FLUKA is a general purpose Monte Carlo transport and interaction code used for fundamental physics and for a wide range of applications. These include cosmic ray physics (muons, neutrinos, extensive air showers, underground physics), both for basic research and applied studies in space and atmospheric flight dosimetry and radiation damage. A review of the hadronic models available in FLUKA and relevant for the description of cosmic ray air showers is presented in this paper. Recent improvements concerning these models are discussed. The FLUKA capabilities in the simulation of the formation and propagation of EM and hadronic showers in the terrestrial atmosphere are shown.

The hadronic models for cosmic ray physics : the FLUKA code solutions / G. Battistoni, F. Cerutti, A. Empl, A. Fasso, A. Ferrari, E. Gadioli, M. V. Garzelli, S. Muraro, M. Pelliccioni, L. S. Pinsky, J. Ranft, S. Roesler, P. R. Sala, R. Villari. - In: NUCLEAR PHYSICS B-PROCEEDINGS SUPPLEMENTS. - ISSN 0920-5632. - 175 - 176:(2008), pp. 88-95. (Intervento presentato al 14. convegno ISVHECRI : International symposium on very high energy cosmic ray interactions tenutosi a Weihai, China nel 2006) [10.1016/j.nuclphysbps.2007.10.013].

The hadronic models for cosmic ray physics : the FLUKA code solutions

E. Gadioli;M.V. Garzelli;
2008

Abstract

FLUKA is a general purpose Monte Carlo transport and interaction code used for fundamental physics and for a wide range of applications. These include cosmic ray physics (muons, neutrinos, extensive air showers, underground physics), both for basic research and applied studies in space and atmospheric flight dosimetry and radiation damage. A review of the hadronic models available in FLUKA and relevant for the description of cosmic ray air showers is presented in this paper. Recent improvements concerning these models are discussed. The FLUKA capabilities in the simulation of the formation and propagation of EM and hadronic showers in the terrestrial atmosphere are shown.
extended air showers
2008
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/60517
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