6533b7d1fe1ef96bd125d969
RESEARCH PRODUCT
Results from a calibration of XENON100 using a source of dissolved radon-220
The Collaboration XenonE. AprileJ. AalbersF. AgostiniM. AlfonsiF. D. AmaroM. AnthonyF. ArneodoP. BarrowL. BaudisB. BauermeisterJ. A. M. LopesR. ItayB. KaminskyG. KesslerA. KishU. OberlackH. LandsmanR. F. LangM. LecallochD. LellouchF. PiastraQ. LinS. LindemannA. ManfrediniM. LindnerI. MarisT. Marrodan UndagoitiaF. V. MassoliJ. MasbouD. MassonD. MayaniM. MessinaY. MengK. MicheneauB. MiguezA. MolinarioJ. SchreinerM. MurraJ. NaganomaS. E. A. OrrigoK. NiE. ShockleyP. PakarhaB. PelssersJ. PienaarR. PersianiM. -C PiroG. P. LanteL. RauchN. PrielS. ReichardC. ReuterS. RosendahlA. RizzoN. RuppR. SaldanhaJ. M. F. Dos SantosM. L. BenabderrahmaneG. SartorelliM. ScheibelhutM. SchumannS. SchindlerS. BruennerL. Scotto LavinaM. SelviM. SilvaP. ShaginH. SimgenM. V. SiversD. ThersA. SteinA. TiseniG. TrincheroN. UpoleC. TunnellH. WangY. WeiC. WeinheimerJ. M. R. CardosoJ. WulfJ. YeT. BergerY. ZhangA. FieguthP. A. BreurA. BrownG. BrunoE. BrownR. BudnikL. ButikoferM. CervantesJ. CalvenD. CichonD. CoderreJ. ConradA. P. ColijnJ. P. CussonneauM. P. DecowskiP. DeperioF. GaoP. DigangiA. DigiovanniS. DiglioE. DuchovniL. LevinsonG. EurinJ. FeiD. FrancoA. D. FerellaW. FulgioneAndrea Gallo RossoM. GarbiniM. GallowayC. GeisL. W. GoetzkeZ. GreeneL. GrandiC. GrignonC. HasterokE. Hogenbirksubject
Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsDark matterFOS: Physical scienceschemistry.chemical_elementRadon01 natural sciencesCoincidenceNuclear physicsRecoilOpticsXenonXENON DARK MATTER WIMPS CALIBRATION RADON0103 physical sciencesCalibration[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsPhysics010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics::Instrumentation and Methods for AstrophysicsOrder (ring theory)Instrumentation and Detectors (physics.ins-det)chemistryHigh Energy Physics::Experimentbusinessdescription
A Rn 220 source is deployed on the XENON100 dark matter detector in order to address the challenges in calibration of tonne-scale liquid noble element detectors. We show that the Pb 212 beta emission can be used for low-energy electronic recoil calibration in searches for dark matter. The isotope spreads throughout the entire active region of the detector, and its activity naturally decays below background level within a week after the source is closed. We find no increase in the activity of the troublesome Rn 222 background after calibration. Alpha emitters are also distributed throughout the detector and facilitate calibration of its response to Rn 222 . Using the delayed coincidence of Rn 220 - Po 216 , we map for the first time the convective motion of particles in the XENON100 detector. Additionally, we make a competitive measurement of the half-life of Po 212 , t1 /2=(293.9 ±(1.0 )stat±(0.6 )sys) ns .
year | journal | country | edition | language |
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2017-04-11 |