MonteCarlo simulations with GEANT4 for the XENON100 Detector

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Location of the XENON-100 experiment LNGS LNGS ROME L’AQUILA Tunnel of 10.4 km TERAMO Xenon 1.4 km rock = 3100 meters water equivalent shielding from cosmic rays Alexander Kish | XENON100 | 14th Geant4 Users Workshop | Catania, Sicily | October 15, 2009 | p.6
The Principle of the XENON experiment Electron/nuclear recoils discrimination based on S2/S1 ratio Alexander Kish | XENON100 | 14th Geant4 Users Workshop | Catania, Sicily | October 15, 2009 | p.7
Page 1 and 2: MonteCarlo simulations with GEANT4
Page 3 and 4: XENON-100 collaboration 45 research
Page 5: Target Volume ~100 kg Muon Veto QUP
Page 9 and 10: Simulation of the Optical Response
Page 11 and 12: Prediction of the Detected Light Yi
Page 13 and 14: Backgrounds Prediction SOURCES OF E
Page 15 and 16: Predicted Electron Recoil Backgroun
Page 17 and 18: Intrinsic Contamination: Delayed Co
Page 19 and 20: Gamma Background from 222 Rn in the
Page 21 and 22: Neutrons from (α,n) reactions and
Page 23 and 24: Muon-Induced Neutron Background Con
Page 25: Thank you. Special thanks to: Dr. E

MonteCarlo simulations with GEANT4 for the XENON100 Detector

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