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1.
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The Application of the Monte Carlo Code FLUKA in Radiation Protection Studies for the Large Hadron Collider
/ Battistoni, Giuseppe (INFN, Milan) ; Broggi, Francesco (INFN, Milan) ; Brugger, Markus (CERN) ; Campanella, Mauro (INFN, Milan) ; Carboni, Massimo (INFN, Legnaro) ; Empl, Anton (Houston U.) ; Fassò, Alberto (Jefferson Lab) ; Gadioli, Ettore (INFN, Milan) ; Cerutti, Francesco (CERN) ; Ferrari, Alfredo (CERN) et al.
2011
- Published in : Prog. Nucl. Sci. Tech. 2 (2011) 358-364
Fulltext: PDF; External link: Fulltext
In : Joint International Conference of the 7th Supercomputing in Nuclear Application and the 3rd Monte Carlo, Tokyo, Japan, 17 - 21 Oct 2010, pp.358-364
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2.
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Applications of FLUKA Monte Carlo code for nuclear and accelerator physics
/ Battistoni, Giuseppe (INFN, Milan ; Milan U.) ; Broggi, Francesco (INFN, Milan ; Milan U.) ; Brugger, Markus (CERN) ; Campanella, Mauro (INFN, Milan ; Milan U.) ; Carboni, Massimo (INFN, Legnaro) ; Empl, Anton (Houston U.) ; Fasso, Alberto (SLAC) ; Gadioli, Ettore (INFN, Milan ; Milan U.) ; Cerutti, Francesco (CERN) ; Ferrari, Alfredo (CERN) et al.
FLUKA is a general purpose Monte Carlo code capable of handling all radiation components from thermal energies (for neutrons) or 1keV (for all other particles) to cosmic ray energies and can be applied in many different fields. Presently the code is maintained on Linux. [...]
2011 - 7 p.
- Published in : Nucl. Instrum. Methods Phys. Res., B 269 (2011) 2850-2856
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3.
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Measurement of Fragmentation Products including Angular Distributions for 3, 5, and 10 GeV/A C and Si on several nuclear targets at the AGS
/ Pinsky, L (SPhN, DAPNIA, Saclay) ; Battistoni, G (Warsaw, Inst. Nucl. Studies) ; Broggi, F (Warsaw, Inst. Nucl. Studies) ; Brugger, M (GANIL) ; Campanella, M (Warsaw, Inst. Nucl. Studies) ; Carboni, M (Ioannina U.) ; Cerutti, F (GANIL) ; Colleoni, P (Warsaw, Inst. Nucl. Studies) ; Crystl, M (SPhN, DAPNIA, Saclay) ; D'Ambrosio, C (Ioannina U.) et al.
Motivated by differences in the predicted fragmentation of heavy ions at energies around 5 GeV/A as employed in the event generators used by the FLUKA Monte Carlo Code [1], a set of measurements were carried out at the AGS facility at the Brookhaven National Laboratory to determine as much information as possible about the cross sections to allow harmonization of those event generators for these incident lab energies. The FLUKA Code employs the RQMD event generator of Sorge [2] for heavy ion interactions starting at 100 MeV/A and extending into the region around 5 GeV/A. [...]
2010
Published version from CERN: PDF;
In : 12th International Conference on Nuclear Reaction Mechanisms, Villa Monastero, Varenna, Italy, 15 - 19 Jun 2009, pp.431-438
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4.
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Update On the Status of the FLUKA Monte Carlo Transport Code
/ Ferrari, A (CERN) ; Lorenzo-Sentis, M (CERN) ; Roesler, S (CERN) ; Smirnov, G (CERN) ; Theis, C (CERN) ; Vlachoudis, V (CERN) ; Carboni, M ; Mostacci, A ; Pelliccioni, M ; Villari, R et al.
2006
In : 15th International Conference on Computing In High Energy and Nuclear Physics, Mumbai, India, 13 - 17 Feb 2006, pp.294-302
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5.
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The FLUKA Code : an overview
/ Ballarini, F ; Battistoni, G ; Campanella, M ; Carboni, M ; Cerutti, F ; Empl, A ; Fassò, A ; Ferrari, A ; Gadioli, E ; Garzelli, M V et al.
SLAC-PUB-11549.-
Stanford, CA : SLAC, 2006 - 10 p.
- Published in : J. Phys.: Conf. Ser. 41 (2006) 151-160
External link: Fulltext from SLAC
In : 19th EPS Nuclear Physics Divisional Conference : New Trends In Nuclear Physics Applications And Technology, Pavia, Italy, 5 - 9 Sep 2005, pp.151-160
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6.
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The cosmic ray proton, helium and CNO fluxes in the 100 TeV energy region from TeV muons and EAS atmospheric Cherenkov light observations of MACRO and EAS-TOP
/ Aglietta, M ; Alessandro, B ; Ambrosio, M ; Antolini, R ; Antonioli, P ; Arneodo, F ; Baldini, A ; Barbarino, G C ; Barish, B C ; Battistoni, G et al.
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80-300 TeV are studied at the National Gran Sasso Laboratories by means of EAS-TOP (Campo Imperatore, 2005 m a.s.l.) and MACRO (deep underground, 3100 m w.e., the surface energy threshold for a muon reaching the detector being E/sub mu //sup th/ approximately=1.3 TeV). The measurement is based on: (a) the selection of primaries based on their energy/nucleon (i.e., with energy/nucleon sufficient to produce a muon with energy larger than 1.3 TeV) and the reconstruction of the shower geometry by means of the muons recorded by MACRO in the deep underground laboratories; (b) the detection of the associated atmospheric Cherenkov light (C.l.) signals by means of the C.l. [...]
2004
- Published in : Astropart. Phys. 21 (2004) 223-40
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10.
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The cosmic ray primary composition between $10^{15}$ and $10^{16}$ ev from Extensive Air Showers electromagnetic and TeV muon data
/ Aglietta, M ; Alessandro, B ; Ambrosio, M ; Antolini, R ; Antonioli, P ; Arneodo, F ; Baldini, A ; Barbarino, G C ; Barish, B C ; Battistoni, G et al.
The cosmic ray primary composition in the energy range between 10/sup 15/ and 10/sup 16/ eV, i.e., around the "knee" of the primary spectrum, has been studied through the combined measurements of the EAS-TOP air shower array (2005 m a.s.l., 10/sup 5/ m/sup 2/ collecting area) and the MACRO underground detector (963 m a.s.l., 3100 m w.e. of minimum rock overburden, 920 m/sup 2/ effective area) at the National Gran Sasso Laboratories. [...]
2004
- Published in : Astropart. Phys. 20 (2004) 641-52
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