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NSR database version of April 27, 2024.

Search: Author = A.Lanza

Found 2 matches.

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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
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