References of "Mancusi, Davide"
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See detailInfluence of nuclear de-excitation on observables relevant for space exploration
Mancusi, Davide ULg; Boudard, Alain; Cugnon, Joseph ULg et al

in Advances in Space Research (2011), 47(7), 1194-1199

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See detailINCL4.5 and Abla07 - Improved versions of the intranuclear cascade (INCL4) and deexcitation (Abla) models
David, Jean-Christophe; Boudard, A; Cugnon, Joseph ULg et al

in Proceedings of the meeting “Shielding Aspects of Accelerators, Targets and Irradiation Facilities - SATIF10”, CERN, June 2010, (2011)

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See detailThe extension of the INCL model for simulation of shielding in space
Pedoux, Sophie ULg; Cugnon, Joseph ULg; Mancusi, Davide ULg et al

in Advances in Space Research (2011), 48(2), 383-389

Radiation hazard for space missions is mainly due to cosmic ray protons, helium nuclei and light ions, whose energy spectrum is maximum around 1 GeV per nucleon but remains non-negligible for energies up ... [more ▼]

Radiation hazard for space missions is mainly due to cosmic ray protons, helium nuclei and light ions, whose energy spectrum is maximum around 1 GeV per nucleon but remains non-negligible for energies up to 15 GeV per nucleon. Nuclear reactions induced by high energy protons are often described by intranuclear cascade plus evaporation models. The attention is focused here on the Liège Intranuclear Cascade model (INCL), which has been shown to reproduce fairly well a great deal of experimental data for nucleon-induced reactions in the 200 MeV to 2 GeV range, when coupled with the ABLA evaporation-fission code. In order to extend the model to other conditions relevant for space radiation, three improvements of INCL are under development. They are reported on here. First, the reaction model has been extended to nucleon-nucleus reactions at incident energies up to 15 GeV, mainly by the inclusion of additional pion production channels in nucleon-nucleon collisions during the cascade. Second, a coalescence mechanism for the emission of light charged particles has been implemented recently. Finally, the model has been modified in order to accommodate light ions as projectiles. First results are shown and compared with illustrative experimental data. Implications for issues concerning radiation protection in space are discussed. [less ▲]

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See detailPHITS simulations of the Matroshka experiment
Gustafsson, K.; Sihver, L.; Mancusi, Davide ULg et al

in Advances in Space Research (2010), 40(10), 1266-1272

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See detailUnified description of fission in fusion and spallation reactions
Mancusi, Davide ULg; Charity, R. J.; Cugnon, Joseph ULg

in Physical Review. C : Nuclear Physics (2010), 82

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See detailImproved modelling of helium and tritium production for spallation targets
Leray, S.; Boudard, A.; Cugnon, Joseph ULg et al

in Nuclear Instruments & Methods in Physics Research. Section B, Beam Interactions with Materials and Atoms (2010), 268(6), 581-586

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See detailConstraining fission parameters for highly excited compound nuclei
Mancusi, Davide ULg; Cugnon, Joseph ULg; Charity, R. J.

in Seminar on Fission, het Pand (2010)

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See detailComparison between the SMM and GEMINI++ de-excitation models
Mancusi, Davide ULg; Cugnon, Joseph ULg; Boudard, A. et al

in Proceedings to the Satellite Meeting on Nuclear Spallation Reactions, International Topical Meeting on Nuclear Research Applications and Utilization of Accelerators 2009 (2010)

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See detailResults with INCL4
Cugnon, Joseph ULg; Mancusi, Davide ULg; Boudard, A. et al

in Proceedings to the Satellite Meeting on Nuclear Spallation Reactions, International Topical Meeting on Nuclear Research Applications and Utilization of Accelerators 2009 (2010)

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See detailSimulation of light ion collisions from Intra Nuclear Cascade (INCL-Fermi Breakup) relevant for medical irradiations and radioprotection
Boudard, A.; Leray, S.; Kaitaniemi, P. et al

in Proceedings to the International Topical Meeting on Nuclear Research Applications and Utilization of Accelerators 2009 (2010)

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See detailSchermatura dei protoni relativistici
Durante, M.; Bertucci, A.; Gialanella, G. et al

(2006, September)

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