6533b7d7fe1ef96bd1267c11

RESEARCH PRODUCT

Conceptual design and simulation of a water Cherenkov muon veto for the XENON1T experiment

Y. MengM. MurraN. PrielJean-pierre CussonneauM. MessinaFlorian KaetherM. SelviK. ArisakaGian Carlo TrincheroEilam GrossA. RizzoA. BehrensC. ReuterS. SchindlerLuke GoetzkeS. E. A. OrrigoJ. A. M. LopesJ. NaganomaAuke-pieter ColijnA. KishD. Mayani ParasGabriella SartorelliA. LyashenkoR. PersianiS. ReichardA. MolinarioL. LevinsonB. MiguezF. ArneodoP. BarrowGiacomo BrunoF. V. MassoliA. TeymourianS. FattoriW. HampelAmos BreskinBoris BauermeisterR. F. LangE. PanticK. BokelohD. LellouchEthan BrownJoão CardosoL. Scotto LavinaW. FulgioneJ. SchreinerM. WeberS. MacmullinM. P. DecowskiManfred LindnerRan BudnikA. D. FerellaG. KesslerK. LungD. ThersG. PlanteA. TiseniHongwei WangC. GrignonF. PiastraJ.m.f. Dos SantosMarc SchumannP. ShaginJulien MasbouH. SimgenJ. PienaarF. AgostiniA. J. Melgarejo FernandezM. AugerM. AlfonsiP. BeltrameS. RosendahlSebastian LindemannC. BalanG. MoranaElena AprileT. Marrodán UndagoitiaCh. WeinheimerUwe OberlackApril S. BrownR. ItayM. GarbiniE. DuchovniLaura BaudisM. Le CallochS. BruennerC. LevyO. VitellsC. GeisH. ContrerasH. Landsman

subject

axionsPhysics - Instrumentation and Detectors[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Cherenkov and transition radiationCherenkov detectorPhysics::Instrumentation and DetectorsDark matterDetector modelling and simulations I (interaction of radiation with matterchemistry.chemical_elementFOS: Physical sciences01 natural scienceslaw.inventionNuclear physicsXenonWIMPlawCherenkov and transition radiation Detector modelling and simulations Cherenkov detectors Dark Matter detectorsetc.)0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentationInstrumentation and Methods for Astrophysics (astro-ph.IM)Dark Matter detectors (WIMPsMathematical PhysicsCherenkov radiationetc)PhysicsMuonTime projection chamber010308 nuclear & particles physicsCherenkov detectorsDetectorAstrophysics::Instrumentation and Methods for Astrophysicsinteraction of photons with matterInstrumentation and Detectors (physics.ins-det)Cherenkov and transition radiation; Cherenkov detectors; Dark Matter detectors (WIMPs axions etc.); Detector modelling and simulations I (interaction of radiation with matter; interaction of hadrons with matter etc); interaction of photons with matter[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]interaction of hadrons with matterchemistryHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for Astrophysics

description

XENON is a direct detection dark matter project, consisting of a time projection chamber (TPC) that uses xenon in double phase as a sensitive detection medium. XENON100, located at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy, is one of the most sensitive experiments of its field. During the operation of XENON100, the design and construction of the next generation detector (of ton-scale mass) of the XENON project, XENON1T, is taking place. XENON1T is being installed at LNGS as well. It has the goal to reduce the background by two orders of magnitude compared to XENON100, aiming at a sensitivity of $2 \cdot 10^{-47} \mathrm{cm}^{\mathrm{2}}$ for a WIMP mass of 50 GeV/c$^{2}$. With this goal, an active system that is able to tag muons and their induced backgrounds is crucial. This active system will consist of a water Cherenkov detector realized with a water volume $\sim$10 m high and $\sim$10 m in diameter, equipped with photomultipliers of 8 inches diameter and a reflective foil. In this paper we present the design and optimization study for this muon veto water Cherenkov detector, which has been carried out with a series of Monte Carlo simulations, based on the GEANT4 toolkit. This study showed the possibility to reach very high detection efficiencies in tagging the passage of both the muon and the shower of secondary particles coming from the interaction of the muon in the rock: >99.5% for the former type of events (which represent $\sim$ 1/3 of all the cases) and >70% for the latter type of events (which represent $\sim$ 2/3 of all the cases). In view of the upgrade of XENON1T, that will aim to an improvement in sensitivity of one order of magnitude with a rather easy doubling of the xenon mass, the results of this study have been verified in the upgraded geometry, obtaining the same conclusions.

10.1088/1748-0221/9/11/p11006http://dx.doi.org/10.1088/1748-0221/9/11/P11006