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NSR database version of May 24, 2024.

Search: Author = S.Zavatarelli

Found 30 matches.

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2023BA34      Phys.Rev. D 108, 102005 (2023)

D.Basilico, G.Bellini, J.Benziger, R.Biondi, B.Caccianiga, F.Calaprice, A.Caminata, A.Chepurnov, D.D'Angelo, A.Derbin, A.Di Giacinto, V.Di Marcello, X.F.Ding, A.Di Ludovico, L.Di Noto, I.Drachnev, D.Franco, C.Galbiati, C.Ghiano, M.Giammarchi, A.Goretti, M.Gromov, D.Guffanti, A.Ianni, A.Ianni, A.Jany, V.Kobychev, G.Korga, S.Kumaran, M.Laubenstein, E.Litvinovich, P.Lombardi, I.Lomskaya, L.Ludhova, I.Machulin, J.Martyn, E.Meroni, L.Miramonti, M.Misiaszek, V.Muratova, R.Nugmanov, L.Oberauer, V.Orekhov, F.Ortica, M.Pallavicini, L.Pelicci, O.Penek, L.Pietrofaccia, N.Pilipenko, A.Pocar, G.Raikov, M.T.Ranalli, G.Ranucci, A.Razeto, A.Re, N.Rossi, S.Schonert, D.Semenov, G.Settanta, M.Skorokhvatov, A.Singhal, O.Smirnov, A.Sotnikov, R.Tartaglia, G.Testera, E.Unzhakov, F.L.Villante, A.Vishneva, R.B.Vogelaar, F.von Feilitzsch, M.Wojcik, M.Wurm, S.Zavatarelli, K.Zuber, G.Zuzel, for the Borexino Collaboration

Final results of Borexino on CNO solar neutrinos

doi: 10.1103/PhysRevD.108.102005
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the XUNDL database. For more information, click here.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2457. Data from this article have been entered in the XUNDL database. For more information, click here.


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2520. Data from this article have been entered in the XUNDL database. For more information, click here.


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1458.


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1195.


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO1073.


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0228.


2001GA40      Nucl.Phys. A688, 530c (2001)

D.Galli, P.G.Prada Moroni, S.Zavatarelli, F.Ferrini, F.Palla

Astrophysical Implications of the New Measurements of the 3He(3He, 2p)4He Cross Section

NUCLEAR REACTIONS 3He(3He, 2p), E=low; compiled, surveyed σ data, star abundance data, 3He abundance discussed.

doi: 10.1016/S0375-9474(01)00778-3
Citations: PlumX Metrics


2001PR12      Nucl.Phys. A688, 572c (2001)

P.G.Prada Moroni, S.Zavatarelli

The Effects on Stellar Evolution of a Low Energy Resonance in the 3He + 3He Reaction

NUCLEAR REACTIONS 3He(3He, 2p), E=low; surveyed σ data, calculated σ assuming hypothetical low-energy resonances, effects on solar neutrino flux and on 3He galactic abundance discussed.

doi: 10.1016/S0375-9474(01)00791-6
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0414.


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0228.


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0342.


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
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


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0379.


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


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
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
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetA0110.


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
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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
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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
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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
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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
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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
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