) H.Costantini, C.Angulo, D.Bemmerer, R.Bonetti, C.Broggini, F.Confortola, P.Corvisiero, J.Cruz, P.Descouvemont, A.Formicola, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, A.Lemut, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, A.Vomiero, S.Zavatarelli Recent results of the 14N(p, γ)15O measurement at LUNA NUCLEAR REACTIONS 14N(p, γ), E=low; measured Eγ, Iγ; deduced S-factors.
doi: 10.1016/j.nuclphysa.2005.05.069
2005IM02 Eur.Phys.J. A 25, 455 (2005) G.Imbriani, H.Costantini, A.Formicola, A.Vomiero, C.Angulo, D.Bemmerer, R.Bonetti, C.Broggini, F.Confortola, P.Corvisiero, J.Cruz, P.Descouvemont, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, A.P.Jesus, M.Junker, J.N.Klug, A.Lemut, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, M.Romano, C.Rossi-Alvarez, F.Schumann, D.Schurmann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter S-factor of 14N(p, γ)15O at astrophysical energies NUCLEAR REACTIONS 14N(p, γ), E(cm)=119-367 keV; measured Eγ, Iγ, excitation functions; deduced astrophysical S-factors. R-matrix analysis.
doi: 10.1140/epja/i2005-10138-7
2005PR20 J.Phys.(London) G31, S1537 (2005) P.Prati, D.Bemmerer, R.Bonetti, C.Broggini, F.Confortola, P.Corvisiero, H.Costantini, J.Cruz, A.Formicola, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, A.Lemut, R.Menegazzo, V.Roca, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter Recent results from the LUNA facility at Gran Sasso NUCLEAR REACTIONS 14N(p, γ), E=low; measured Eγ, Iγ; deduced astrophysical S-factor. Solid and gas targets.
doi: 10.1088/0954-3899/31/10/027
2005SC17 Nucl.Phys. A758, 367c (2005) D.Schurmann, A.Di Leva, N.De Cesare, L.Gialanella, G.Imbriani, C.Lubritto, A.Ordine, V.Roca, H.Rocken, C.Rolfs, D.Rogalla, M.Romano, F.Schumann, F.Strieder, F.Terrasi, H.-P.Trautvetter Measurement of the cross section of 12C(α, γ)16O using the recoil mass separator ERNA NUCLEAR REACTIONS 12C(α, γ), E(cm)=1.3-5.0 MeV; measured Eγ, Iγ, (recoil)γ-coin; deduced astrophysical S-factors. Recoil mass separator.
doi: 10.1016/j.nuclphysa.2005.05.067
2005SC29 Eur.Phys.J. A 26, 301 (2005) D.Schurmann, A.Di Leva, L.Gialanella, D.Rogalla, F.Strieder, N.De Cesare, A.D'Onofrio, G.Imbriani, R.Kunz, C.Lubritto, A.Ordine, V.Roca, C.Rolfs, M.Romano, F.Schumann, F.Terrasi, H.-P.Trautvetter First direct measurement of the total cross-section of 12C(α, γ)16O NUCLEAR REACTIONS 4He(12C, γ), E=0.7-5.0 MeV; measured total recoil spectra, σ. 12C(α, γ), E=1.9-4.9 MeV; deduced astrophysical S-factors.
doi: 10.1140/epja/i2005-10175-2
2004CO27 Nuovo Cim. C 27, 423 (2004) F.Confortola, D.Bemmerer, R.Bonetti, C.Broggini, P.Corvisiero, H.Costantini, J.Cruz, A.Formicola, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Gyurky, G.Imbriani, A.P.Jesus, M.Junker, A.Lemut, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli The 14N(p, γ)15O measurement at low energy NUCLEAR REACTIONS 14N(p, γ), E=low; measured astrophysical S-factors. Solid and gas targets.
doi: 10.1393/ncc/i2005-10009-5
2004FO02 Phys.Lett. B 591, 61 (2004) A.Formicola, G.Imbriani, H.Costantini, C.Angulo, D.Bemmerer, R.Bonetti, C.Broggini, P.Corvisiero, J.Cruz, P.Descouvemont, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Gyurky, A.P.Jesus, M.Junker, A.Lemut, R.Menegazzo, P.Prati, V.Roca, C.Rolfs, M.Romano, C.Rossi Alvarez, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, A.Vomiero, S.Zavatarelli Astrophysical S-factor of 14N(p, γ)15O NUCLEAR REACTIONS 14N(p, γ), E=140-400 keV; measured Eγ, Iγ, capture σ; deduced astrophysical S-factor. R-matrix analysis.
doi: 10.1016/j.physletb.2004.03.092
2002GI12 Nucl.Instrum.Methods Phys.Res. B197, 150 (2002) L.Gialanella, U.Greife, N.De Cesare, A.D'Onofrio, M.Romano, L.Campajola, A.Formicola, Z.Fulop, G.Gyurky, G.Imbriani, C.Lubritto, A.Ordine, V.Roca, D.Rogalla, C.Rolfs, M.Russo, C.Sabbarese, E.Somorjai, F.Strieder, F.Terrasi, H.P.Trautvetter Off-Line production of a 7Be radioactive ion beam NUCLEAR REACTIONS 7Li(p, n), E=11.4 MeV; measured yield; deduced radioactive beam production features.
doi: 10.1016/S0168-583X(02)01386-1
2002RA11 Eur.Phys.J. A 13, 377 (2002) F.Raiola, P.Migliardi, G.Gyurky, M.Aliotta, A.Formicola, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, H.Costantini, J.Cruz, A.D'Onofrio, Z.Fulop, G.Gervino, L.Gialanella, A.Guglielmetti, G.Imbriani, C.Gustavino, A.P.Jesus, M.Junker, R.W.Kavanagh, P.G.P.Moroni, A.Ordine, J.V.Pinto, E.Somorjai, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli Enhanced Electron Screening in d(d, p) for Deuterated Ta NUCLEAR REACTIONS 2H(d, p), E=2.10, 21.5 keV; measured σ, astrophysical S-factor; deduced electron screening potential for atomic and molecular beams and a deuterated Ta target. Possible causes for a large electron screening discussed.
doi: 10.1007/s10050-002-8766-5
2001AL25 Nucl.Phys. A690, 790 (2001) M.Aliotta, F.Raiola, G.Gyurky, A.Formicola, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, H.Costantini, A.D'Onofrio, Z.Fulop, G.Gervino, L.Gialanella, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, P.G.Moroni, A.Ordine, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli Electron Screening Effect in the Reactions 3He(d, p)4He and d(3He, p)4He NUCLEAR REACTIONS 3He(d, p), E(cm)=5-60 keV; 2H(3He, p), E(cm)=10-40 keV; measured proton spectra, excitation functions, S(E); deduced electron screening contributions.
doi: 10.1016/S0375-9474(01)00366-9
2001GI03 Nucl.Phys. A688, 254c (2001) L.Gialanella, M.Aliotta, D.Rogalla, C.Rolfs, F.Schumann, F.Strieder, S.Theis, H.P.Trautvetter, L.Campajola, G.Imbriani, V.Roca, M.Romano, A.D'Onofrio, C.Sabbarese, F.Terrasi, C.Agodi, R.Alba, A.Del Zoppo, P.Figuera, P.Sapienza, C.Spitaleri, G.Gyurky, E.Somorjai, U.Greife A New Measurement of the E1 Amplitude in 12C(α, γ0)16O NUCLEAR REACTIONS 4He(12C, γ), E=5.8-12.4 MeV; measured Eγ, σ, E1 S factor. R-matrix calculations.
doi: 10.1016/S0375-9474(01)00709-6
2001GI11 Eur.Phys.J. A 11, 357 (2001) L.Gialanella, D.Rogalla, F.Strieder, S.Theis, G.Gyurky, C.Agodi, R.Alba, M.Aliotta, L.Campajola, A.Del Zoppo, A.D'Onofrio, P.Figuera, U.Greife, G.Imbriani, A.Ordine, V.Roca, C.Rolfs, M.Romano, C.Sabbarese, P.Sapienza, F.Schumann, E.Somorjai, F.Terrasi, H.P.Trautvetter The E1 Capture Amplitude in 12C(α, γ0)16O NUCLEAR REACTIONS 4He(12C, γ), (12C, 12C), E(cm)=1.10-3.103 MeV; measured Eγ, σ, S-factor. Astrophysics implications discussed.
doi: 10.1007/s100500170075
2001RA21 Eur.Phys.J. A 10, 487 (2001) F.Raiola, G.Gyurky, M.Aliotta, A.Formicola, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, H.Costantini, A.D'Onofrio, Z.Fulop, G.Gervino, L.Gialanella, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, R.W.Kavanagh, P.G.P.Moroni, A.Ordine, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli Stopping Power of Low-Energy Deuterons in 3He Gas NUCLEAR REACTIONS 3He(d, p), E=10-100 keV; measured proton spectra; deduced deuteron stpping power in He gas.
doi: 10.1007/s100500170107
2001RO17 Nucl.Phys. A688, 549c (2001) D.Rogalla, M.Aliotta, C.A.Barnes, L.Campajola, A.D'Onofrio, L.Gialanella, U.Greife, G.Imbriani, A.Ordine, V.Roca, C.Rolfs, M.Romano, C.Sabbarese, D.Schurmann, F.Schumann, F.Strieder, S.Theis, F.Terrasi, H.P.Trautvetter Recoil Separator ERNA: Improved measurements of the astrophysical key reaction 12C(α, γ)16O NUCLEAR REACTIONS 12C(α, γ), E=low; analyzed data, future measurement discussed.
doi: 10.1016/S0375-9474(01)00784-9
2001ST27 Nucl.Phys. A696, 219 (2001) F.Strieder, L.Gialanella, G.Gyurky, F.Schumann, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, H.Costantini, A.D'Onofrio, A.Formicola, Z.Fulop, G.Gervino, U.Greife, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, P.G.P.Moroni, A.Ordine, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, E.Somorjai, O.Straniero, F.Terrasi, H.P.Trautvetter, S.Zavatarelli Absolute Cross Section of 7Be(p, γ)8B NUCLEAR REACTIONS 7Be(p, γ), E(cm)=0.32-2.61 MeV; measured delayed Eα, σ(E); deduced astrophysical S-factor. Comparison with previous results.
doi: 10.1016/S0375-9474(01)01121-6
2001TE03 Nucl.Phys. A688, 539c (2001) F.Terrasi, L.Gialanella, G.Imbriani, F.Strieder, L.Campajola, A.D'Onofrio, U.Greife, G.Gyurky, C.Lubritto, A.Ordine, V.Roca, C.Rolfs, M.Romano, D.Rogalla, C.Sabbarese, E.Somorjai, H.P.Trautvetter Direct Measurement of the Absolute Cross Section of p(7Be, γ)8B NUCLEAR REACTIONS 1H(7Be, γ), E=8 MeV; measured σ, S-factor. Comparison with earlier data.
doi: 10.1016/S0375-9474(01)00781-3
2001ZA07 Nucl.Phys. A688, 514c (2001) S.Zavatarelli, P.Corvisiero, H.Costantini, P.G.Prada Moroni, P.Prati, R.Bonetti, A.Guglielmetti, C.Broggini, L.Campajola, A.Formicola, L.Gialanella, G.Imbriani, A.Ordine, V.Roca, M.Romano, A.D'Onofrio, F.Terrasi, G.Gervino, C.Gustavino, M.Junker, D.Rogalla, C.Rolfs, F.Schumann, F.Strieder, H.P.Trautvetter The D(3He, p)4He Fusion Reaction: Electron screening effect and astrophysical S(E) factor at low energies NUCLEAR REACTIONS 2H(3He, p), E=4.2-13.8 keV; measured σ, S-factor. Comparison with earlier data and with calculations that include electron screening effects.
doi: 10.1016/S0375-9474(01)00773-4
2000CO17 Phys.Lett. 482B, 43 (2000) H.Costantini, A.Formicola, M.Junker, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, A.D'Onofrio, A.Fubini, G.Gervino, L.Gialanella, U.Greife, A.Guglielmetti, C.Gustavino, G.Imbriani, A.Ordine, P.G.Prada Moroni, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, F.Schumann, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli Stopping Power, Electron Screening and the Astrophysical S(E) Factor of d(3He, p)4He NUCLEAR REACTIONS 2H(3He, p), E=11-35 keV; measured σ; deduced electron screening effect, stopping power, astrophysical S factor. Gas target.
doi: 10.1016/S0370-2693(00)00513-X
2000FO14 Eur.Phys.J. A 8, 443 (2000) A.Formicola, M.Aliotta, G.Gyurky, F.Raiola, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, H.Costantini, A.D'Onofrio, Z.Fulop, G.Gervino, L.Gialanella, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, A.Ordine, P.Prati, V.Roca, D.Rogalla, C.Rolfs, M.Romano, F.Schumann, E.Somorjai, O.Straniero, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli Energy Loss of Deuterons in 3He Gas: A threshold effect NUCLEAR REACTIONS 3He(d, p), E=15-100 keV; measured proton yield; deduced stopping power by normalizing yield to known cross section. Nuclear astrophysics implications discussed.
doi: 10.1007/s100530050054
2000GI04 Eur.Phys.J. A 7, 303 (2000) L.Gialanella, F.Strieder, L.Campajola, A.D'Onofrio, U.Greife, G.Gyurky, G.Imbriani, G.Oliviero, A.Ordine, V.Roca, C.Rolfs, M.Romano, D.Rogalla, C.Sabbarese, E.Somorjai, F.Terrasi, H.P.Trautvetter Absolute Cross Section of p(7Be, γ)8B using a Novel Approach NUCLEAR REACTIONS 1H(7Be, γ), E(cm)=992 keV; measured σ; deduced S factor. Comparison with other measurements, radioactive beams, nuclear astrophysics.
doi: 10.1007/PL00013599
1999BO23 Phys.Rev.Lett. 82, 5205 (1999) R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, A.D'Alessandro, M.Dessalvi, A.D'Onofrio, A.Fubini, G.Gervino, L.Gialanella, U.Greife, A.Guglielmetti, C.Gustavino, G.Imbriani, M.Junker, P.Prati, V.Roca, C.Rolfs, M.Romano, F.Schuemann, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli, and the LUNA Collaboration First Measurement of the 3He(3He, 2p)4He Cross Section Down to the Lower Edge of the Solar Gamow Peak NUCLEAR REACTIONS 3He(3He, 2p), E(cm)=16.5-24.4 keV; measured σ, astrophysical S-factor; deduced electron screening effect, no narrow resonance.
doi: 10.1103/PhysRevLett.82.5205
1999BU26 J.Phys.(London) G25, L71 (1999) B.Burggraf, K.Farzin, J.Grabis, Th.Last, E.Manthey, H.P.Trautvetter, C.Rolfs Energy Shift of First Excited State in 10Be ? NUCLEAR REACTIONS 9Be(d, p), E=1.0 MeV; measured Eγ, Iγ(θ). 10Be deduced level energy. Comparison with ternary fission results.
doi: 10.1088/0954-3899/25/9/101
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
1999PR12 Nucl.Phys. (Supplement) A654, 920c (1999) P.Prati, R.Bonetti, C.Broggini, L.Campajola, P.Corvisiero, A.D'Alessandro, M.Dessalvi, A.D'Onofrio, A.Fubini, G.Gervino, L.Gialanella, U.Greife, A.Guglielmetti, C.Gustavino, M.Junker, A.Ordine, V.Roca, C.Rolfs, M.Romano, F.Schuemann, F.Strieder, F.Terrasi, H.P.Trautvetter, S.Zavatarelli The LUNA Facility at the National Laboratory of Gran Sasso: Recent results and future activities NUCLEAR REACTIONS 3He(3He, 2p), E(cm)=16-25 keV; measured astrophysical S-factors, upper limits. Plans for future experiments discussed.
doi: 10.1016/S0375-9474(00)88573-5
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
1999RO25 Eur.Phys.J. A 6, 471 (1999) D.Rogalla, M.Aliotta, C.A.Barnes, L.Campajola, A.D'Onofrio, E.Fritz, L.Gialanella, U.Greife, G.Imbriani, A.Ordine, J.Ossmann, V.Roca, C.Rolfs, M.Romano, C.Sabbarese, D.Schurmann, F.Schumann, F.Strieder, S.Theis, F.Terrasi, H.P.Trautvetter Recoil Separator ERNA: Ion beam specifications
doi: 10.1007/s100500050371
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
1998SC38 Eur.Phys.J. A 2, 337 (1998) F.Schumann, S.Zavatarelli, L.Gialanella, U.Greife, M.Junker, D.Rogalla, C.Rolfs, F.Strieder, H.P.Trautvetter Electron Screening in Backward Elastic Scattering NUCLEAR REACTIONS W, Ta(α, α), E=76-3988 keV; measured σ(Eα, θ=165°); deduced atomic screening potential energy.
doi: 10.1007/s100500050130
1998SO07 Astron.Astrophys. 333, 1112 (1998) E.Somorjai, Zs.Fulop, A.Z.Kiss, C.E.Rolfs, H.P.Trautvetter, U.Greife, M.Junker, S.Goriely, M.Arnould, M.Rayet, T.Rauscher, H.Oberhummer Experimental Cross Section of 144Sm(α, γ)148Gd and Implications for the p-Process NUCLEAR REACTIONS 144Sm(α, γ), E=10.5-13.4 MeV; measured σ; deduced astrophysical S-factors, stellar production ratio. Activation method. Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0416. 1998ST20 Eur.Phys.J. A 3, 1 (1998) F.Strieder, F.Schumann, L.Gialanella, U.Greife, D.Rogalla, C.Rolfs, H.P.Trautvetter, Zs.Fulop, G.Gyurky, E.Somorjai, R.W.Kavanagh, L.Campajola, A.D'Onofrio, A.Ordine, V.Roca, M.Romano, F.Terrasi, C.Arpesella, A.D'Alessandro, C.Gustavino, M.Junker, O.Straniero, P.Corvisiero, M.Dessalvi, P.Prati, S.Zavatarelli, C.Broggini, G.Gervino, A.Fubini, E.Bellotti, R.Bonetti, A.Guglielmetti Loss of 8Li Recoil Nuclei in 7Li(d, p)8Li and Implications on the 7Be(p, γ)8B Cross Section NUCLEAR REACTIONS 7Li(d, p), E=0.4-1.8 MeV; measured yields; deduced recoil loss for several backing materials. 7Be(p, γ), E not given; deduced possible corrections to σ. Astrophysical implications.
doi: 10.1007/s100500050141
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
1997SO19 Nucl.Phys. A621, 293c (1997) E.Somorjai, Zs.Fulop, A.Z.Kiss, C.Rolfs, H.-P.Trautvetter, U.Greife, M.Junker, M.Arnould, M.Rayet, H.Oberhummer Experimental Cross Section of 144Sm(α, γ)148Gd NUCLEAR REACTIONS, ICPND 144Sm(α, γ), E=10.5-13.4 MeV; measured residual nucleus α-decay; deduced production σ. Activation method, solid state nuclear track detectors. Statistical model calculations.
doi: 10.1016/S0375-9474(97)00258-3
1997ST19 Nucl.Phys. A621, 123c (1997) F.Strieder, L.Campajola, A.D'Onofrio, L.Gialanella, U.Greife, V.Roca, C.Rolfs, M.Romano, M.Romoli, S.Schmidt, W.H.Schulte, H.P.Trautvetter, D.Zahnow The d(7Li, p)8Li Cross Section Near E(cm) = 0.61 MeV NUCLEAR REACTIONS, ICPND 2H(7Li, 8Li), E=0.47-4 MeV; measured recoil β-delayed α-decay spectra; deduced σ.
doi: 10.1016/S0375-9474(97)00222-4
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
1997ZA06 Z.Phys. A359, 211 (1997) D.Zahnow, C.Rolfs, S.Schmidt, H.P.Trautvetter Low-Energy S(E) Factor of 9Be(p, α)6Li and 9Be(p, d)8Be NUCLEAR REACTIONS, ICPND 9Be(p, α), (p, d), E=16-390 keV; measured astrophysical S-factors, σ(θ). 10B deduced resonances E, Γ.
doi: 10.1007/s002180050389
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
1996AR23 Nucl.Phys. B(Proc.Suppl.) S48, 375 (1996) C.Arpesella, F.Bartolucci, E.Bellotti, C.Broggini, P.Corvisiero, G.Fiorentini, A.Fubini, G.Gervino, U.Greife, C.Gustavino, M.Junker, P.Prati, C.Rolfs, H.P.Trautvetter, D.Zahnow, S.Zavatarelli Status of the LUNA Experiment
doi: 10.1016/0920-5632(96)00275-7
1996CA43 Z.Phys. A356, 107 (1996) L.Campajola, L.Gialanella, K.Brand, A.D'Onofrio, U.Greife, E.Huttel, R.Kubat, G.Oliviero, H.Rebel, V.Roca, C.Rolfs, M.Romano, M.Romoli, S.Schmidt, W.H.Schulte, F.Strieder, F.Terrasi, H.-P.Trautvetter, D.Zahnow Production of an 8.0 MeV 7Be Ion Beam at the Naples TTT-3 Accelerator NUCLEAR REACTIONS 1H(7Be, γ), E=8 MeV; measured residual nuclei production. Radioactive beam from 7Li(p, n) reaction.
doi: 10.1007/s002180050154
1996FU11 Z.Phys. A355, 203 (1996) Zs.Fulop, A.Z.Kiss, E.Somorjai, C.E.Rolfs, H.P.Trautvetter, T.Rauscher, H.Oberhummer 70Ge(α, γ)74Se Cross Section Measurements at Energies of Astrophysical Interest NUCLEAR REACTIONS, ICPND 70Ge(α, γ), E=5.05-7.8 MeV; measured Eγ, Iγ, γγ-coin; deduced σ(E), astrophysical S-factor vs E, (α, γ), (γ, α) reaction rates. Statistical model comparison.
doi: 10.1007/s002180050099
1996GI11 Nucl.Instrum.Methods Phys.Res. A376, 174 (1996) L.Gialanella, F.Strieder, K.Brand, L.Campajola, A.D'Onofrio, U.Greife, E.Huttel, F.Petrazzuolo, V.Roca, C.Rolfs, M.Romano, M.Romoli, S.Schmidt, W.H.Schulte, F.Terrasi, H.P.Trautvetter, D.Zahnow A Recoil Separator for the Measurement of Radiative Capture Reactions NUCLEAR REACTIONS 1H(12C, γ), E=2, 11 MeV; measured Eγ, Iγ; deduced absolute reaction σ. Recoil separator plus windowless gas target.
doi: 10.1016/0168-9002(96)00264-1
1996ST08 Nucl.Phys. A601, 168 (1996) F.Stegmuller, C.Rolfs, S.Schmidt, W.H.Schulte, H.P.Trautvetter, R.W.Kavanagh 22Na(p, γ)23Mg Resonant Reaction at Low Energies NUCLEAR REACTIONS 22Na(p, γ), E=0.2-0.63 MeV; measured γ-spectra; deduced reaction rates. 23Mg deduced resonance energies, resonance strengths, reaction rates.
doi: 10.1016/0375-9474(96)00084-X
1996ST18 Z.Phys. A355, 209 (1996) F.Strieder, L.Gialanella, U.Greife, C.Rolfs, S.Schmidt, W.H.Schulte, H.P.Trautvetter, D.Zahnow, F.Terrasi, L.Campajola, A.D'Onofrio, V.Roca, M.Romano, M.Romoli The d(7Li, p)8Li Cross Section Near E(cm) = 0.61 MeV NUCLEAR REACTIONS, ICPND 2H(7Li, p), E(cm) ≈ 0.61 MeV; measured proton yield, β-delayed α-activity of residual 8Li. 2H(7Li, p), E(cm)=0.5-0.75 MeV; measured σ(θ); deduced absolute σ(E), consequences for expected flux of high energy solar neutrinos.
doi: 10.1007/s002180050100
1995SC36 Nucl.Phys. A591, 227 (1995) S.Schmidt, C.Rolfs, W.H.Schulte, H.P.Trautvetter, R.W.Kavanagh, C.Hategan, S.Faber, B.D.Valnion, G.Graw 22Na(3He, d)23Mg Reaction Studies of States Near the Proton Threshold and Hydrogen Burning of 22Na NUCLEAR REACTIONS 22Na(3He, d), E=30 MeV; measured deuteron spectra, σ(θ); deduced stellar reaction rates. 23Mg deduced resonances, J, π, Γ(p), resonance strengths. DWBA analysis.
doi: 10.1016/0375-9474(95)00164-V
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
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
1994KI02 Nucl.Phys. A567, 354 (1994) J.D.King, R.E.Azuma, J.B.Vise, J.Gorres, C.Rolfs, H.P.Trautvetter, A.E.Vlieks Cross Section and Astrophysical S-Factor for the 13C(p, γ)14N Reaction NUCLEAR REACTIONS, ICPND 13C(p, γ), E=120-950 keV; measured γ-ray yield 14N. 13C(p, γ), E=120-950 keV; calculated astrophysical S-factor, thermonuclear reaction rate. 14N deduced resonance parameters, branching ratios, direct capture contributions, spectroscopic factors for proton-bound states.
doi: 10.1016/0375-9474(94)90154-6
1994PR09 Z.Phys. A350, 171 (1994) P.Prati, C.Arpesella, F.Bartolucci, H.W.Becker, E.Bellotti, C.Broggini, P.Corvisiero, G.Fiorentini, A.Fubini, G.Gervino, F.Gorris, U.Greife, C.Gustavino, M.Junker, C.Rolfs, W.H.Schulte, H.P.Trautvetter, D.Zahnow Electron Screening in the d + 3He Fusion Reaction NUCLEAR REACTIONS, ICPND 2H(3He, p), E(cm)=5.4-31.3 keV; measured spectra, astrophysical S-factor; deduced electron screening potential. Windowless gas target system.
doi: 10.1007/BF01290685
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
1993GI04 Nucl.Phys. A561, 95 (1993) U.Giesen, C.P.Browne, J.Gorres, S.Graff, C.Iliadis, H.-P.Trautvetter, M.Wiescher, V.Harms, K.L.Kratz, B.Pfeiffer, R.E.Azuma, M.Buckby, J.D.King The Astrophysical Implications of Low-Energy Resonances in 22Ne + α NUCLEAR REACTIONS 22Ne(6Li, d), E=32 MeV; measured σ(θ), σ(Ed). 22Ne(α, n), E=0.6-9 MeV; measured neutron yield vs E; deduced model parameters, resonance yield, reaction rates. 26Mg deduced resonances, J, π, α-spectroscopic factors, resonance strength.
doi: 10.1016/0375-9474(93)90167-V
1993IL01 Nucl.Phys. A559, 83 (1993) C.Iliadis, J.Gorres, J.G.Ross, K.W.Scheller, M.Wiescher, C.Grama, Th.Schange, H.P.Trautvetter, H.C.Evans Explosive Hydrogen Burning of 31P NUCLEAR REACTIONS, ICPND 31P(p, γ), (p, α), E=160-370 keV; 28Si(α, γ), E=2.4-2.6 MeV; measured γ yield vs E; deduced stellar reaction rates, temperature dependence. 32S deduced proton thershold state features.
doi: 10.1016/0375-9474(93)90181-V
1993IL02 Phys.Rev. C48, R1479 (1993) C.Iliadis, J.Hohne, F.Kappeler, J.Meissner, H.P.Trautvetter, M.Wiescher Measurement of the Resonance at E(R) = 1422 keV in 36Ar(p, γ)37K NUCLEAR REACTIONS 36Ar(p, γ), E=0.90-1.45 MeV; measured γ yield, θγ=45°, Eγ, Iγ. 37K deduced level, Γγ/Γp, resonance strength, Gamow-Teller transition strength.
doi: 10.1103/PhysRevC.48.R1479
1993SC36 Astrophys.J. 413, 750 (1993) H.Schatz, F.Kappeler, P.E.Koehler, M.Wiescher, H.-P.Trautvetter 17O(n, α)14C: Closure of Primordial CNO Bi-Cycle ( Question ) NUCLEAR REACTIONS 17O(n, α), E=10-250 keV; measured σ(E); calculated astrophysical reaction rates, big bang model implications. Other data input.
doi: 10.1086/173042
1993TR06 J.Phys.(London) G19, S95 (1993) Charged-Particle Thermonuclear Reactions NUCLEAR REACTIONS, ICPND 3He(3He, 2p), E(cm) ≤ 350 keV; 7Be(p, γ), E ≈ 0.01 MeV; compiled, reviewed σ(E), astrophysical S-factor vs E, data, calculations. Other reactions, aspects discussed.
doi: 10.1088/0954-3899/19/S/008
1992BE21 Z.Phys. A343, 483 (1992) M.Berheide, C.Rolfs, U.Schroder, H.P.Trautvetter Search for the 70 keV Resonance in 17O(p, α)14N NUCLEAR REACTIONS, ICPND 17O(p, α), E ≈ 140-200 MeV; measured thick target yield curves; deduced resonance strength upper limit near 70 keV resonance in 18F.
doi: 10.1007/BF01289827
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
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
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
1990IL01 Nucl.Phys. A512, 509 (1990) Ch.Iliadis, Th.Schange, C.Rolfs, U.Schroder, E.Somorjai, H.P.Trautvetter, K.Wolke, P.M.Endt, S.W.Kikstra, A.E.Champagne, M.Arnould, G.Paulus Low-Energy Resonances in 25Mg(p, γ)26Al, 26Mg(p, γ)27Al and 27Al(p, γ)28Si NUCLEAR REACTIONS 25,26Mg, 27Al(p, γ), E < 340 keV; measured γ-spectra, γ-branchings. 26,27Al, 28Si deduced resonances, J, π, Γ, γ-branching ratios.
doi: 10.1016/0375-9474(90)90084-Y
1990SE09 Nucl.Phys. A514, 471 (1990) S.Seuthe, C.Rolfs, U.Schroder, W.H.Schulte, E.Somorjai, H.P.Trautvetter, F.B.Waanders, R.W.Kavanagh, H.Ravn, M.Arnould, G.Paulus Resonances in the 22Na(p, γ)23Mg Reaction NUCLEAR REACTIONS, ICPND 22Na(p, γ), E=0.17-1.29 MeV; measured γ-spectra; deduced stellar reaction rates. 23Mg deduced resonances, resonance strengths.
doi: 10.1016/0375-9474(90)90153-D
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. 1989WU03 Nucl.Instrum.Methods Phys.Res. B40/41, 413 (1989) S.Wustenbecker, W.H.Schulte, H.Ebbing, H.Baumeister, H.W.Becker, B.Cleff, C.Rolfs, H.P.Trautvetter, G.E.Mitchell, J.S.Schweitzer, C.A.Peterson Technical Improvements for High Resolution Ion Beam Experiments NUCLEAR REACTIONS 23Na(p, γ), E ≈ 309 keV; 27Al(p, γ), E ≈ 327 keV; measured thick target γ yield curve.
doi: 10.1016/0168-583X(89)91010-0
1989WU06 Nucl.Instrum.Methods Phys.Res. A279, 448 (1989) S.Wustenbecker, H.Ebbing, W.H.Schulte, H.Baumeister, H.W.Becker, B.Cleff, C.Rolfs, H.P.Trautvetter, G.E.Mitchell, J.S.Schweitzer, C.A.Peterson Improvements in Targetry and High Voltage Stability for High Resolution Ion Beam Experiments NUCLEAR REACTIONS 23Na(p, γ), E=0.309 MeV; 21Ne(p, γ), E ≈ 0.272 MeV; 26Mg(p, γ), E=0.338 MeV; 27Al(p, γ), E=0.327 MeV; measured thick target γ-yield vs E. High resolution ion beams, energies around resonances.
doi: 10.1016/0168-9002(89)91292-8
1988BR17 Z.Phys. A330, 167 (1988) K.Brehm, H.W.Becker, C.Rolfs, H.P.Trautvetter, F.Kappeler, W.Ratynski The Cross Section of 14N(n, p)14C at Stellar Energies and Its Role as a Neutron Poison for S-Process Nucleosynthesis NUCLEAR REACTIONS 14N(n, p), E ≈ 25, 52.4 keV; measured σ(Ep), proton yield; deduced absolute <σ>, reaction rates, role in s-process nucleosynthesis. Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22078. 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. 1988SE09 Nucl.Instrum.Methods Phys.Res. A272, 814 (1988) S.Seuthe, H.W.Becker, C.Rolfs, S.Schmidt, H.P.Trautvetter, R.W.Kavanagh, F.B.Waanders Construction and Properties of a Gamma-Ray Detector Based on D(γ, n)H Neutron Counting NUCLEAR REACTIONS 27Al(p, γ), E ≈ 200-450 keV; 19F(p, αγ), E ≈ 750-1000 keV; measured γ yields. 28Si levels deduced resonance strength. Neutron counting based γ-detector. RADIOACTIVITY 60Co(β-); measured γ yields. 60Ni deduced hexadecapole transition strength. Neutron counting based γ-detector.
doi: 10.1016/0168-9002(88)90763-2
1988TI01 Nucl.Phys. A477, 105 (1988) R.Timmermann, H.W.Becker, C.Rolfs, U.Schroder, H.P.Trautvetter Search for Low-Energy Resonances in 27Al(p, α)24Mg NUCLEAR REACTIONS, ICPND 27Al(p, α), E=200-360 keV; measured σ(E(α)). 27Al(p, γ), E=200-360 keV; measured thick target γ-yields; deduced astrophysical reaction rates. 28Si deduced resonance strengths. Targets of low boron contamination.
doi: 10.1016/0375-9474(88)90363-6
1987BE17 Z.Phys. A327, 341 (1987) H.W.Becker, C.Rolfs, H.P.Trautvetter Low-Energy Cross Sections for 11B(p, 3α) NUCLEAR REACTIONS, ICPND 11B(p, 3α), E(cm)=22-1100 keV; measured Eα, Iα, σ(E, θ), σ(E, θ(α1), θ(α2)), α-yield vs Eα. 11B(p, α), E=140-1100 keV; measured α yield vs θ, σ(θ). 1H(11B, α), E=1.68-13.2 MeV; measured σ(E); deduced absolute σ, astrophysical S(E) factor. 12C deduced resonance, Γ. Solid, windowless gas targets, Si detectors, kinematically complete experiment. Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0413. 1987KR09 Nucl.Phys. A467, 273 (1987) A.Krauss, H.W.Becker, H.P.Trautvetter, C.Rolfs Astrophysical S(E) Factor of 3He(3He, 2p)4He at Solar Energies NUCLEAR REACTIONS, ICPND 3He(3He, 2p), E(cm)=17.9-342.5 keV; measured σ(E, θ); deduced reaction σ, astrophysical factor S(E). Windowless gas targets, beam calorimeter, cosmic background rejection, electronic shielding.
doi: 10.1016/0375-9474(87)90530-6
1987KR18 Nucl.Phys. A465, 150 (1987) A.Krauss, H.W.Becker, H.P.Trautvetter, C.Rolfs, K.Brand Low-Energy Fusion Cross Sections of D + D and D + 3He Reactions NUCLEAR REACTIONS, ICPND 2H(d, n), (d, p), E(cm)=2.98-162.5 keV; 3He(d, p), E(cm)=6.95-141.8 keV; measured σ(E, θ); deduced reaction σ, astrophysical S(E) factor. Windowless gas targets, beam calorimeter.
doi: 10.1016/0375-9474(87)90302-2
1987PL03 Nucl.Phys. A465, 291 (1987) R.Plaga, H.W.Becker, A.Redder, C.Rolfs, H.P.Trautvetter, K.Langanke The Scattering of Alpha Particles from 12C and the 12C(α, γ)16O Stellar Reaction Rate NUCLEAR REACTIONS, ICPND 12C(α, α0), E=1-66 MeV; measured σ(E, θ); deduced astrophysical S-factor vs E, capture σ. 16O deduced level parameters. Enriched 12C targets.
doi: 10.1016/0375-9474(87)90436-2
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
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
1987SC10 Nucl.Phys. A467, 240 (1987) U.Schroder, H.W.Becker, G.Bogaert, J.Gorres, C.Rolfs, H.P.Trautvetter, R.E.Azuma, C.Campbell, J.D.King, J.Vise Stellar Reaction Rate of 14N(p, γ)15O and Hydrogen Burning in Massive Stars NUCLEAR REACTIONS, ICPND 14N(p, γ), E=0.2-3.6 MeV; measured σ(E, E(γ), θ(γ)); deduced astrophysical S-factor, capture σ . 15O deduced levels, J, π, Γ, spectroscopic factors. Windowless gas, implanted 14N targets. Ge(Li) detectors.
doi: 10.1016/0375-9474(87)90528-8
1987SE13 Nucl.Instrum.Methods Phys.Res. A260, 33 (1987) S.Seuthe, H.W.Becker, A.Krauss, A.Redder, C.Rolfs, U.Schroder, H.P.Trautvetter, K.Wolke, S.Wustenbecker, R.W.Kavanagh, F.B.Waanders Production and Properties of Implanted Targets NUCLEAR REACTIONS, ICPND 12C(p, γ), E=220-340 keV; 12C(α, γ), E=2.65-2.85 MeV; 14N(p, γ), E=260-360 keV; 20Ne(p, γ), E=1165-1185 keV; 23Na(p, γ), E=300-400 keV; measured γ-ray yields. Implanted targets.
doi: 10.1016/0168-9002(87)90385-8
1987WU04 Nucl.Instrum.Methods Phys.Res. A256, 9 (1987) S.Wustenbecker, H.W.Becker, C.Rolfs, H.P.Trautvetter, K.Brand, G.E.Mitchell, J.S.Schweitzer Technical Developments for Ion Beams with High Energy Resolution NUCLEAR REACTIONS 27Al(p, γ), E ≈ 992 keV; 20Ne, 18O(p, γ), E ≈ 1167 keV; measured γ-yields; deduced beam energy stability, oscillator frequency dependences.
doi: 10.1016/0168-9002(87)91034-5
1986TR02 Z.Phys. A323, 1 (1986) H.P.Trautvetter, H.W.Becker, U.Heinemann, L.Buchmann, C.Rolfs, F.Kappeler, M.Baumann, H.Freiesleben, H.-J.Lutke-Stetzkamp, P.Geltenbort, F.Gonnenwein Destruction of 26Al in Explosive Nucleosynthesis NUCLEAR REACTIONS 7Li(p, n), E=1.911, 2.105 MeV; 3H(p, n), E=1.125 MeV; measured En, σ(φn); 6Li(n, α), 26Al(n, p), E=40 meV-0.31 MeV; measured Ep, Ip, Iα, Ip(E); deduced astrophysical reaction rate. Artificially produced 26Al, natural Li, enriched 3H targets, surface barrier detectors. Data from this article have been entered in the EXFOR database. For more information, access X4 dataset22712. 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
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