Speaker
G. Battistoni
(INFN Milano, Italy)
Description
The FLUKA Monte Carlo transport code is being used for different
applications in High Energy, Cosmic Ray and Accelerator Physics.
Here we review some of the ongoing projects which are
based on this simulation tool.
In particular, as far as accelerator physics is concerned, we wish
to summarize the work in progress for the LHC and the CNGS project.
From the point of view of experimental activity, a part the activity
going
in the framework of LHC detectors, we wish to discuss
as a major example the application of FLUKA to the ICARUS Liquid
Argon TPC.
Upgrades in cosmic ray calculations, to demonstrate the capability
of FLUKA to reproduce existing experimental data, are also presented
Primary authors
A. Empl
(University of Houston, Texas, USA)
A. Fasso
(SLAC, Stanford, USA)
A. Ferrari
(CERN, Geneva, Switerland)
A. Ottolenghi
(Universita' and INFN Pavia)
D. Scannicchio
(Univeristy and INFN, Pavia, Italy)
E. Gadioli
(University and INFN, Milano, Italy)
F. Ballarini
(University and INFN Pavia, Italy)
F. Cerutti
(Univeristy and INFN Milano, Italy)
G. Battistoni
(INFN Milano, Italy)
J. Ranft
(University of Siegen, Germany)
K. TSOULOU
(CERN Geneva, Switzerland)
L. Pinsky
(University of Houston, Texas, USA)
M V. Garzelli
(Univeristy and INFN, Milano, Italy)
M. PELLICCIONI
(INFN, Frascati, Italy)
P. Sala
(ETH, Zurich, Switerland)
S. MURARO
(INFN Milano, Italy)
S. Roesler
(CERN, Geneva, Switzerland)
T. RANCATI
(INFN Milano, Italy)
V. PARINI
(INFN and University di Pavia, Italy)
V. Vlachoudis
(CERN, Geneva, Switerland)
