0000000001241027

AUTHOR

Y. Mei

showing 10 related works from this author

Likelihood approach to the first dark matter results from XENON100

2011

Many experiments that aim at the direct detection of Dark Matter are able to distinguish a dominant background from the expected feeble signals, based on some measured discrimination parameter. We develop a statistical model for such experiments using the Profile Likelihood ratio as a test statistic in a frequentist approach. We take data from calibrations as control measurements for signal and background, and the method allows the inclusion of data from Monte Carlo simulations. Systematic detector uncertainties, such as uncertainties in the energy scale, as well as astrophysical uncertainties, are included in the model. The statistical model can be used to either set an exclusion limit or …

PhysicsNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Scale (ratio)010308 nuclear & particles physicsMonte Carlo methodDark matterFOS: Physical sciencesStatistical model01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Frequentist inferenceWeakly interacting massive particles0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Test statisticLimit (mathematics)Statistical physics010306 general physicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Erratum: Study of the electromagnetic background in the XENON100 experiment [Phys. Rev. D 83, 082001 (2011)]

2012

Nuclear physicsPhysicsNuclear and High Energy PhysicsDark matterParticle detectorPhysical Review D
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Dark Matter Results from 100 Live Days of XENON100 Data

2011

We present results from the direct search for dark matter with the XENON100 detector, installed underground at the Laboratori Nazionali del Gran Sasso of INFN, Italy. XENON100 is a two-phase time projection chamber with a 62 kg liquid xenon target. Interaction vertex reconstruction in three dimensions with millimeter precision allows to select only the innermost 48 kg as ultra-low background fiducial target. In 100.9 live days of data, acquired between January and June 2010, no evidence for dark matter is found. Three candidate events were observed in a pre-defined signal region with an expected background of 1.8 +/- 0.6 events. This leads to the most stringent limit on dark matter interact…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Large Underground Xenon experiment010308 nuclear & particles physicsDARK MATTERDark matterHadronFOS: Physical sciencesGeneral Physics and AstronomyElementary particleFermion01 natural sciencesParticle detectorHigh Energy Physics - ExperimentWIMPSNuclear physicsHigh Energy Physics - Experiment (hep-ex)XENONWIMP0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]TPC010306 general physicsNucleonAstrophysics - Cosmology and Nongalactic Astrophysics
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Neutrinoless double beta decay with 82 SeF 6 and direct ion imaging

2018

We present a new neutrinoless double beta decay concept: the high pressure selenium hexafluoride gas time projection chamber. Combining techniques pioneered in high pressure xenon gas such as topological discrimination, with the high Q-value afforded by double beta decay isotope $^{82}$Se, a promising new detection technique is outlined. Lack of free electrons in SeF$_6$ mandates the use of an ion TPC. The microphysics of ion production and drift, which have many nuances, are explored. Background estimates are produced suggesting such a detector may achieve background indices of better than 1 count per ton per year in the region of interest at the 100~kg scale, and still better at the ton-s…

PhysicsTime projection chamberPhysics - Instrumentation and Detectors010308 nuclear & particles physicschemistry.chemical_elementFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)01 natural sciences7. Clean energyBeta decayParticle detectorIonHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)XenonchemistryDouble beta decay0103 physical sciences010306 general physicsInstrumentationMathematical PhysicsRadioactive decayLeptonJournal of Instrumentation
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Implications on inelastic dark matter from 100 live days of XENON100 data

2011

The XENON100 experiment has recently completed a dark matter run with 100.9 live-days of data, taken from January to June 2010. Events in a 48kg fiducial volume in the energy range between 8.4 and 44.6 keVnr have been analyzed. A total of three events have been found in the predefined signal region, compatible with the background prediction of (1.8 \pm 0.6) events. Based on this analysis we present limits on the WIMP-nucleon cross section for inelastic dark matter. With the present data we are able to rule out the explanation for the observed DAMA/LIBRA modulation as being due to inelastic dark matter scattering off iodine at a 90% confidence level.

PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsScatteringDARK MATTERSignal regionDark matterFOS: Physical sciences01 natural sciencesWIMPSNuclear physicsXENON0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]TPC010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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The distributed Slow Control System of the XENON100 experiment

2012

The XENON100 experiment, in operation at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy, was designed to search for evidence of dark matter interactions inside a volume of liquid xenon using a dual-phase time projection chamber. This paper describes the Slow Control System (SCS) of the experiment with emphasis on the distributed architecture as well as on its modular and expandable nature. The system software was designed according to the rules of Object-Oriented Programming and coded in Java, thus promoting code reusability and maximum flexibility during commissioning of the experiment. The SCS has been continuously monitoring the XENON100 detector since mid 2008, remotely recordi…

Physics - Instrumentation and Detectorsarchitecture[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]JavaComputer scienceReal-time computingFOS: Physical scienceschemistry.chemical_elementControl and monitor systems online; Control systems; Detector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases)algorithms01 natural sciencesXenon0103 physical scienceshardwareDETECTOR CONTROL SYSTEMS[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]CONTROL SYSTEMS010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationMathematical Physicscomputer.programming_languageTime projection chamber010308 nuclear & particles physicsbusiness.industryControl and monitor systems onlineDetector control systems (detector and experiment monitoring and slow-control systemsEmphasis (telecommunications)Volume (computing)Instrumentation and Detectors (physics.ins-det)Modular design[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]chemistryControl systemAstrophysics - Instrumentation and Methods for Astrophysicsdatabases)businesscomputerSystem software
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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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Study of the electromagnetic background in the XENON100 experiment

2011

The XENON100 experiment, located at the Laboratori Nazionali del Gran Sasso (LNGS), aims to directly detect dark matter in the form of Weakly Interacting Massive Particles (WIMPs) via their elastic scattering off xenon nuclei. We present a comprehensive study of the predicted electronic recoil background coming from radioactive decays inside the detector and shield materials, and intrinsic contamination. Based on GEANT4 Monte Carlo simulations using a detailed geometry together with the measured radioactivity of all detector components, we predict an electronic recoil background in the WIMP-search energy range (0-100 keV) in the 30 kg fiducial mass of less than 10e-2 events/(kg-day-keV), co…

Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsMonte Carlo methodDark matterchemistry.chemical_elementFOS: Physical sciences01 natural sciences7. Clean energyParticle detectorNuclear physicsXenonRecoil0103 physical sciences010306 general physicsNuclear ExperimentInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsElastic scattering010308 nuclear & particles physicsDetectorAstrophysics::Instrumentation and Methods for Astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]chemistryHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for AstrophysicsRadioactive decayAstrophysics - Cosmology and Nongalactic Astrophysics
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Material screening and selection for XENON100

2011

Results of the extensive radioactivity screening campaign to identify materials for the construction of XENON100 are reported. This Dark Matter search experiment is operated underground at Laboratori Nazionali del Gran Sasso (LNGS), Italy. Several ultra sensitive High Purity Germanium detectors (HPGe) have been used for gamma ray spectrometry. Mass spectrometry has been applied for a few low mass plastic samples. Detailed tables with the radioactive contaminations of all screened samples are presented, together with the implications for XENON100.

PhysicsPhysics - Instrumentation and Detectors010308 nuclear & particles physicsGamma rayLow activityFOS: Physical sciencesAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Mass spectrometry01 natural sciencesSemiconductor detectorNuclear physics0103 physical sciencesMass spectrum[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsGamma ray spectrometryUltra sensitive
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Erratum to: Guidelines for the use and interpretation of assays for monitoring autophagy (3rd edition) (Autophagy, 12, 1, 1-222, 10.1080/15548627.201…

2016

non presente

Molecular Biology; Cell BiologyCell BiologySettore BIO/06 - Anatomia Comparata E CitologiaMolecular Biology
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