0000000000148507

AUTHOR

L. Bütikofer

showing 8 related works from this author

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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A low-mass dark matter search using ionization signals in XENON100

2016

We perform a low-mass dark matter search using an exposure of 30\,kg$\times$yr with the XENON100 detector. By dropping the requirement of a scintillation signal and using only the ionization signal to determine the interaction energy, we lowered the energy threshold for detection to 0.7\,keV for nuclear recoils. No dark matter detection can be claimed because a complete background model cannot be constructed without a primary scintillation signal. Instead, we compute an upper limit on the WIMP-nucleon scattering cross section under the assumption that every event passing our selection criteria could be a signal event. Using an energy interval from 0.7\,keV to 9.1\,keV, we derive a limit on …

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsPhysics::Instrumentation and DetectorsDark matterFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSignalHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMPIonization0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsPhysicsScintillation010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)Physics and Astronomy (miscellaneous) DARK MATTER XENON TPC WIMPHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Scintillation counterEnergy (signal processing)Astrophysics - Cosmology and Nongalactic Astrophysics
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The XENON1T Dark Matter Experiment

2017

The XENON1T experiment at the Laboratori Nazionali del Gran Sasso (LNGS) is the first WIMP dark matter detector operating with a liquid xenon target mass above the ton-scale. Out of its 3.2 t liquid xenon inventory, 2.0 t constitute the active target of the dual-phase time projection chamber. The scintillation and ionization signals from particle interactions are detected with low-background photomultipliers. This article describes the XENON1T instrument and its subsystems as well as strategies to achieve an unprecedented low background level. First results on the detector response and the performance of the subsystems are also presented. © 2017, The Author(s).

xenon: targetPhotomultiplierCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)WIMP[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Dark matterchemistry.chemical_elementFOS: Physical scienceslcsh:Astrophysics01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)XENONXenonbackground: lowWIMP[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]Ionization0103 physical scienceslcsh:QB460-466[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark Matterlcsh:Nuclear and particle physics. Atomic energy. Radioactivity[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsEngineering (miscellaneous)Instrumentation and Methods for Astrophysics (astro-ph.IM)[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]AstrophysiquePhysicsScintillationxenon: liquidTime projection chamberphotomultiplier010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)dark matter: detectortime projection chamberchemistrylcsh:QC770-798TPCAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]performanceAstrophysics - Cosmology and Nongalactic AstrophysicsEuropean Physical Journal C
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Physics reach of the XENON1T dark matter experiment.

2016

The XENON1T experiment is currently in the commissioning phase at the Laboratori Nazionali del Gran Sasso, Italy. In this article we study the experiment's expected sensitivity to the spin-independent WIMP-nucleon interaction cross section, based on Monte Carlo predictions of the electronic and nuclear recoil backgrounds. The total electronic recoil background in $1$ tonne fiducial volume and ($1$, $12$) keV electronic recoil equivalent energy region, before applying any selection to discriminate between electronic and nuclear recoils, is $(1.80 \pm 0.15) \cdot 10^{-4}$ ($\rm{kg} \cdot day \cdot keV)^{-1}$, mainly due to the decay of $^{222}\rm{Rn}$ daughters inside the xenon target. The nu…

dark matter simulationsPhysics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and Detectorsdark matter experimentFOS: Physical scienceschemistry.chemical_elementCosmic ray7. Clean energy01 natural sciencesdark matter simulationNuclear physicsRecoilXenonIonization0103 physical sciencesNeutronNuclear Experiment010306 general physicsPhysicsMuon010308 nuclear & particles physicsdark matter experimentsAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)dark matter experiments; dark matter simulationschemistryNeutrinoNucleonAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Removing krypton from xenon by cryogenic distillation to the ppq level

2017

The XENON1T experiment aims for the direct detection of dark matter in a detector filled with 3.3 tons of liquid xenon. In order to achieve the desired sensitivity, the background induced by radioactive decays inside the detector has to be sufficiently low. One major contributor is the β -emitter 85 Kr which is present in the xenon. For XENON1T a concentration of natural krypton in xenon natKr/Xe<200ppq (parts per quadrillion, 1 ppq =10−15mol/mol) is required. In this work, the design, construction and test of a novel cryogenic distillation column using the common McCabe–Thiele approach is described. The system demonstrated a krypton reduction factor of 6.4⋅10⁵ with thermodynamic stabili…

7. Clean energy
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Search for WIMP Inelastic Scattering off Xenon Nuclei with XENON100

2017

We present the first constraints on the spin-dependent, inelastic scattering cross section of weakly interacting massive particles (WIMPs) on nucleons from XENON100 data with an exposure of 7.64 ×103 kg .days . XENON100 is a dual-phase xenon time projection chamber with 62 kg of active mass, operated at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy and designed to search for nuclear recoils from WIMP-nucleus interactions. Here we explore inelastic scattering, where a transition to a low-lying excited nuclear state of Xe 129 is induced. The experimental signature is a nuclear recoil observed together with the prompt deexcitation photon. We see no evidence for such inelastic WIMP-Xe…

Physics - Instrumentation and DetectorsXenonPhysics and Astronomy (miscellaneous)Physics::Instrumentation and Detectors[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)XenonRecoilWIMP[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark MatterNuclear Experiment[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]nucleus: recoilPhysicsTime projection chamberAstrophysics::Instrumentation and Methods for AstrophysicsWIMP nucleon: cross sectionInstrumentation and Detectors (physics.ins-det)Excited stateWeakly interacting massive particlesTPCNucleonchannel cross section: measuredsignatureAstrophysics - Cosmology and Nongalactic AstrophysicsParticle physicsdata analysis methodCosmology and Nongalactic Astrophysics (astro-ph.CO)WIMPchemistry.chemical_elementFOS: Physical sciencesInelastic scatteringspin: dependenceNuclear physicsstatistical analysis[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]photon: emission0103 physical sciencescross section: inelastic scattering[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsWIMP nucleon: inelastic scattering010308 nuclear & particles physicsS030DP2WIMP nucleus: interactionGran SassochemistryDirect Searchtime projection chamber: xenonHigh Energy Physics::Experiment[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]experimental results
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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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Search for two-neutrino double electron capture of $^{124}$Xe with XENON100

2017

Two-neutrino double electron capture is a rare nuclear decay where two electrons are simultaneously captured from the atomic shell. For $^{124}$Xe this process has not yet been observed and its detection would provide a new reference for nuclear matrix element calculations. We have conducted a search for two-neutrino double electron capture from the K-shell of $^{124}$Xe using 7636 kg$\cdot$d of data from the XENON100 dark matter detector. Using a Bayesian analysis we observed no significant excess above background, leading to a lower 90 % credibility limit on the half-life $T_{1/2}>6.5\times10^{20}$ yr. We also evaluated the sensitivity of the XENON1T experiment, which is currently bein…

Nuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsElectron captureenergy resolutionFOS: Physical scienceschemistry.chemical_elementelectron: captureElectron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciencesBayesianX-rayneutrinoXenon0103 physical sciencesSensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det][ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear Experiment (nucl-ex)010306 general physics[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear ExperimentPhysicsnucleus: decayTime projection chamberphotomultiplier010308 nuclear & particles physicsbackgroundInstrumentation and Detectors (physics.ins-det)dark matter: detectorAtomic shellsensitivitytime projection chamberGran SassoxenonchemistryNeutrinoAtomic physicsRadioactive decayexperimental results
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