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NSR database version of April 29, 2024.

Search: Author = M.Galmarini

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1994CA29      Acta Phys.Pol. B25, 475 (1994)

M.Cavinato, E.Fabrici, E.Gadioli, E.Gadioli Erba, M.Galmarini, P.Vergani

Non Equilibrium Particle Emission in Nuclear Reactions

NUCLEAR REACTIONS ¹⁶⁵Ho(¹²C, X), E=25 MeV/nucleon; ⁴⁰Ca(⁴⁰Ar, X), E=20 MeV/nucleon; ¹⁰⁷Ag(¹⁶O, X), E=30 MeV/nucleon; ¹⁹⁷Au(³⁶Ar, X), E=35 MeV/nucleon; compiled, reviewed data, analyses; deduced new mechanism evidence. Boltzmann master equation approach.

1994CA49      Z.Phys. A347, 237 (1994)

M.Cavinato, E.Fabrici, E.Gadioli, E.Gadioli Erba, M.Galmarini, A.Gritti

Intermediate Mass Fragment Emission in Boltzmann Master Equation Theory of Pre-Equilibrium Reactions

NUCLEAR REACTIONS ¹⁹⁷Au(³⁶Ar, X), E=35 MeV/nucleon; calculated intermediate mass fragments angle integrated multiplicity spectra. ⁵⁴Fe(p, X), E=62 MeV; calculated light charged particle spectra. Ag(³²S, X), E=30 MeV/nucleon; calculated light particles multiplicity spectra. Coalescence model.

doi: 10.1007/BF01289790
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1993VE09      Phys.Rev. C48, 1815 (1993)

P.Vergani, E.Gadioli, E.Vaciago, E.Fabrici, E.Gadioli Erba, M.Galmarini, G.Ciavola, C.Marchetta

Complete and Incomplete Fusion and Emission of Preequilibrium Nucleons in the Interaction of ¹²C with ¹⁹⁷Au Below 10 MeV/nucleon

NUCLEAR REACTIONS, ICPND ¹⁹⁷Au(¹²C, X), E ≤ 10 MeV/nucleon; measured production σ(E) for ^{206,205,204,203}At, ^{203,202,205,204}Po, ^{203,202,201,200,199}Bi, ^201,200,199Pb, ^199,198m,198Tl. Complete, incomplete fusion, preequilibrium emission. Activation technique.

doi: 10.1103/PhysRevC.48.1815
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Data from this article have been entered in the EXFOR database. For more information, access X4 datasetO2447.

1992CE03      Phys.Rev. C45, 2369 (1992)

I.Cervesato, E.Fabrici, E.Gadioli, E.Gadioli-Erba, M.Galmarini

Light Particle Emission in Boltzmann Master Equation Theory of Pre-Equilibrium Reactions

NUCLEAR REACTIONS ¹⁰⁷Ag(³²S, X), E=960 MeV; calculated deuteron spectra; ¹⁰⁷Ag(¹⁶O, X), E=480 MeV; calculated proton, deuteron, triton, α-particles. ¹⁶⁵Ho(¹²C, xn), E=300 MeV; ¹⁶⁵Ho(²⁰Ne, xn), E=402-600 MeV; ⁴⁰Ca(⁴⁰Ar, xn), E=20 MeV/nucleon; ²⁰⁹Bi(p, xn), E=90 MeV; calculated neutron spectra. ⁶⁰Ni(n, xp), E=60 MeV; calculated proton spectra. ¹²⁰Sn, ⁵⁴Fe(p, X), E=62 MeV; calculated spectra of X=p, d, t, α, ³He; ⁵⁴Fe, ⁸⁹Y, ¹²⁰Sn, ¹⁹⁷Au(p, xα), E=62 MeV; calculated α spectra. Preequilibrium reactions, Boltzmann master equation.

doi: 10.1103/PhysRevC.45.2369
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1991FA02      Z.Phys. A338, 17 (1991)

E.Fabrici, E.Gadioli, E.Gadioli Erba, M.Galmarini

Fast Neutron Emission from Partial Fusion Heavy Ion Reactions

NUCLEAR REACTIONS Ni, ¹⁶⁵Ho(¹⁴N, X), E=35 MeV/nucleon; analyzed (nucleon)(fragment)-coin data; deduced reaction mechanism. Boltzmann master equation.

doi: 10.1007/BF01279112
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1991PA09      Phys.Rev. C44, 1528 (1991)

D.J.Parker, P.Vergani, E.Gadioli, J.J.Hogan, F.Vettore, E.Gadioli-Erba, E.Fabrici, M.Galmarini

Recoil Range Study of Complete and Incomplete Fusion of C and Au at 10 MeV/Nucleon

NUCLEAR REACTIONS ¹⁹⁷Au(¹²C, X), E=120 MeV; measured residue production σ, X=¹⁹⁶Au-²⁰⁴Po; deduced reaction mechanism. Monte Carlo calculations.

doi: 10.1103/PhysRevC.44.1528
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1990FA11      Phys.Rev. C42, 2163 (1990)

E.Fabrici, E.Gadioli, E.Gadioli Erba, M.Galmarini

Hard Photon Emission in Heavy-Ion Reactions

NUCLEAR REACTIONS ⁴⁰Ca(⁴⁰Ar, xn), E=20 MeV/nucleon; ¹⁶⁵Ho(C, xn), E=24 MeV/nucleon; ²⁰⁹Bi(p, xn), E=90 MeV; calculated neutron spectrum. C, Cu, Ag, ¹⁹⁷Au(p, X), E=72 MeV; ¹⁹⁷Au(p, X), E=168 MeV; Pb, C(n, X), E=20, 30, 40 MeV/nucleon; ¹²C(¹²C, X), E=48, 60, 74 MeV/nucleon; C(⁸⁶Kr, X), E=44 MeV/nucleon; ¹⁵⁸Gd(⁴⁰Ar, X), E=44 MeV/nucleon; ²³⁸U, ¹²C(¹²C, X), E=84 MeV/nucleon; Sn(¹³⁶Xe, X), E=89 MeV/nucleon; calculated γ-spectra, multiplicities. Single p-n bremsstrahlung process.

doi: 10.1103/PhysRevC.42.2163
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1989FA11      Phys.Rev. C40, 2548 (1989)

E.Fabrici, E.Gadioli, E.Gadioli Erba, M.Galmarini, F.Fabbri, G.Reffo

Importance of Nucleon-Nucleon Interactions in Hardening Nucleon Spectra in Heavy Ion Fusion

NUCLEAR REACTIONS ¹⁶⁵Ho(¹²C, xn), E=300 MeV; ¹⁶⁵Ho(²⁰Ne, xn), E=600, 402 MeV; calculated preequilibrium neutron multiplicity distributions. ⁴⁰Ca(⁴⁰Ar, xn), E=800 MeV; ²⁷Al, ⁵⁸Ni, ¹²⁰Sn, ¹⁹⁷Au(³²S, xp), E not given; calculated nucleon spectra; deduced nucleon-nucleon interaction role. Master equation approach.

doi: 10.1103/PhysRevC.40.2548
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