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NSR database version of April 25, 2024.

Search: Author = G.Fiorentini

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2013FI07      Phys.Rev.Lett. 111, 022502 (2013)

G.A.Fiorentini, for the MINERvA Collaboration

Measurement of Muon Neutrino Quasielastic Scattering on a Hydrocarbon Target at E_ν ∼ 3.5 GeV

doi: 10.1103/PhysRevLett.111.022502
Citations: PlumX Metrics

2010FI04      Phys.Rev. C 81, 034602 (2010)

G.Fiorentini, A.Ianni, G.Korga, M.Lissia, F.Mantovani, L.Miramonti, L.Oberauer, M.Obolensky, O.Smirnov, Y.Suvorov

Nuclear physics for geo-neutrino studies

RADIOACTIVITY ²¹⁴Bi(β^-); analyzed data from Counting Test Facility (CTF) data from Gran Sasso Laboratory for geo-neutrino specific signals; proposed detector design for direct measurement of the energy distribution of antineutrinos from decays of long-lived radioactive isotopes. Monte Carlo simulation. Electron-Gamma (EG) computer code.

doi: 10.1103/PhysRevC.81.034602
Citations: PlumX Metrics

2004DE20      Phys.Lett. B 590, 13 (2004)

S.Degl'Innocenti, G.Fiorentini, B.Ricci, F.L.Villante

The ¹⁴N(p, γ)¹⁵O reaction, solar neutrinos and the age of the globular clusters

NUCLEAR REACTIONS ¹⁴N(p, γ), E=low; analyzed astrophysical S-factor. Implications for solar models and globular cluster dating discussed.

doi: 10.1016/j.physletb.2004.04.003
Citations: PlumX Metrics

2004FI06      Prog.Theor.Phys.(Kyoto), Suppl. 154, 309 (2004)

G.Fiorentini, B.Ricci, F.L.Villante

Nuclear Fusion in the Sun

doi: 10.1143/PTPS.154.309
Citations: PlumX Metrics

2004RA05      Eur.Phys.J. A 19, 283 (2004)

F.Raiola, L.Gang, C.Bonomo, G.Gyurky, M.Aliotta, H.W.Becker, R.Bonetti, C.Broggini, P.Corvisiero, A.D'Onofrio, Z.Fulop, G.Gervino, L.Gialanella, M.Junker, P.Prati, V.Roca, C.Rolfs, M.Romano, E.Somorjai, F.Strieder, F.Terrasi, G.Fiorentini, K.Langanke, J.Winter

Enhanced electron screening in d(d, p)t for deuterated metals

NUCLEAR REACTIONS ²H(d, p), E=low; measured yields in deuterated metals; deduced electron screening effect, astrophysical S-factors.

doi: 10.1140/epja/i2003-10125-0
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1220.

2003BO29      Nucl.Phys. A719, 37c (2003)

C.Bonomo, G.Fiorentini, Z.Fulop, L.Gang, G.Gyurky, K.Langanke, F.Raiola, C.Rolfs, E.Somorjai, F.Strieder, J.Winter, M.Aliotta

Enhanced electron screening in d(d, p)t for deuterated metals: a possible classical explanation

NUCLEAR REACTIONS ²H(d, p), E not given; analyzed yields in several deuterated materials; deduced electron screening effect.

doi: 10.1016/S0375-9474(03)00955-2
Citations: PlumX Metrics

2003FI01      Phys.Rev. C 67, 014603 (2003)

G.Fiorentini, C.Rolfs, F.L.Villante, B.Ricci

Fusion rate enhancement due to energy spread of colliding nuclei

NUCLEAR REACTIONS ²H(d, X), E=low; calculated fusion rate enhancement due to energy spread of colliding nuclei.

doi: 10.1103/PhysRevC.67.014603
Citations: PlumX Metrics

2001FI07      Phys.Lett. 503B, 121 (2001)

G.Fiorentini, B.Ricci, F.L.Villante

Helioseismology and Screening of Nuclear Reactions in the Sun

NUCLEAR REACTIONS ¹H, ⁷Be(p, X), ^3,4He(³He, X), E not given; analyzed reaction screening models, consistency with helioseismic data.

doi: 10.1016/S0370-2693(01)00221-0
Citations: PlumX Metrics

1999AN35      Nucl.Phys. A656, 3 (1999)

C.Angulo, M.Arnould, M.Rayet, P.Descouvemont, D.Baye, C.Leclercq-Willain, A.Coc, S.Barhoumi, P.Aguer, C.Rolfs, R.Kunz, J.W.Hammer, A.Mayer, T.Paradellis, S.Kossionides, C.Chronidou, K.Spyrou, S.Degl'Innocenti, G.Fiorentini, B.Ricci, S.Zavatarelli, C.Providencia, H.Wolters, J.Soares, C.Grama, J.Rahighi, A.Shotter, M.Lamehi-Rachti

A Compilation of Charged-Particle Induced Thermonuclear Reaction Rates

COMPILATION ¹H(p, e⁺ν), ²H, ^6,7Li, ^7,9Be, ^10,11B, ^12,13C, ^13,14,15N, ^16,17,18O, ¹⁹F, ^20,21,22Ne, ^22,23Na, ^24,25,26Mg, ^26,27Al, ²⁸Si(p, γ), ²H(d, γ), (d, p), ^2,3H(d, n), ^2,3H, ³He, ⁷Li, ⁷Be, ¹²C, ^14,15N, ^16,18O, ^20,22Ne(α, γ), ³He(³He, 2p), ^6,7Li, ⁹Be, ^10,11B, ^14,15N, ^17,18O, ¹⁹F, ²⁰Ne, ²³Na, ²⁴Mg, ²⁷Al(p, α), ⁷Li, ⁹Be, ¹³C, ¹⁴N, ^17,18O, ^21,22Ne, ²³Na, ^25,26Mg, ²⁷Al(α, n), ⁹Be, ¹¹B, ¹³C, ^14,15N, ¹⁹F, ²³Na(p, n), ⁹Be(p, d), E < 10 MeV; compiled, analyzed σ, S-factors; calculated astrophysical reaction rates vs T₉. Analytical approximations.

doi: 10.1016/S0375-9474(99)00030-5
Citations: PlumX Metrics

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

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

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

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

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

1998DE02      Phys.Lett. 416B, 365 (1998)

S.Degl'Innocenti, G.Fiorentini, B.Ricci

Helioseismology and p + p → d + e⁺ + ν(e) in the Sun

NUCLEAR REACTIONS ¹H(p, e⁺), E not given; analyzed helioseismic data; deduced astrophysical S-factor limits with respect to standard solar model.

doi: 10.1016/S0370-2693(97)01197-0
Citations: PlumX Metrics

1998FI02      Phys.Rev. D58, 063506 (1998)

G.Fiorentini, E.Lisi, S.Sarkar, F.L.Villante

Quantifying Uncertainies in Primordial Nucleosynthesis without Monte Carlo Simulations

NUCLEAR REACTIONS ¹H(n, γ), ²H(p, γ), (d, n), (d, p), ³H(d, n), (α, γ), ³He(n, p), (d, p), (α, γ), ⁷Li(p, α), ⁷Be(n, p), E not given; analyzed reaction rate uncertanties; deduced uncertainties in elemental abundances from primordial nucleosynthesis. Monte Carlo calculations.

doi: 10.1103/PhysRevD.58.063506
Citations: PlumX Metrics

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

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

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

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

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

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

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

Further Direct Approaches to the Nuclear Reactions in the Sun

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

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

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

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

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

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

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
Citations: PlumX Metrics

1996BE10      Phys.Lett. 365B, 185 (1996)

V.Berezinsky, G.Fiorentini, M.Lissia

LAST HOPE for an Astrophysical Solution to the Solar Neutrino Problem

doi: 10.1016/0370-2693(95)01241-9
Citations: PlumX Metrics

1996CA17      Z.Phys. A354, 237 (1996)

V.Castellani, G.Fiorentini, B.Ricci, O.Straniero

The Fate of Li and Be in Stars and the Laboratory

NUCLEAR REACTIONS ^6,7Li, ⁹Be(p, X), E not given; calculated reactivity N(A)<σv> vs temperature, other aspects; deduced Li, Be fate in stars and reproducibility in laboratory related futures.

doi: 10.1007/s002180050040
Citations: PlumX Metrics

1996CA47      Nucl.Phys. B(Proc.Suppl.) S48, 343 (1996)

E.Calabresu, G.Fiorentini, M.Lissia, B.Ricci

Intermediate Energy Solar Neutrinos

doi: 10.1016/0920-5632(96)00270-8
Citations: PlumX Metrics

1996FE04      Phys.Lett. 387B, 427 (1996)

N.Ferrari, G.Fiorentini, B.Ricci

The ⁵¹Cr Neutrino Source and Borexino: A desirable marriage

doi: 10.1016/0370-2693(96)01023-4
Citations: PlumX Metrics

1995FI02      Z.Phys. A350, 289 (1995)

G.Fiorentini, R.W.Kavanagh, C.Rolfs

Prospects for Underground Accelerator Research

NUCLEAR REACTIONS, ICPND ³He(d, p), E ≤ 40 keV; compiled, reviewed astrophysical S-factor data, analyses. ¹²C(α, γ), E(cm) ≤ 3 MeV; compiled, reviewed capture σ(E) data, analyses. ²¹Ne(p, γ), E ≈ resonance; compiled, reviewed γ yield data, analyses; ³He(³He, 2p), E ≤ 350 keV; compiled, reviewed σ(E), astrophysical S-factor data, analyses. Underground accelerator research prospects discussed.

doi: 10.1007/BF01291186
Citations: PlumX Metrics

1995RI07      Phys.Rev. C52, 1095 (1995)

B.Ricci, S.Degl'Innocenti, G.Fiorentini

Screening of Nuclear Reactions in the Sun and Solar Neutrinos

NUCLEAR REACTIONS ⁹Be, ¹H(p, X), E=solar; ⁴He(α, X), E=solar; calculated solar neutrino production associated enhancement factor vs solar profile. Different screening models.

doi: 10.1103/PhysRevC.52.1095
Citations: PlumX Metrics

1994CA19      Phys.Lett. 324B, 425 (1994)

V.Castellani, S.Degl'Innocenti, G.Fiorentini, M.Lissia, B.Ricci

Future Solar Neutrino Spectroscopy and Neutrino Properties

doi: 10.1016/0370-2693(94)90217-8
Citations: PlumX Metrics

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

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

Laboratory for Underground Nuclear Astrophysics (LUNA)

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

doi: 10.1016/0168-9002(94)91182-7
Citations: PlumX Metrics

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
Citations: PlumX Metrics
Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0627.

1992CI06      Phys.Lett. 297B, 197 (1992)

R.Cimiraglia, G.Fiorentini, B.Ricci

Molecular Trapping of Nuclei Produced in Neutrino Capture Reactions

NUCLEAR REACTIONS ⁷¹Ga(ν, e^-), E=solar; calculated fraction of ⁷¹Ge nuclei trapped in molecular GaGe.

doi: 10.1016/0370-2693(92)91092-N
Citations: PlumX Metrics

1990BR12      Nucl.Phys. A513, 316 (1990)

L.Bracci, G.Fiorentini, V.S.Melezhik, G.Mezzorani, P.Quarati

Atomic Effects in the Determination of Nuclear Cross Sections of Astrophysical Interest

NUCLEAR STRUCTURE ⁷Li, ⁷Be, ¹¹B, ¹²C, ¹⁴N, ¹⁶O; calculated proton induced reaction atomic correction factor.

ATOMIC PHYSICS ⁷Li, ⁷Be, ¹¹B, ¹²C, ¹⁴N, ¹⁶O; calculated proton induced reaction atomic correction factor.

doi: 10.1016/0375-9474(90)90101-Q
Citations: PlumX Metrics

1990BR34      J.Phys.(London) G16, 83 (1990)

L.Bracci, G.Fiorentini, G.Mezzorani

Nuclear Fusion in Molecular Systems

doi: 10.1088/0954-3899/16/1/012
Citations: PlumX Metrics

1984BR16      Nucl.Phys. A423, 429 (1984)

L.Bracci, G.Fiorentini

The Muon Attachment Probability after Prompt Fission

NUCLEAR REACTIONS ²³⁸U(μ^-, F), E at rest; calculated fission fragment muon attachment probability; deduced fragment mass dependence.

doi: 10.1016/0375-9474(84)90034-4
Citations: PlumX Metrics

1983BO30      Phys.Lett. 132B, 39 (1983)

P.Boi, L.Bracci, G.Fiorentini, P.Quarati

On the Significance of Muon Distribution between the Fission Fragments

NUCLEAR REACTIONS ²³⁸U(μ^-, F), E at rest; calculated muon attachment probability to fission fragments; deduced fragment final kinetic energy, mass asymmetry dependence.

doi: 10.1016/0370-2693(83)90217-4
Citations: PlumX Metrics

Note: The following list of authors and aliases matches the search parameter G.Fiorentini: , G.A.FIORENTINI