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NSR database version of April 27, 2024.

Search: Author = C.Arpesella

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2008AR01      Phys.Lett. B 658, 101 (2008)

C.Arpesella, for the Borexino Collaboration

First real time detection of ⁷Be solar neutrinos by Borexino

RADIOACTIVITY ⁷Be(EC); measured solar neutrino spectrum with the Borexino detector and compared to solar models.

doi: 10.1016/j.physletb.2007.09.054
Citations: PlumX Metrics

1999AR02      Nucl.Phys. B(Proc.Supp.) S70, 249 (1999)

C.Arpesella, E.Bellotti, N.Ferrari, L.Zanotti

Looking for Double Beta Decay of ¹⁵⁰Nd to Excited States of ¹⁵⁰Sm by Gamma Ray Spectroscopy

RADIOACTIVITY ¹⁵⁰Nd(2β^-); measured Eγ, Iγ; deduced 2β decay T_1/2 lower limits.

doi: 10.1016/S0920-5632(98)00430-7
Citations: PlumX Metrics

1999BE81      Astropart.Phys. 10, 115 (1999)

P.Belli, R.Bernabei, A.Incicchitti, C.Arpesella, V.V.Kobychev, O.A.Ponkratenko, V.I.Tretyak, Yu.G.Zdesenko

New limits on 2β⁺ decay processes in ¹⁰⁶Cd

RADIOACTIVITY ¹⁰⁶Cd(2β⁺), (β⁺EC), (2EC); measured T_1/2 lower limits.

doi: 10.1016/S0927-6505(98)00034-6
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

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.

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
Citations: PlumX Metrics

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.

1996AR22      Nucl.Phys.(Proc.Suppl.) S48, 247 (1996)

C.Arpesella, E.Bellotti, E.Fiorini, L.Miramonti, P.P.Sverzellati

Search for Inclusive Double Beta Decay of ¹⁵⁰Nd to Excited States ¹⁵⁰Sm at Laboratori Nazionali del Gran Sasso

RADIOACTIVITY ¹⁵⁰Nd(2β); measured 2ν-accompanied 2β-decay T_1/2 lower limits to three final states. Deexcitation γ-spectra measured by hyper-pure Ge detectors.

doi: 10.1016/0920-5632(96)00252-6
Citations: PlumX Metrics

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

1996AR24      Appl.Radiat.Isot. 47, 991 (1996)

C.Arpesella

A Low Background Counting Facility at Laboratori Nazionali del Gran Sasso

doi: 10.1016/S0969-8043(96)00097-8
Citations: PlumX Metrics

1996AR26      Nucl.Instrum.Methods Phys.Res. A372, 415 (1996)

C.Arpesella, E.Bellotti, L.Miramonti, P.P.Sverzellati

Gamma Ray Activity of Neodymium Samples

RADIOACTIVITY ²³²Th(α); ^235,238U(α); ²³¹Pa(α); ²²⁸Ac(β^-), (α); ²²⁶Ra(α); ¹⁷⁶Lu(β^-); ¹³⁸La(β^-), (EC); ¹³⁷Cs(β^-); ⁶⁰Co(β^-); ⁴⁰K(β^-), (β⁺), (EC); measured activity, three samples; deduced contamination related features. Natural Nd samples also included.

doi: 10.1016/0168-9002(95)00850-0
Citations: PlumX Metrics

1996AR35      Astropart.Phys. 4, 333 (1996)

C.Arpesella, C.Broggini, C.Cattadori

A Possible Gas for Solar Neutrino Spectroscopy

doi: 10.1016/0927-6505(95)00051-8
Citations: PlumX Metrics

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
Citations: PlumX Metrics

1994AR29      Europhys.Lett. 27, 29 (1994)

C.Arpesella, A.S.Barabash, E.Bellotti, C.Brofferio, E.Fiorini, P.P.Sverzellati, V.I.Umatov

Search for ββ Decay of ⁹⁶Zr and ¹⁵⁰Nd to Excited States of ⁹⁶Mo and ¹⁵⁰Sm

RADIOACTIVITY ⁹⁶Zr, ¹⁵⁰Nd(2β); ⁹⁶Zr(β^-); measured T_1/2 lower limits. Ge γ-detector.

doi: 10.1209/0295-5075/27/1/006
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.