Abstract
We report on measurements of thermal neutron fluxes at different locations in the STAR experimental hall during pp = 510 GeV Run 13 at RHIC. We compared these measurements with calculations based on \textsc{PYTHIA} as minimum bias events generator, the detailed GEANT3 simulation of the STAR detector and the experimental hall, and using GCALOR as neutron transport code. A good (within 30%) agreement was found at locations near (1m) and very far (10m) from the beam pipe. For intermediate locations ( 5m) the simulation overestimates neutron flux by a factor of 3.
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