NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = A.Fubini Found 25 matches. 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
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
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
1992DE24 Z.Phys. A342, 291 (1992) P.P.Delsanto, A.Fubini, F.Murgia, P.Quarati Photofission of 209Bi, 232Th and 238U in the Quasi-Deuteron Energy Region NUCLEAR REACTIONS 209Bi, 238U, 232Th(γ, F), E ≈ 20-120 MeV; analyzed photon induced fission data. Quasideuteron model.
doi: 10.1007/BF01291512
1974FU10 Lett.Nuovo Cim. 9, 682 (1974) Competition between Neutron Emission and Fission for 234U, 236U, 240Pu And 242Pu Compound Nuclei NUCLEAR REACTIONS 233,235U, 239,241Pu(n, γ), (n, n'), (n, n'F), (n, 2n), (n, F), E=1-10 MeV; calculated n-width/F-width.
doi: 10.1007/BF02763391
1973FU17 Nuovo Cim. 18A, 711 (1973) A.Fubini, R.Alberini, D.Lattanzi 203Tl(n, γ) Reaction and Level Structure of 204Tl NUCLEAR REACTIONS 203Tl(n, γ), E=thermal; measured Eγ, Iγ, γγ-coin. 204Tl deduced levels, J, π.
doi: 10.1007/BF02727587
1972FU04 Lett.Nuovo Cim. 3, 401 (1972) A.Fubini, P.R.Oliva, D.Prosperi Analysis of E2 Radiation Widths for Highly Excited Nuclear Levels NUCLEAR STRUCTURE A=80, A=140, A=200; analyzed E2 radiative widths for highly excited states.
doi: 10.1007/BF02826051
1972FU06 Nuovo Cim. 8A, 748 (1972) A.Fubini, D.Prosperi, F.Terrasi, I.Vata 175Lu(n, γ) Reaction and Level Structure of 176Lu NUCLEAR REACTIONS 175Lu(n, γ), E=thermal; measured Eγ, Iγ; deduced Q. 176Lu deduced levels, γ-branching. Ge(Li) detector.
doi: 10.1007/BF02722766
1972FU10 Lett.Nuovo Cim. 4, 430 (1972) Correlation between (n, γ) and (d, p) Reaction on 139La NUCLEAR REACTIONS 139La(n, γ), E=thermal; measured Eγ, Iγ; analyzed neutron capture/ deuteron stripping correlations. 140La deduced transitions.
doi: 10.1007/BF02824426
1972FU12 Lett.Nuovo Cim. 4, 1003 (1972) Correlation between (n, γ) and (d, p) Reactions in 176Lu NUCLEAR REACTIONS 176Lu(n, γ), E=thermal; measured Eγ, Iγ; deduced Q. 176Lu(d, p); analyzed σ. 177Lu levels deduced configurations, capture-stripping correlations.
doi: 10.1007/BF02757123
1971FU06 Nuovo Cim. 2A, 109 (1971) A.Fubini, M.Popa, D.Prosperi, F.Terrasi Investigation of the Reaction 35Cl(n, γ)36Cl NUCLEAR REACTIONS 35Cl(n, γ), E=thermal; measured Eγ, Iγ, γγ-coin; deduced Q. 36Cl deduced levels, γ-branching.
doi: 10.1007/BF02723991
1971FU15 Lett.Nuovo Cim. 2, 992 (1971) Analysis of 204Tl Level Scheme NUCLEAR REACTIONS 203Tl(n, γ), E=thermal; measured Eγ, Iγ. 204Tl deduced levels. Ge(Li) detector.
doi: 10.1007/BF02785832
1970FU03 Lett.Nuovo Cimento 3, 785 (1970) A New Isomer of 128I NUCLEAR REACTIONS 127I(n, γ), E=thermal; measured γγ-coin, γγ-delay, Eγ. 128mI deduced J, π, levels, T1/2, γ-multipolarity.
doi: 10.1007/BF02753430
1970FU04 Nuovo Cimento 68A, 502 (1970) A.Fubini, N.Lo Iudice, D.Prosperi, E.Salusti A Number-Conserving Calculation of the Low-Energy Spectra of the Odd-Odd Tl Isotopes NUCLEAR STRUCTURE 196,198,200,202,204Tl; calculated levels. Number-conserving formalism.
doi: 10.1007/BF02758145
1969FU02 Nuovo Cimento Lett. 1, 467 (1969) A.Fubini, M.Giannini, D.Prosperi, V.Rado M1 Transitions Following the Slow-Neutron Capture in 115In NUCLEAR REACTIONS 115In(n, γ)116In, E= thermal; measured Eγ, Iγ; deduced Q. 116In deduced levels, γ-multipolarity. Ge(Li) detector.
doi: 10.1007/BF02752589
1968PA17 Proc.Intern.Symp.Nucl.Struct., Dubna, Intern.At.Energy Agency, Vienna, p.483 (1968) D.Paya, J.Blons, A.Fubini, A.Michaudon The Intermediate Structure Observed in the Fission Cross-Sections of 237Np and Possibly of 239Pu NUCLEAR REACTIONS 237Np(n, F), E=10-2000 eV; 239Pu(n, F), E=0.5-4 keV; measured σ(E); deduced intermediate structure in subthreshold fission. Data from this article have been entered in the EXFOR database. For more information, access X4 dataset20447. Back to query form |