MARS flux simulations - update Sergei Striganov Fermilab June 3, 2009.

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Presentation transcript:

MARS flux simulations - update Sergei Striganov Fermilab June 3, 2009

Technical problems  Detectors are small 0.75x0.75x0.05 cm3  Direct MARS simulations can not provide acceptable statistical accuracy in reasonable time (7x24 hours 16 CPU)  Two ways to get small enough statistical errors: 1. using large detector size 2. pre-calculate sources for all detectors and run sources until get small statistical errors

Choice of methods Even with 20x20x0.1 cm3 detectors statistical errors exceed 40% for one of detectors in run Jet vertical radius is determined by magnetic field: 0 Tesla – 8.65 mm, 5 Tesla – 8.4 mm, 10 Tesla – 7.95 mm. Jet horizontal radius is same for round jet, but density is reduced. For elliptic jet horizontal radius is 0.25 cm2/vertical radius. Ilias model is used to determine beam size as function of beam intensity Source terms were calculated for 7 setups: elliptic jet, 0 Tesla, 0.25 Tp elliptic jet, 5 Tesla, 16 Tp elliptic rising radius jet, 5 Tesla, 16 Tp round jet, 0 Tesla, 0.25 Tp round jet, 5 Tesla, 16 Tp no jet, 0 Tesla, 0.25 Tp no jet, 5 Tesla, 16 Tp

Detector size in simulation All previous calculation were performed with large detectors. It is important to check how results depends on detector size. Simulations with large detector size (with reduced and/or real density) overestimate results obtained with real detector size It is more simple to run jobs with real detector size and pre- calculated sources, then find acceptable large detector size

Preliminary results

Conclusion  Simulation of particle detector signals should be performed with real detector size  It looks like that difference of detector signals for round and elliptic jet are not small  Systematic problems with -20 degree detector still unclear  Simulation with 5 other inputs should clarify dependence of detector signals on magnetic field and beam intensity  Update of measured detector signals at 14 and 24 GeV/c and different magnetic fields and beam intensities is needed