0000000001008765

AUTHOR

V. Hannen

showing 4 related works from this author

Calibration of high voltages at the ppm level by the difference of $$^{83{\mathrm{m}}}$$ 83m Kr conversion electron lines at the KATRIN experiment

2018

The neutrino mass experiment KATRIN requires a stability of 3 ppm for the retarding potential at − 18.6 kV of the main spectrometer. To monitor the stability, two custom-made ultra-precise high-voltage dividers were developed and built in cooperation with the German national metrology institute Physikalisch-Technische Bundesanstalt (PTB). Until now, regular absolute calibration of the voltage dividers required bringing the equipment to the specialised metrology laboratory. Here we present a new method based on measuring the energy difference of two $$^{83{\mathrm{m}}}$$ 83m Kr conversion electron lines with the KATRIN setup, which was demonstrated during KATRIN’s commissioning measurements …

lcsh:QB460-466lcsh:QC770-798lcsh:Astrophysicslcsh:Nuclear and particle physics. Atomic energy. RadioactivityEuropean Physical Journal C: Particles and Fields
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Improved Upper Limit on the Neutrino Mass from a Direct Kinematic Method by KATRIN

2019

We report on the neutrino mass measurement result from the first four-week science run of the Karlsruhe Tritium Neutrino experiment KATRIN in spring 2019. Beta-decay electrons from a high-purity gaseous molecular tritium source are energy analyzed by a high-resolution MAC-E filter. A fit of the integrated electron spectrum over a narrow interval around the kinematic end point at 18.57 keV gives an effective neutrino mass square value of (−1.0−1.1+0.9) eV2. From this, we derive an upper limit of 1.1 eV (90% confidence level) on the absolute mass scale of neutrinos. This value coincides with the KATRIN sensitivity. It improves upon previous mass limits from kinematic measurements by almost a …

Semileptonic decayPhysics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and DetectorsFOS: Physical sciencesGeneral Physics and AstronomyKinematicsElectron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]KATRIN01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)mass: scaleneutrino: mass: measured0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530S066MAESensitivity (control systems)Limit (mathematics)structure[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentPhysicstritiumPhysicsformationS066M2EInstrumentation and Detectors (physics.ins-det)semileptonic decaysensitivityddc:kinematicsElementary Particles and Fieldselectron: energy spectrumHigh Energy Physics::ExperimentPräzisionsexperimente - Abteilung BlaumNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)Astrophysics - Cosmology and Nongalactic AstrophysicsKATRINexperimental results
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Gamma-induced background in the KATRIN main spectrometer

2019

The KATRIN experiment aims to measure the effective electron antineutrino mass $$m_{\overline{\nu }_e}$$ mν¯e with a sensitivity of $${0.2}\,{\hbox {eV}/\hbox {c}^2}$$ 0.2eV/c2 using a gaseous tritium source combined with the MAC-E filter technique. A low background rate is crucial to achieving the proposed sensitivity, and dedicated measurements have been performed to study possible sources of background electrons. In this work, we test the hypothesis that gamma radiation from external radioactive sources significantly increases the rate of background events created in the main spectrometer (MS) and observed in the focal-plane detector. Using detailed simulations of the gamma flux in the e…

Speichertechnik - Abteilung BlaumPhysics - Instrumentation and Detectorsgamma ray: backgroundshieldingshielding: magneticPhysicsFOS: Physical scienceslcsh:AstrophysicsInstrumentation and Detectors (physics.ins-det)electron: secondarysensitivityKATRINbackground: lowlcsh:QB460-466electron: backgroundlcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530gamma ray: flux[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Electromagnetismonumerical calculationselectrostatic
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DARWIN: Towards the ultimate dark matter detector

2016

DARk matter WImp search with liquid xenoN (DARWIN) will be an experiment for the direct detection of dark matter using a multi-ton liquid xenon time projection chamber at its core. Its primary goal will be to explore the experimentally accessible parameter space for Weakly Interacting Massive Particles (WIMPs) in a wide mass-range, until neutrino interactions with the target become an irreducible background. The prompt scintillation light and the charge signals induced by particle interactions in the xenon will be observed by VUV sensitive, ultra-low background photosensors. Besides its excellent sensitivity to WIMPs above a mass of 5 GeV/c2, such a detector with its large mass, low-energy …

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsdouble beta decay7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentPhysics Particles & FieldsNeutrino detectorHigh Energy Physics - Experiment (hep-ex)XenonWIMPPHOTOMULTIPLIERAXIONSphysics.ins-detsolar and atmospheric neutrinosPhysicsDark matter detectorTime projection chamberdark matter detectorsPhysicsSolar and atmospheric neutrinoInstrumentation and Detectors (physics.ins-det)Nuclear & Particles PhysicsNeutrino detectorSOLAR NEUTRINOSGASPhysical SciencesNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsGRAN SASSODark matter detectors; Double beta decay; Neutrino detectors; Solar and atmospheric neutrinosDark matterchemistry.chemical_elementFOS: Physical sciencesAstronomy & AstrophysicsLIQUID-XENON DETECTOR0202 Atomic Molecular Nuclear Particle And Plasma PhysicsSettore FIS/05 - Astronomia e AstrofisicaSEARCH0103 physical sciencesIsotopes of xenonZEPLIN-III[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsAxionInstrumentation and Methods for Astrophysics (astro-ph.IM)Science & Technology010308 nuclear & particles physicshep-exAstronomyAstronomy and Astrophysics0201 Astronomical And Space ScienceschemistryHigh Energy Physics::ExperimentSCINTILLATIONneutrino detectorsastro-ph.IMJournal of Cosmology and Astroparticle Physics
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