Kavli Affiliate: Li Xin Li
| First 5 Authors: Zhen Cao, F. Aharonian, Q. An, Axikegu, Y. X. Bai
| Summary:
KM2A is one of the main sub-arrays of LHAASO, working on gamma ray astronomy
and cosmic ray physics at energies above 10 TeV. Detector simulation is the
important foundation for estimating detector performance and data analysis. It
is a big challenge to simulate the KM2A detector in the framework of Geant4 due
to the need to track numerous photons from a large number of detector units
(>6000) with large altitude difference (30 m) and huge coverage (1.3 km^2). In
this paper, the design of the KM2A simulation code G4KM2A based on Geant4 is
introduced. The process of G4KM2A is optimized mainly in memory consumption to
avoid memory overffow. Some simpliffcations are used to signiffcantly speed up
the execution of G4KM2A. The running time is reduced by at least 30 times
compared to full detector simulation. The particle distributions and the
core/angle resolution comparison between simulation and experimental data of
the full KM2A array are also presented, which show good agreement.
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