Search results for " Wimps"

showing 4 items of 4 documents

Search for Event Rate Modulation in XENON100 Electronic Recoil Data

2015

We have searched for periodic variations of the electronic recoil event rate in the (2-6) keV energy range recorded between February 2011 and March 2012 with the XENON100 detector, adding up to 224.6 live days in total. Following a detailed study to establish the stability of the detector and its background contributions during this run, we performed an un-binned profile likelihood analysis to identify any periodicity up to 500 days. We find a global significance of less than 1 sigma for all periods suggesting no statistically significant modulation in the data. While the local significance for an annual modulation is 2.8 sigma, the analysis of a multiple-scatter control sample and the phas…

Dark Matter Wimps ModulationPhysicsPhysics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)530 PhysicsDetectorDark matterPhase (waves)FOS: Physical sciencesGeneral Physics and AstronomySigmaInstrumentation and Detectors (physics.ins-det)AstrophysicsParticle detectorHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)RecoilModulation[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Event (particle physics)Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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Analysis of the XENON100 dark matter search data

2014

The XENON100 experiment, situated in the Laboratori Nazionali del Gran Sasso, aims at the direct detection of dark matter in the form of weakly interacting massive particles (WIMPs), based on their interactions with xenon nuclei in an ultra low background dual-phase time projection chamber. This paper describes the general methods developed for the analysis of the XENON100 data. These methods have been used in the 100.9 and 224.6 live days science runs from which results on spin-independent elastic, spin-dependent elastic and inelastic WIMP-nucleon cross-sections have already been reported.

Large Underground Xenon experimentPhysics - Instrumentation and DetectorsXenonWIMPPhysics::Instrumentation and DetectorsDirect detectionDark matterchemistry.chemical_elementFOS: Physical sciencesDarkSideWIMP Argon ProgrammeNuclear physicsXenonDark matterStatistical analysisNuclear ExperimentInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsTime projection chamberAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)WIMPschemistryWeakly interacting massive particlesDark matter; Direct detection; WIMPs; XenonAstrophysics - Instrumentation and Methods for AstrophysicsAstroparticle Physics
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Results from a calibration of XENON100 using a source of dissolved radon-220

2017

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 R…

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::Experimentbusiness
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IceCube: A multipurpose neutrino telescope

2008

IceCube is a new high-energy neutrino telescope which will be coming online in the near future. IceCube will be capable of measuring fluxes of all three flavors of neutrino, and its peak neutrino energy sensitivity will be in the TeV–PeV range. Here, after a brief description of the detector, we describe its anticipated performance with a selection of physics topics: supernovae, extraterrestrial diffuse and point sources of neutrinos, gamma-ray bursts, neutrinos from WIMP annihilation, and cosmic ray composition.

Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoGeneral Physics and AstronomyAstrophysics7. Clean energy01 natural sciencesWIMP0103 physical sciencesNeutrinos010306 general physicsCosmic rays; Neutrinos; WIMPsCosmic raysPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsAstronomySolar neutrino problemWIMPsCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomy
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