2 types of simulations are required in this experiment. The first one is based
on an exact calculation of the magnetic field and then allows a very precise
determination of the proton trajectories. This is needed to precisely define
the shape and the location of the detectors. We can use also this
simulation to predict the contributions of the physical background
(background reactions coming from the target). The second type of
simulation uses
the
GEANT
software from the CERN.
It permits a very good and complete description of a particle passing
through the matter. An exact field calculation is not possible in
this simulation because of the computing time. The program will be
used to simulate the neutral background (neutrons, gamma) which can
interact with the detector.
The simulation without GEANT:
Kinematics of G0 experiment for the
forward angles measurements.
Impact of the trajectories in the focal plane (detector plane).
The simulation with GEANT:
Get
the simulation (last update the 11/01/2002), and read the
README file.
Comparison
of GRAAL photoproduction and Orsay photoproduction
and electroproduction
Generators
and experimental measurement of background particles.
Results (counting rates and time of flight of particles)
for first version of geometry (g0-5a.euclid) with no Cerenkov and FPD
at their nominal position (same results for
LD2 target).
Results (counting rates
and time of flight of particles)
for the version 2 of geometry (g0-5b.euclid), with Cerenkov and FPD
moved by 35 cm (downstream) from their nominal position (same results for
LD2 target).
Get the postscripts files for:
LH2 rates for 424 MeV,
576 MeV,
799 MeV.
LD2 rates for 424 MeV,
576 MeV,
799 MeV.
Ratio upstream/downstream window of the target for pions at
424 MeV,
576 MeV,
799 MeV.
And virtual/real ratio for pions and LD2 target at
424 MeV,
576 MeV,
799 MeV.
Simulation of
the data stream with realistic Time Of Fligth using the results of Geant.
Creation of coda files.