Search results for " Direct search"

showing 4 items of 4 documents

Intrinsic backgrounds from Rn and Kr in the XENON100 experiment

2018

In this paper, we describe the XENON100 data analyses used to assess the target-intrinsic background sources radon ([InlineMediaObject not available: see fulltext.]), thoron ([InlineMediaObject not available: see fulltext.]) and krypton ([InlineMediaObject not available: see fulltext.]). We detail the event selections of high-energy alpha particles and decay-specific delayed coincidences. We derive distributions of the individual radionuclides inside the detector and quantify their abundances during the main three science runs of the experiment over a period of ∼4years, from January 2010 to January 2014. We compare our results to external measurements of radon emanation and krypton concentr…

data analysis methodPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)WIMPFOS: Physical scienceschemistry.chemical_elementlcsh:AstrophysicsRadonSciences de l'ingénieur01 natural sciencesIonNuclear physicsradon: nuclideXENONlcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Engineering (miscellaneous)nuclidebackground: radioactivitybackground: suppressionkryptonPhysicsRadionuclidePhysique010308 nuclear & particles physicsKryptonInstrumentation and Detectors (physics.ins-det)Alpha particleAstronomieDark Matter direct search experimentrespiratory tract diseasesRadon DaughtersBackgroundchemistrylcsh:QC770-798TPCAstrophysics - Instrumentation and Methods for Astrophysics
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XENON1T Dark Matter Data Analysis: Signal Reconstruction, Calibration and Event Selection

2019

The XENON1T experiment at the Laboratori Nazionali del Gran Sasso is the most sensitive direct detection experiment for dark matter in the form of weakly interacting particles (WIMPs) with masses above $6\,$GeV/$c^2$ scattering off nuclei. The detector employs a dual-phase time projection chamber with 2.0 metric tons of liquid xenon in the target. A one metric $\mathrm{ton}\times\mathrm{year}$ exposure of science data was collected between October 2016 and February 2018. This article reports on the performance of the detector during this period and describes details of the data analysis that led to the most stringent exclusion limits on various WIMP-nucleon interaction models to date. In pa…

xenon: targetWIMP nucleon: interactiondata analysis methodPhysics - Instrumentation and Detectorsinteraction: modelPhysics::Instrumentation and DetectorsDark matterchemistry.chemical_elementFOS: Physical sciencesdark matter: direct detection01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)XENONXenon0103 physical sciencesCalibration[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark MatterParticle Physics Experiments[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentDark Matter Direct Search Signal reconstruction calibratiuonPhysicsxenon: liquidTime projection chamber010308 nuclear & particles physicsScatteringSignal reconstructionDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)calibrationtime projection chamberEvent selectionchemistryHigh Energy Physics::Experimentperformance
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Dark Matter Search Results from a One Ton-Year Exposure of XENON1T

2018

We report on a search for Weakly Interacting Massive Particles (WIMPs) using 278.8 days of data collected with the XENON1T experiment at LNGS. XENON1T utilizes a liquid xenon time projection chamber with a fiducial mass of $(1.30 \pm 0.01)$ t, resulting in a 1.0 t$\times$yr exposure. The energy region of interest, [1.4, 10.6] $\mathrm{keV_{ee}}$ ([4.9, 40.9] $\mathrm{keV_{nr}}$), exhibits an ultra-low electron recoil background rate of $(82\substack{+5 \\ -3}\textrm{ (sys)}\pm3\textrm{ (stat)})$ events/$(\mathrm{t}\times\mathrm{yr}\times\mathrm{keV_{ee}})$. No significant excess over background is found and a profile likelihood analysis parameterized in spatial and energy dimensions exclude…

Dark matterGeneral Physics and Astronomychemistry.chemical_elementS030DI5WIMP: massElectronParameter spacedark matter: direct detectionGravitation and AstrophysicsS030DI101 natural sciencesS030DI3S030DI2Nuclear physicsXenonRecoilWIMPelectron: recoil0103 physical sciencesS046DM2[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 physicsnumerical calculationsDark Matter WIMP TPC XENON Direct searchPhysicsxenon: liquidTime projection chamber010308 nuclear & particles physicsbackgrounddark matter: massGran SassoWIMP nucleonchemistryWeakly interacting massive particles[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]time projection chamber: xenon[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Search for Light Dark Matter Interactions Enhanced by the Migdal Effect or Bremsstrahlung in XENON1T.

2019

Direct dark matter detection experiments based on a liquid xenon target are leading the search for dark matter particles with masses above ∼5 GeV/c2, but have limited sensitivity to lighter masses because of the small momentum transfer in dark matter-nucleus elastic scattering. However, there is an irreducible contribution from inelastic processes accompanying the elastic scattering, which leads to the excitation and ionization of the recoiling atom (the Migdal effect) or the emission of a bremsstrahlung photon. In this Letter, we report on a probe of low-mass dark matter with masses down to about 85 MeV/c2 by looking for electronic recoils induced by the Migdal effect and bremsstrahlung us…

xenon: targetPhysics - Instrumentation and Detectorsdark matter: interactionelastic scatteringGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)XenonIonizationexcited state[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentLight dark matterElastic scatteringPhysicsxenon: liquidatommomentum transferMomentum transferBremsstrahlungInstrumentation and Detectors (physics.ins-det)photon: bremsstrahlungS030DN5Weakly interacting massive particlesExcited stateAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterLight Dark Matter Direct search Liquid Xenon TPCFOS: Physical sciencesS030DI5chemistry.chemical_elementNuclear physicsParticle dark matterrecoilionization0103 physical sciencesDark matter[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsscintillation counterS030DP5010308 nuclear & particles physicsdown: masssensitivityDark matter Particle dark matter Weakly interacting massive particles* Automatic Keywords *chemistryElementary Particles and Fieldsbremsstrahlung: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Physical review letters
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