0000000000086240

AUTHOR

H. Qiu

showing 11 related works from this author

Excess electronic recoil events in XENON1T

2020

We report results from searches for new physics with low-energy electronic recoil data recorded with the XENON1T detector. With an exposure of 0.65 t-y and an unprecedentedly low background rate of $76\pm2$ events/(t y keV) between 1 and 30 keV, the data enables sensitive searches for solar axions, an enhanced neutrino magnetic moment, and bosonic dark matter. An excess over known backgrounds is observed at low energies and most prominent between 2 and 3 keV. The solar axion model has a 3.4$\sigma$ significance, and a 3D 90% confidence surface is reported for axion couplings to electrons, photons, and nucleons. This surface is inscribed in the cuboid defined by $g_{ae}<3.8 \times 10^{-12}$,…

xenon: targetaxionssolar axionmagnetic momentdimension: 3neutrino: solarPhysics beyond the Standard ModelSolar neutrinodark matter: direct detection01 natural sciences7. Clean energyHigh Energy Physics - ExperimentDark matter direct detection axionHigh Energy Physics - Experiment (hep-ex)neutrinoXENONHigh Energy Physics - Phenomenology (hep-ph)background: lowRecoilelectron: recoil[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]beta-raysParticle Physics Experimentscoupling: (axion 2electron)multi-purpose particle detectornuclear instrumentationComputingMilieux_MISCELLANEOUSinstrumentationPhysicsxenon: liquidboson: dark matteraxion 2nucleontritiumnew physics: search forsemileptonic decayboson: vectortensionneutrino: magnetic momentHigh Energy Physics - Phenomenologyaxion 2photonlow backgroundbosonNeutrinoionizing radiationNucleonAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)dark matter detectorelectronic recoilElectron captureXENON1T detectorDark matterlow-energy electronic recoil dataFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]dark matterNONuclear physicsPE2_2PE2_1tritium: semileptonic decay0103 physical sciencessolar axion modelsurface[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]axion: couplingPE2_4010306 general physicspseudoscalarAxiondark matter: vectordark matter XENON1T detector electronic recoilsolar neutrinodetectorDark Matter Axions Beta Decay Liquid Xenon TPC010308 nuclear & particles physicsaxion 2electroncoupling: (axion 2nucleon)dark matter: detectormodel: axionGran Sassometrology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]axionstellar constraintscoupling: (axion 2photon)High Energy Physics::Experimentparticle dark matterdirect detectionbeta decayaxion: solar[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]experimental results
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Light Dark Matter Search with Ionization Signals in XENON1T

2019

We report constraints on light dark matter (DM) models using ionization signals in the XENON1T experiment. We mitigate backgrounds with strong event selections, rather than requiring a scintillation signal, leaving an effective exposure of (22±3) tonne day. Above ∼0.4 keVee, we observe &lt;1 event/(tonne day keVee), which is more than 1000 times lower than in similar searches with other detectors. Despite observing a higher rate at lower energies, no DM or CEvNS detection may be claimed because we cannot model all of our backgrounds. We thus exclude new regions in the parameter spaces for DM-nucleus scattering for DM masses mχ within 3–6 GeV/c2, DM-electron scattering for mχ&gt;30 MeV/c2, a…

Light Dark Matter TPC Ionization Axion-Like particlesCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonFOS: Physical sciencesGeneral Physics and AstronomyS030DI5S029AECAstrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)S030DE5Ionization0103 physical sciencesionization[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsAbsorption (electromagnetic radiation)Light dark matterscintillation counterPhysicsDark Matter WIMP Dark-Matter detectors Time-projection chamber detectorsScintillationScatteringbackgrounddark matter: massphotonscatteringS029HPHS030DN5* Automatic Keywords *Scintillation counterElementary Particles and Fieldsaxion-like particles[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)absorptionAstrophysics - Cosmology and Nongalactic 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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$^{222}$Rn emanation measurements for the XENON1T experiment

2021

The selection of low-radioactive construction materials is of utmost importance for the success of low-energy rare event search experiments. Besides radioactive contaminants in the bulk, the emanation of radioactive radon atoms from material surfaces attains increasing relevance in the effort to further reduce the background of such experiments. In this work, we present the $^{222}$Rn emanation measurements performed for the XENON1T dark matter experiment. Together with the bulk impurity screening campaign, the results enabled us to select the radio-purest construction materials, targeting a $^{222}$Rn activity concentration of 10 $\mu$Bq/kg in 3.2 t of xenon. The knowledge of the distribut…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Radon emanationFOS: Physical scienceschemistry.chemical_element01 natural sciencesNOHigh Energy Physics - Experimentradon: nuclideHigh Energy Physics - Experiment (hep-ex)XENONXenon222 RnPE2_2PE2_10103 physical sciencesActivity concentration[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark Matter[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsEngineering (miscellaneous)background: radioactivityPhysicsradon: admixture010308 nuclear & particles physicsdetector: surfacescreeningInstrumentation and Detectors (physics.ins-det)chemistryXenon Dark matter 222 Rn radioactivityDark Matter Radon emanation XENON Direct Dark MatterDirect Dark MatterradioactivityAtomic physics
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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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Projected WIMP sensitivity of the XENONnT dark matter experiment

2020

XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In this work, we predict the experimental background and project the sensitivity of XENONnT to the detection of weakly interacting massive particles (WIMPs). The expected average differential background rate in the energy region of interest, corresponding to (1, 13) keV and (4, 50) keV for electronic and nuclear recoils, amounts to 12.3 ± 0.6 (keV t y)-1 and (2.2± 0.5)× 10−3 (keV t y)-1, respectively, in a 4 t fiducial mass. We compute unified confidence intervals using the profile construction method, in order to ensure proper coverage…

WIMP nucleon: scatteringdata analysis methodCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsHadronDark matterFOS: Physical sciencesElementary particledark matter: direct detection01 natural sciencesWIMP: dark matterHigh Energy Physics - ExperimentNONuclear physicsHigh Energy Physics - Experiment (hep-ex)XENONPE2_2WIMPPE2_1electron: recoil0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutron[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsPE2_4Dark matter experimentComputingMilieux_MISCELLANEOUSactivity reportnucleus: recoilPhysicsxenon: liquid010308 nuclear & particles physicsbackgroundAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)Dark matter experiments dark matter simulationssensitivityBaryonDark matter experimentsDark matter simulationsWeakly interacting massive particlesDark matter experiments; Dark matter simulationsNucleon[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Constraining the spin-dependent WIMP-nucleon cross sections with XENON1T

2019

We report the first experimental results on spin-dependent elastic weakly interacting massive particle (WIMP) nucleon scattering from the XENON1T dark matter search experiment. The analysis uses the full ton year exposure of XENON1T to constrain the spin-dependent proton-only and neutron-only cases. No significant signal excess is observed, and a profile likelihood ratio analysis is used to set exclusion limits on the WIMP-nucleon interactions. This includes the most stringent constraint to date on the WIMP-neutron cross section, with a minimum of 6.3 × 10−42 cm2 at 30 GeV/c2 and 90% confidence level. The results are compared with those from collider searches and used to exclude new paramet…

WIMP nucleon: interactionWIMP nucleon: scatteringParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)IsoscalarDark matterNuclear TheoryMassive particleGeneral Physics and AstronomyFOS: Physical sciencesParameter spacedark matter: direct detectionGravitation and Astrophysicsspin: dependence01 natural scienceslaw.inventionHigh Energy Physics - Phenomenology (hep-ph)WIMPlawisoscalar0103 physical sciencesS046DM1mediation010306 general physicsColliderPseudovectorPhysicsS030DN2S030DN1S030DP3S030DN3S030DP2S030DP1WIMP nucleon: cross sectionaxial-vectorHigh Energy Physics - PhenomenologyWIMPs Spin Dependent Cross Sections Neutron Cross Sections Likelihood methoddark matter: scattering[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::ExperimentNucleon[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysicsexperimental results
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First Results on the Scalar WIMP-Pion Coupling, Using the XENON1T Experiment

2018

We present first results on the scalar coupling of weakly interacting massive particles (WIMPs) to pions from 1 t yr of exposure with the XENON1T experiment. This interaction is generated when the WIMP couples to a virtual pion exchanged between the nucleons in a nucleus. In contrast to most nonrelativistic operators, these pion-exchange currents can be coherently enhanced by the total number of nucleons and therefore may dominate in scenarios where spin-independent WIMP-nucleon interactions are suppressed. Moreover, for natural values of the couplings, they dominate over the spin-dependent channel due to their coherence in the nucleus. Using the signal model of this new WIMP-pion channel, …

Nuclear TheoryPhysics::Instrumentation and DetectorsNuclear TheoryGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMPPions[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentS030UDMPhysicsStarke Wechselwirkung und exotische Kerne – Abteilung BlaumAstrophysics::Instrumentation and Methods for AstrophysicsnucleonsuppressionHigh Energy Physics - PhenomenologyWeakly interacting massive particlesmedicine.anatomical_structureWeakly interacting massive particlesNucleonCoherence (physics)Astrophysics - Cosmology and Nongalactic AstrophysicsWIMP nucleon: interactionParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]FOS: Physical sciencesWIMP: massspin: dependenceGravitation and Astrophysicsoperator: nonrelativisticDark matter Particle dark matter Pions Weakly interacting massive particles Dark matter detectorsNuclear Theory (nucl-th)PionParticle dark matter0103 physical sciencesmedicineDark mattercross section: upper limit010306 general physicsCouplingDark matter detectorsnucleusScalar (physics)coherenceDark Matter WIMP-Pion coupling Xenon Direct seartch[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experiment[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Nucleus
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Correction to: Potentially modifiable factors contributing to outcome from acute respiratory distress syndrome: the LUNG SAFE study (Intensive Care M…

2018

The members of the LUNG SAFE Investigators and the ESICM Trials Group were provided in such a way that they could not be indexed as collaborators on PubMed. The publisher apologizes for this error.

Critical Care and Intensive Care Medicine
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Resolved versus confirmed ARDS after 24 h: insights from the LUNG SAFE study

2018

Purpose: To evaluate patients with resolved versus confirmed ARDS, identify subgroups with substantial mortality risk, and to determine the utility of day 2 ARDS reclassification. Methods: Our primary objective, in this secondary LUNG SAFE analysis, was to compare outcome in patients with resolved versus confirmed ARDS after 24 h. Secondary objectives included identifying factors associated with ARDS persistence and mortality, and the utility of day 2 ARDS reclassification. Results: Of 2377 patients fulfilling the ARDS definition on the first day of ARDS (day 1) and receiving invasive mechanical ventilation, 503 (24%) no longer fulfilled the ARDS definition the next day, 52% of whom initial…

MaleARDSmedicine.medical_treatmentlnfectious Diseases and Global Health Radboud Institute for Molecular Life Sciences [Radboudumc 4]ARDS reassessment; ARDS Survival; Berlin criteria ARDS; Persisting ARDS;Critical Care and Intensive Care Medicineassisted ventilation0302 clinical medicineRisk Factors030212 general & internal medicinerisk factor AdultTidal volumecomparative studyeducation.field_of_studyRespiratory Distress SyndromeMortality rateRemission Inductiontidal volumeARDS reassessment; ARDS Survival; Berlin criteria ARDS; Persisting ARDS; Critical Care and Intensive Care MedicineARDS reassessmentartificial ventilationclinical trialimmunosuppressive treatmentadult respiratory distress syndromeMiddle AgedARDS SurvivalMonte Carlo methodmedicine.anatomical_structureclassificationpositive end expiratory pressureCardiologyDisease ProgressionSOFA scoredisease severityFemaleAdultmedicine.medical_specialtyPopulationdisease classificationArticleNO03 medical and health sciencesremissionlength of stayAnesthesiologyInternal medicinemedicinepneumoniaSequential Organ Failure Assessment ScoreHumanshumaneducationAgedMechanical ventilationhospital mortalityLungbusiness.industryRisk Factordisease associationRespiratory Distress Syndrome AdultPersisting ARDSmedicine.diseasemajor clinical studymortalityRespiration Artificialbreathing rate030228 respiratory systemdisease exacerbationBerlin criteria ARDSbusinessIntensive care medicine
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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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