NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = C.Gustavino Found 62 matches. 2023SK01 J.Phys.(London) G50, 045201 (2023) J.Skowronski, R.M.Gesue, A.Boeltzig, G.F.Ciani, D.Piatti, D.Rapagnani, M.Aliotta, C.Ananna, F.Barile, D.Bemmerer, A.Best, C.Broggini, C.G.Bruno, A.Caciolli, M.Campostrini, F.Cavanna, P.Colombetti, A.Compagnucci, P.Corvisiero, L.Csedreki, T.Davinson, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, A.Formicola, Z.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, G.Gyurky, G.Imbriani, M.Junker, M.Lugaro, P.Marigo, E.Masha, R.Menegazzo, V.Paticchio, R.Perrino, P.Prati, V.Rigato, L.Schiavulli, R.S.Sidhu, O.Straniero, T.Szucs, S.Zavatarelli Advances in radiative capture studies at LUNA with a segmented BGO detector NUCLEAR REACTIONS 12,13C, 14N, 17O, 25Mg(p, γ), 13C(α, n), E ∼ 200 keV; measured reaction products, Eγ, Iγ; deduced yields, resonance parameters, a high-efficiency detection of shorter-lived nuclides. A BGO summing detector at LUNA.
doi: 10.1088/1361-6471/acb961
2022PI05 Eur.Phys.J. A 58, 194 (2022) D.Piatti, E.Masha, M.Aliotta, J.Balibrea-Correa, F.Barile, D.Bemmerer, A.Best, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, F.Cavanna, T.Chillery, G.F.Ciani, A.Compagnucci, P.Corvisiero, L.Csedreki, T.Davinson, R.Depalo, A.di Leva, Z.Elekes, F.Ferraro, E.M.Fiore, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, M.Lugaro, P.Marigo, R.Menegazzo, V.Mossa, F.R.Pantaleo, V.Paticchio, R.Perrino, P.Prati, D.Rapagnani, L.Schiavulli, J.Skowronski, K.Stockel, O.Straniero, T.Szucs, M.P.Takacs, S.Zavatarelli First direct limit on the 334 keV resonance strength in 22Ne(α, γ)26Mg reaction NUCLEAR REACTIONS 22Ne(α, γ), E(cm)=334 keV; measured reaction products, Eγ, Iγ; deduced probability density functions of the resonance strength, resonances. Comparison with available data. The Laboratory for Underground Nuclear Astrophysics (LUNA) 400 kV accelerator, located in the deep underground INFN Laboratori Nazionali del Gran Sasso.
doi: 10.1140/epja/s10050-022-00827-2
2022VI01 Phys.Rev. C 105, 014001 (2022) M.Viviani, E.Filandri, L.Girlanda, C.Gustavino, A.Kievsky, L.E.Marcucci, R.Schiavilla X17 boson and the3H(p, e+e-)4He and 3He(n, e+e-4He processes: A theoretical analysis NUCLEAR REACTIONS 3H(p, γ)4He, E(cm)<0.85 MeV; 3He(n, γ)4He, E(cm)<2 MeV; calculated astrophysical S factor, total σ(E) using Δ-less (N3LO500/N2LO500) and Δ-full (NVIa/3NIa) χEFT formalism, and compared with experimental data. 3H(p, e-e+)4He, E=0.90 MeV; calculated five-fold differential σ(E, θ) as function of the electron energy using N3LO500/N2LO500 interactions in the ATOMKI setup. 3H(p, e-e+)4He, E=0.40, 0.90 MeV; 3He(n, e-e+)4He, E=0.17, 0.35, 0.70, 2.0 MeV; calculated four-fold differential σ(E, θ) based on the N3LO500/N2LO500 interactions, including results obtained from the exchange of a scalar, pseudoscalar, vector, and axial X17 boson, and compared with differential σ data for 3H(p, e-e+)4He, E=0.51, 0.61.0.90 MeV reaction from ATOMKI (reported by 2021Kr08: Phys. Rev. C 104, 044003). 3H(p, p)(p, p'), E=0.9 MeV; calculated reduced matrix elements (RMEs) for channels with J≤2, dependences on the three-momentum transfer and proton incident energy of electromagnetic RMEs using N3LO500/N2LO500 or NVIa/3NIa chiral interactions. 3He(n, e-e+)4He, 3He(n, γ)4He, E=0.17, 0.35, 0.70, 1.00, 2.00, 3.50 MeV; calculated total σ(E) using the N3LO500/N2LO500 and NVIa/3NIa Hamiltonians; deduced X17 coupling constants from the fit of the 2019 ATOMKI angular distribution data for 3H(p, e+e-)4He, E=0.90 MeV. Relevance to possible future experiments probing e+ - e- pair production in a four-nucleon system such as 4He at a number of candidate facilities.
doi: 10.1103/PhysRevC.105.014001
2021CS01 Nucl.Instrum.Methods Phys.Res. A994, 165081 (2021) L.Csedreki, G.F.Ciani, J.Balibrea-Correa, A.Best, M.Aliotta, F.Barile, D.Bemmerer, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, F.Cavanna, T.Chillery, P.Colombetti, P.Corvisiero, T.Davinson, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, E.M.Fiore, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, Z.Janas, M.Junker, I.Kochanek, M.Lugaro, P.Marigo, E.Masha, C.Mazzocchi, R.Menegazzo, V.Mossa, F.R.Pantaleo, V.Paticchio, R.Perrino, D.Piatti, P.Prati, L.Schiavulli, K.Stockel, O.Straniero, T.Szucs, M.P.Takacs, F.Terrasi, S.Zavatarelli Characterization of the LUNA neutron detector array for the measurement of the 13C(α, n)16O reaction NUCLEAR REACTIONS 13C(α, n), E=300-400 keV; 51V(p, n), E=5 MeV; measured reaction products, En, In, Eγ, Iγ; deduced yields, neutron efficiencies, possiblity to measure the σ approaching its s-process Gamow peak. Comparison with Geant4 simulations.
doi: 10.1016/j.nima.2021.165081
2020CI06 Eur.Phys.J. A 56, 75 (2020) G.F.Ciani, L.Csedreki, J.Balibrea-Correa, A.Best, M.Aliotta, F.Barile, D.Bemmerer, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, F.Cavanna, T.Chillery, P.Colombetti, P.Corvisiero, T.Davinson, R.Depalo, A.Di Leva, L.Di Paolo, Z.Elekes, F.Ferraro, E.M.Fiore, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, I.Kochanek, M.Lugaro, P.Marigo, E.Masha, R.Menegazzo, V.Mossa, F.R.Pantaleo, V.Paticchio, R.Perrino, D.Piatti, P.Prati, L.Schiavulli, K.Stockel, O.Straniero, T.Szucs, M.P.Takacs, F.Terrasi, D.Trezzi, S.Zavatarelli A new approach to monitor 13C-targets degradation in situ for 13C(α, n)16O cross-section measurements at LUNA
doi: 10.1140/epja/s10050-020-00077-0
2019BE31 Phys.Lett. B 797, 134900 (2019) A.Best, F.R.Pantaleo, A.Boeltzig, G.Imbriani, M.Aliotta, J.Balibrea-Correa, D.Bemmerer, C.Broggini, C.G.Bruno, R.Buompane, A.Caciolli, F.Cavanna, T.Chillery, G.F.Ciani, P.Corvisiero, L.Csedreki, T.Davinson, R.J.deBoer, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, E.M.Fiore, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, M.Junker, I.Kochanek, M.Lugaro, P.Marigo, R.Menegazzo, V.Mossa, V.Paticchio, R.Perrino, D.Piatti, P.Prati, L.Schiavulli, K.Stockel, O.Straniero, F.Strieder, T.Szucs, M.P.Takacs, D.Trezzi, M.Wiescher, S.Zavatarelli Cross section of the reaction 18O(p, γ)19F at astrophysical energies: The 90 keV resonance and the direct capture component NUCLEAR REACTIONS 18O(p, γ), E<1 MeV; measured reaction products, Eγ, Iγ; deduced γ-ray energies, resonance parameters, σ. Comparison with available data.
doi: 10.1016/j.physletb.2019.134900
2019BO09 Phys.Lett. B 795, 122 (2019) A.Boeltzig, A.Best, F.R.Pantaleo, G.Imbriani, M.Junker, M.Aliotta, J.Balibrea-Correa, D.Bemmerer, C.Broggini, C.G.Bruno, R.Buompane, A.Caciolli, F.Cavanna, T.Chillery, G.F.Ciani, P.Corvisiero, L.Csedreki, T.Davinson, R.J.deBoer, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, E.M.Fiore, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, I.Kochanek, M.Lugaro, P.Marigo, R.Menegazzo, V.Mossa, F.Munnik, V.Paticchio, R.Perrino, D.Piatti, P.Prati, L.Schiavulli, K.Stockel, O.Straniero, F.Strieder, T.Szucs, M.P.Takacs, D.Trezzi, M.Wiescher, S.Zavatarelli Direct measurements of low-energy resonance strengths of the 23Na(p, γ)24Mg reaction for astrophysics NUCLEAR REACTIONS 23Na(p, γ), E<1 MeV; measured reaction products, Eγ, Iγ; deduced resonance parameters, strengths, astrophysical reaction rates. Comparison with available data.
doi: 10.1016/j.physletb.2019.05.044
2019BR07 Phys.Lett. B 790, 237 (2019) C.G.Bruno, M.Aliotta, P.Descouvemont, A.Best, T.Davinson, D.Bemmerer, A.Boeltzig, C.Broggini, A.Caciolli, F.Cavanna, T.Chillery, G.F.Ciani, P.Corvisiero, R.Depalo, A.Di Leva, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, M.Lugaro, P.Marigo, R.Menegazzo, V.Mossa, F.R.Pantaleo, D.Piatti, P.Prati, K.Stockel, O.Straniero, F.Strieder, T.Szucs, M.P.Takacs, D.Trezzi Improved astrophysical rate for the 18O(p, α)15N reaction by underground measurements NUCLEAR REACTIONS 18O(p, α)15N, E=60-360 keV; measured reaction products, Ep, Ip, Eα, Iα; deduced differential yield, resonance energies, S-factor, J, π, reaction rates.
doi: 10.1016/j.physletb.2019.01.017
2018BE17 Europhys.Lett. 122, 52001 (2018) D.Bemmerer, F.Cavanna, R.Depalo, M.Aliotta, M.Anders, A.Boeltzig, C.Broggini, C.Bruno, A.Caciolli, T.Chillery, P.Corvisiero, T.Davinson, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, R.Menegazzo, V.Mossa, F.R.Pantaleo, P.Prati, D.A.Scott, K.Stocker, O.Straniero, T.Szucs, M.P.Takacs, D.Trezzi Effect of beam energy straggling on resonant yield in thin gas targets: The cases 22Ne(p, γ)23Na and 14N(p, γ)15O NUCLEAR REACTIONS 22Ne, 14N(p, γ), E<300 keV; analyzed available data; deduced correction for narrow resonance yields.
doi: 10.1209/0295-5075/122/52001
2017TR01 Astropart.Phys. 89, 57 (2017) D.Trezzi, M.Anders, M.Aliotta, A.Bellini, D.Bemmerer, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, F.Cavanna, P.Corvisiero, H.Costantini, T.Davinson, R.Depalo, Z.Elekes, M.Erhard, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, M.Junker, A.Lemut, M.Marta, C.Mazzocchi, R.Menegazzo, V.Mossa, F.Pantaleo, P.Prati, C.Rossi Alvarez, D.A.Scott, E.Somorjai, O.Straniero, T.Szucs, M.Takacs Big Bang 6Li nucleosynthesis studied deep underground (LUNA collaboration) NUCLEAR REACTIONS 2H(α, γ), E(cm)=80, 93, 120, 133 keV; measured reaction products, Eγ, Iγ; deduced σ, S-factor, thermonuclear reaction rates. Comparison with available data.
doi: 10.1016/j.astropartphys.2017.01.007
2016DE34 Phys.Rev. C 94, 055804 (2016) R.Depalo, F.Cavanna, M.Aliotta, M.Anders, D.Bemmerer, A.Best, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, G.F.Ciani, P.Corvisiero, T.Davinson, A.Di Leva, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, R.Menegazzo, V.Mossa, F.R.Pantaleo, D.Piatti, P.Prati, O.Straniero, T.Szucs, M.P.Takacs, D.Trezzi Direct measurement of low-energy 22Ne(p, γ)23Na resonances NUCLEAR REACTIONS 22Ne(p, γ), E=70-300 keV; measured Eγ, Iγ, γγ-coin at the LUNA 400 kV accelerator, deep underground at the Gran Sasso National Laboratories (LNGS). 23Na; deduced levels, resonance energies and strengths, J, π, thermonuclear reaction rates. Comparison with previous experimental data.
doi: 10.1103/PhysRevC.94.055804
2016GU07 Eur.Phys.J. A 52, 74 (2016) C.Gustavino, M.Anders, D.Bemmerer, Z.Elekes, D.Trezzi Primordial nucleosynthesis COMPILATION 2H(p, γ), E(cm)=1-1000 keV;3He(α, γ), E=0.01-2.5 MeV;2H(α, γ), E=0.025-3 MeV; compiled S-factors.
doi: 10.1140/epja/i2016-16074-5
2015BR09 Eur.Phys.J. A 51, 94 (2015) C.G.Bruno, D.A.Scott, A.Formicola, M.Aliotta, T.Davinson, M.Anders, A.Best, D.Bemmerer, C.Broggini, A.Caciolli, F.Cavanna, P.Corvisiero, R.Depalo, A.Di Leva, Z.Elekes, Zs.Fulop, G.Gervino, C.J.Griffin, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, R.Menegazzo, E.Napolitani, P.Prati, E.Somorjai, O.Straniero, F.Strieder, T.Szucs, D.Trezzi, for the LUNA Collaboration Resonance strengths in the 17, 18O(p, α)14, 15N reactions and background suppression underground - Commissioning of a new setup for charged-particle detection at LUNA NUCLEAR REACTIONS 17,18O(p, α), E=151, 193 keV; measured Eα, Iα; deduced resonance strength, energy, thick target yield as a by-product of commissioning of new setup.
doi: 10.1140/epja/i2015-15094-y
2015CA27 Phys.Rev.Lett. 115, 252501 (2015); Erratum Phys.Rev.Lett. 120, 239901 (2018) F.Cavanna, R.Depalo, M.Aliotta, M.Anders, D.Bemmerer, A.Best, A.Boeltzig, C.Broggini, C.G.Bruno, A.Caciolli, P.Corvisiero, T.Davinson, A.di Leva, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, R.Menegazzo, V.Mossa, F.R.Pantaleo, P.Prati, D.A.Scott, E.Somorjai, O.Straniero, F.Strieder, T.Szucs, M.P.Takacs, D.Trezzi, for the LUNA Collaboration Three New Low-Energy Resonances in the 22Ne(p, γ)23Na Reaction NUCLEAR REACTIONS 20,21,22Ne(p, γ), E=70-300 keV; measured reaction products, Eγ, Iγ; deduced resonance energies and strengths, thermonuclear reaction rates. Comparison with available data.
doi: 10.1103/PhysRevLett.115.252501
2014AN05 Phys.Rev.Lett. 113, 042501 (2014) M.Anders, D.Trezzi, R.Menegazzo, M.Aliotta, A.Bellini, D.Bemmerer, C.Broggini, A.Caciolli, P.Corvisiero, H.Costantini, T.Davinson, Z.Elekes, M.Erhard, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, M.Junker, A.Lemut, M.Marta, C.Mazzocchi, P.Prati, C.Rossi Alvarez, D.A.Scott, E.Somorjai, O.Straniero, T.Szucs, for the LUNA Collaboration First Direct Measurement of the 2H(α, γ)6Li Cross Section at Big Bang Energies and the Primordial Lithium Problem NUCLEAR REACTIONS 2H(α, γ), E=400 keV; measured reaction products, Eγ, Iγ; deduced S-factor, σ. Comparison with available data.
doi: 10.1103/PhysRevLett.113.042501
2014CA47 Eur.Phys.J. A 50, 179 (2014) F.Cavanna, R.Depalo, M.-L.Menzel, M.Aliotta, M.Anders, D.Bemmerer, C.Broggini, C.G.Bruno, A.Caciolli, P.Corvisiero, T.Davinson, A.di Leva, Z.Elekes, F.Ferraro, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, R.Menegazzo, P.Prati, C.Rossi Alvarez, D.A.Scott, E.Somorjai, O.Straniero, F.Strieder, T.Szucs, D.Trezzi, for the LUNA Collaboration A new study of the 22Ne(p, γ)23Na reaction deep underground: Feasibility, setup and first observation of the 186 keV resonance NUCLEAR REACTIONS 22Ne(p, γ), E=120-400 keV; measured Eγ, Iγ at LUNA. 23Na deduced γ transitions, 186 keV resonance.
doi: 10.1140/epja/i2014-14179-5
2014DI01 Phys.Rev. C 89, 015803 (2014), Erratum Phys.Rev. C 90, 019902 (2014) A.Di Leva, D.A.Scott, A.Caciolli, A.Formicola, F.Strieder, M.Aliotta, M.Anders, D.Bemmerer, C.Broggini, P.Corvisiero, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, J.Jose, M.Junker, M.Laubenstein, R.Menegazzo, E.Napolitani, P.Prati, V.Rigato, V.Roca, E.Somorjai, C.Salvo, O.Straniero, T.Szucs, F.Terrasi, D.Trezzi Underground study of the 17O(p, γ)18F reaction relevant for explosive hydrogen burning NUCLEAR REACTIONS 17O(p, γ)18F, E(cm)=160-370 keV; measured Eγ, Iγ, on- and off-resonance γ spectra, γ-branching ratios from decay of resonances, half-life using activation method at underground LUNA accelerator at Gran Sasso National Laboratory; deduced S factors for secondary transitions, total S factor, resonance strength, astrophysical S factor and reaction rates. 18F; deduced levels, analysis of astrophysically important 183-keV resonance. Comparison with previous experimental results. 15N, 18,19F, 18O; evaluated abundances by Nova model calculations. RADIOACTIVITY 18F(β+)[from 17O(p, γ), E(cm)=160-370 keV]; measured Eγ, Iγ, half-life.
doi: 10.1103/PhysRevC.89.015803
2014FO06 Nucl.Instrum.Methods Phys.Res. A742, 258 (2014) A.Formicola, C.G.Bruno, A.Caciolli, F.Cavanna, R.Depalo, A.Di Leva, D.A.Scott, D.Trezzi, M.Aliotta, M.Anders, D.Bemmerer, C.Broggini, P.Corvisiero, Z.Elekes, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, G.Imbriani, M.Junker, R.Menegazzo, P.Prati, E.Somorjai, O.Straniero, F.Strieder, T.Szucs Cross-section measurements at astrophysically relevant energies: The LUNA experiment NUCLEAR REACTIONS 17O(p, γ), E(cm)=183 keV; measured reaction products, Eγ, Iγ; deduced σ, resonance strength, S-factor. Comparison with available data.
doi: 10.1016/j.nima.2013.11.082
2013AN07 Eur.Phys.J. A 49, 28 (2013) M.Anders, D.Trezzi, A.Bellini, M.Aliotta, D.Bemmerer, C.Broggini, A.Caciolli, H.Costantini, P.Corvisiero, T.Davinson, Z.Elekes, M.Erhard, A.Formicola, Zs.Fulop, G.Gervino, A.Guglielmetti, C.Gustavino, Gy.Gyurky, M.Junker, A.Lemut, M.Marta, C.Mazzocchi, R.Menegazzo, P.Prati, C.Rossi Alvarez, D.Scott, E.Somorjai, O.Straniero, T.Szucs, LUNA Collaboration Neutron-induced background by an α-beam incident on a deuterium gas target and its implications for the study of the 2H(α, γ)6Li reaction at LUNA NUCLEAR REACTIONS 2H(α, γ), E=280, 400 keV; measured Eγ, Iγ; deduced yields vs Eγ, existence of cosmological 6Li plateau.
doi: 10.1140/epja/i2013-13028-5
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
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
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
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
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
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
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
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
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
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
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
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
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
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
1995AR31 Nucl.Instrum.Methods Phys.Res. A360, 607 (1995) C.Arpesella, E.Bellotti, C.Broggini, P.Corvisiero, A.Fubini, G.Gervino, U.Greife, C.Gustavino, M.Junker, A.Lanza, P.Prati, C.Rolfs, D.Zahnow, S.Zavatarelli A Monte Carlo Code for Nuclear Astrophysics Experiments NUCLEAR REACTIONS 3He(d, p), (3He, 2p), E=153 keV; 2H(d, X), 9Be(p, X), E not given; analyzed spectra. Monte Carlo code for astrophysical applications, ion energy, angular straggling, Doppler broadening effects accurately evaluated.
doi: 10.1016/0168-9002(95)00038-0
1994BE59 Nucl.Instrum.Methods Phys.Res. A345, 456 (1994) G.Bencivenni, M.D'Incecco, G.Felici, C.Gustavino, E.Iacuessa A Modular Design for Glass Spark Counters
doi: 10.1016/0168-9002(94)90499-5
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
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
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