Monte Carlo Simulation Variance Reduction Techniques for Photon Transport in Liquid Xenon Detectors
arXiv:2007.07719 · doi:10.1088/1475-7516/2021/03/071
Abstract
Monte Carlo simulations are a crucial tool for the analysis and prediction of various background components in liquid xenon (LXe) detectors. With improving shielding in new experiments, the simulation of external backgrounds, such as induced by gamma rays from detector materials, gets more computationally expensive. We introduce and validate an accelerated Monte Carlo simulation technique for photon transport in liquid xenon detectors. The method simulates photon-induced interactions within a defined geometry and energy range with high statistics while interactions outside of the region of interest are not simulated directly but are taken into account by means of probability weights. For a simulation of gamma induced backgrounds in an exemplary detector geometry we achieve a three orders of magnitude acceleration compared to a standard simulation of a current ton-scale LXe dark matter experiment.
References in corpus (11)
- Dark Matter Search Results from a One TonneYear Exposure of XENON1T
- Physics reach of the XENON1T dark matter experiment
- DARWIN: towards the ultimate dark matter detector
- Projected WIMP sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment
- Search for Neutrinoless Double-Beta Decay with the Complete EXO-200 Dataset
- Projected WIMP Sensitivity of the XENONnT Dark Matter Experiment
- The LUX-ZEPLIN (LZ) Experiment
- Radiogenic and Muon-Induced Backgrounds in the LUX Dark Matter Detector
- XENON1T Dark Matter Data Analysis: Signal Reconstruction, Calibration and Event Selection
- Material radioassay and selection for the XENON1T dark matter experiment
- The LUX-ZEPLIN (LZ) radioactivity and cleanliness control programs