0000000000586067

AUTHOR

K. L. Giboni

showing 8 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
researchProduct

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
researchProduct

Limits on the release of Rb isotopes from a zeolite based 83mKr calibration source for the XENON project

2011

The isomer 83mKr with its half-life of 1.83 h is an ideal calibration source for a liquid noble gas dark matter experiment like the XENON project. However, the risk of contamination of the detector with traces of the much longer lived mother isotop 83Rb (86.2 d half-life) has to be ruled out. In this work the release of 83Rb atoms from a 1.8 MBq 83Rb source embedded in zeolite beads has been investigated. To do so, a cryogenic trap has been connected to the source for about 10 days, after which it was removed and probed for the strongest 83Rb gamma-rays with an ultra-sensitive Germanium detector. No signal has been found. The corresponding upper limit on the released 83Rb activity means tha…

Materials sciencePhysics - Instrumentation and DetectorsIsotope530 Physics3105 InstrumentationDark matterDetectorRadiochemistryCyclotronchemistry.chemical_elementNoble gasFOS: Physical sciences10192 Physics InstituteInstrumentation and Detectors (physics.ins-det)Semiconductor detectorlaw.inventionGenerator (circuit theory)Xenonchemistrylaw2610 Mathematical PhysicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentationInstrumentation and Methods for Astrophysics (astro-ph.IM)Mathematical Physics
researchProduct

Observation and applications of single-electron charge signals in the XENON100 experiment

2014

The XENON100 dark matter experiment uses liquid xenon in a time projection chamber (TPC) to measure xenon nuclear recoils resulting from the scattering of dark matter Weakly Interacting Massive Particles (WIMPs). In this paper, we report the observation of single-electron charge signals which are not related to WIMP interactions. These signals, which show the excellent sensitivity of the detector to small charge signals, are explained as being due to the photoionization of impurities in the liquid xenon and of the metal components inside the TPC. They are used as a unique calibration source to characterize the detector. We explain how we can infer crucial parameters for the XENON100 experim…

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsDrift velocity[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsDark matterchemistry.chemical_elementFOS: Physical sciencesdouble phase TPC01 natural sciencesdark matterHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)XenonWIMPdouble phase TPC; photoionization; single electron; xenon0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsphotoionizationInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsTime projection chamber010308 nuclear & particles physicsScatteringDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)single electron3. Good health[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]xenonchemistryWeakly interacting massive particlesAtomic physicsAstrophysics - Instrumentation and Methods for AstrophysicsJ. Phys.
researchProduct

Dark matter results from 225 live days of XENON100 data

2012

We report on a search for particle dark matter with the XENON100 experiment, operated at the Laboratori Nazionali del Gran Sasso (LNGS) for 13 months during 2011 and 2012. XENON100 features an ultra-low electromagnetic background of (5.3 \pm 0.6) \times 10^-3 events (kg day keVee)^-1 in the energy region of interest. A blind analysis of 224.6 live days \times 34 kg exposure has yielded no evidence for dark matter interactions. The two candidate events observed in the pre-defined nuclear recoil energy range of 6.6-30.5 keVnr are consistent with the background expectation of (1.0 \pm 0.2) events. A Profile Likelihood analysis using a 6.6-43.3 keVnr energy range sets the most stringent limit o…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsLarge Underground Xenon experimentDark matterFOS: Physical sciencesGeneral Physics and AstronomyWIMP Argon Programme01 natural sciences7. Clean energyParticle detectorHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMP0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsLiquid XenonPhysicsRange (particle radiation)010308 nuclear & particles physicsDARK MATTERInstrumentation and Detectors (physics.ins-det)High Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]DAMA/NaITPCPandaXDirect search for Dark MatterAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
researchProduct

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
researchProduct

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
researchProduct

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
researchProduct