0000000001202999

AUTHOR

R. Gumbsheimer

showing 17 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
researchProduct

First operation of the KATRIN experiment with tritium

2020

AbstractThe determination of the neutrino mass is one of the major challenges in astroparticle physics today. Direct neutrino mass experiments, based solely on the kinematics of $$\upbeta $$β-decay, provide a largely model-independent probe to the neutrino mass scale. The Karlsruhe Tritium Neutrino (KATRIN) experiment is designed to directly measure the effective electron antineutrino mass with a sensitivity of $$0.2\hbox { eV}$$0.2eV ($$90\%$$90% CL). In this work we report on the first operation of KATRIN with tritium which took place in 2018. During this commissioning phase of the tritium circulation system, excellent agreement of the theoretical prediction with the recorded spectra was …

Physics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsFOS: Physical scienceslcsh:Astrophysics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]TritiumKATRIN01 natural sciencesantineutrino/e: massHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)lcsh:QB460-4660103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]lcsh:Nuclear and particle physics. Atomic energy. RadioactivityMass scaleddc:530Electron Capture[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)010306 general physicsEngineering (miscellaneous)Nuclear ExperimentAstroparticle physicsPhysics010308 nuclear & particles physicstritiumPhysicsQuímicaInstrumentation and Detectors (physics.ins-det)sensitivityddc:lcsh:QC770-798TritiumHigh Energy Physics::ExperimentNeutrinoPräzisionsexperimente - Abteilung BlaumNeutrino Mass[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Electron neutrinoperformanceKATRINAstrophysics - Cosmology and Nongalactic Astrophysicsexperimental results
researchProduct

Reduction of stored-particle background by a magnetic pulse method at the KATRIN experiment

2018

Arenz, M., et al. “Reduction of Stored-Particle Background by a Magnetic Pulse Method at the KATRIN Experiment.” The European Physical Journal C, vol. 78, no. 9, Sept. 2018. © 2018 The Authors

Speichertechnik - Abteilung BlaumPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Field (physics)Physics::Instrumentation and DetectorsFOS: Physical scienceslcsh:AstrophysicsElectronKATRIN01 natural sciencesradon: nuclideNeutrino mass0103 physical scienceslcsh:QB460-466coillcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530Sensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsnumerical calculationsEngineering (miscellaneous)background: radioactivitybackground: suppressionPhysicsSpectrometer010308 nuclear & particles physicsPhysicsOrder (ring theory)Monte Carlo methodsInstrumentation and Detectors (physics.ins-det)Radon backgroundPulse (physics)13. Climate actionBackground reduction methodsPartículaslcsh:QC770-798spectrometerAtomic physicsElectricidadElectron neutrinoKATRIN
researchProduct

Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory

2011

We present the results of an analysis of data recorded at the Pierre Auger Observatory in which we search for groups of directionally-aligned events (or ‘multiplets’) which exhibit a correlation between arrival direc- tion and the inverse of the energy. These signatures are expected from sets of events coming from the same source after having been deflected by intervening coherent magnetic fields. The observation of several events from the same source would open the possibility to accurately reconstruct the position of the source and also measure the integral of the component of the magnetic field orthogonal to the trajectory of the cos- mic rays. We describe the largest multiplets found an…

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Field (physics)Astronomyultra-high energy cosmic rays; Pierre Auger Observatory; arrival directionsFOS: Physical sciencesCosmic rayAstrophysics01 natural sciencesCosmic RayAugerPosition (vector)0103 physical sciencesFIELDPierre auger observatory010303 astronomy & astrophysicsUltra-high energy cosmic rayDETECTORCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)Pierre Auger ObservatoryPhysicsArrival directions010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsIsotropyFísicaAstronomy and AstrophysicsASTROFÍSICAUltra-high energy cosmic raysMagnetic fieldExperimental High Energy PhysicsData analysisComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]RAIOS CÓSMICOSArrival directionUltra-High Energy Cosmic Ray
researchProduct

Suppression of Penning discharges between the KATRIN spectrometers

2020

The KArlsruhe TRItium Neutrino experiment (KATRIN) aims to determine the effective electron (anti)neutrino mass with a sensitivity of $0.2\textrm{ eV/c}^2$ (90$\%$ C.L.) by precisely measuring the endpoint region of the tritium $\beta$-decay spectrum. It uses a tandem of electrostatic spectrometers working as MAC-E (magnetic adiabatic collimation combined with an electrostatic) filters. In the space between the pre-spectrometer and the main spectrometer, an unavoidable Penning trap is created when the superconducting magnet between the two spectrometers, biased at their respective nominal potentials, is energized. The electrons accumulated in this trap can lead to discharges, which create a…

Speichertechnik - Abteilung BlaumPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsPenning trapFOS: Physical scienceslcsh:AstrophysicsSuperconducting magnetElectronTritiumKATRIN01 natural sciencesNuclear physics0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. RadioactivityElectron Captureddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentEngineering (miscellaneous)PhysicsSpectrometer010308 nuclear & particles physicsPhysicsInstrumentation and Detectors (physics.ins-det)Químicamagnet: superconductivityspectrometer: electrostaticPenning trapBeamlineBeta (plasma physics)electron: backgroundlcsh:QC770-798NeutrinoNeutrino MassKATRIN
researchProduct

First transmission of electrons and ions through the KATRIN beamline

2018

The Karlsruhe Tritium Neutrino (KATRIN) experiment is a large-scale effort to probe the absolute neutrino mass scale with a sensitivity of 0.2 eV (90% confidence level), via a precise measurement of the endpoint spectrum of tritium β-decay. This work documents several KATRIN commissioning milestones: the complete assembly of the experimental beamline, the successful transmission of electrons from three sources through the beamline to the primary detector, and tests of ion transport and retention. In the First Light commissioning campaign of autumn 2016, photoelectrons were generated at the rear wall and ions were created by a dedicated ion source attached to the rear section; in July 2017, …

Physics - Instrumentation and DetectorsIon beamFOS: Physical sciencesbeam transportion: beam[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]KATRIN7. Clean energy01 natural sciencesIonNuclear physics0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]electron: beam010306 general physicsInstrumentation[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear ExperimentMathematical Physicsactivity reportPhysics010308 nuclear & particles physicsphotoelectron: emissionInstrumentation and Detectors (physics.ins-det)Photoelectric effectstabilitysensitivityIon sourceddc:BeamlineCathode rayNeutrinoperformanceKATRIN
researchProduct

The Fluorescence Detector of the Pierre Auger Observatory

2010

The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays. It combines a surface array to measure secondary particles at ground level together with a fluorescence detector to measure the development of air showers in the atmosphere above the array. The fluorescence detector comprises 24 large telescopes specialized for measuring the nitrogen fluorescence caused by charged particles of cosmic ray air showers. In this paper we describe the components of the fluorescence detector including its optical system, the design of the camera, the electronics, and the systems for relative and absolute calibration. We also discuss the operation and the monitoring of the detecto…

Physics::Instrumentation and DetectorsAstronomyAUGERPIERRE7. Clean energy01 natural sciencesAugerFluorescence detectorData acquisitionDEPENDENCEATMOSPHERIC MULTIPLE-SCATTERINGInstrumentationPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsCOSMIC-RAYSUltra High Energy Cosmic RayCharged particleLIGHTSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAUGERNuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaMeasure (physics)FOS: Physical sciencesCosmic rayEXTENSIVE AIR-SHOWERSENERGIAFluorescence spectroscopyOptics0103 physical sciencesCosmic rays; Fluorescence detectorRECONSTRUCTION010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger ObservatoryPIERRE010308 nuclear & particles physicsbusiness.industryFísicaULTRA-HIGH ENERGY[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Experimental High Energy PhysicsPierre Auger observatoryCAPABILITIESHigh Energy Physics::Experimentbusiness
researchProduct

Calibration of high voltages at the ppm level by the difference of $^{83\mathrm{m}}$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 [superscript 83m]Kr conversion electron lines with the KATRIN setup, which was demonstrated during KATRIN’s commissioning measurements in July 2…

Speichertechnik - Abteilung BlaumPhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)FOS: Physical sciences7. Clean energy01 natural sciencesNuclear physics0103 physical sciencesCalibrationddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsEngineering (miscellaneous)[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]PhysicsTeoría de los quantaSpectrometer010308 nuclear & particles physicsPhysicsVoltage dividerInstrumentation and Detectors (physics.ins-det)MetrologyNeutrinoEnergy (signal processing)VoltageKATRIN
researchProduct

Search for First Harmonic Modulation in the Right Ascension Distribution of Cosmic Rays Detected at the Pierre Auger Observatory

2011

We present the results of searches for dipolar-type anisotropies in different energy ranges above 2.5 × 1017 eV with the surface detector array of the Pierre Auger Observatory, reporting on both the phase and the amplitude measurements of the first harmonic modulation in the right-ascension distribution. Upper limits on the amplitudes are obtained, which provide the most stringent bounds at present, being below 2% at 99% C.L. for EeV energies. We also compare our results to those of previous experiments as well as with some theoretical expectations.

Large scale anisotripies[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Auger ExperimentAstronomyAstrophysics::High Energy Astrophysical PhenomenaPhase (waves)FOS: Physical sciencesCosmic rayAstrophysicsanisotropySURFACE DETECTOR01 natural sciencesCosmic RayAugerLarge scale anisotropiesObservatoryLarge scale anisotropie0103 physical sciences010303 astronomy & astrophysicsUltra-high energy cosmic rayCiencias ExactasHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryFÍSICA DE PARTÍCULASUltra High Energy Cosmic Rays.010308 nuclear & particles physicsORIGINPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and AstrophysicsPierre Auger ObservatoryUltra-high energy cosmic raysENERGY-SPECTRUMRadiación cósmicaAnisotropíaAmplitudeHarmonicsUltra-high energy cosmic rays; Large scale anisotropies; Pierre Auger ObservatoryExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGARRAYFísica nuclearRight ascensionAstrophysics - High Energy Astrophysical Phenomena
researchProduct

High-resolution spectroscopy of gaseous $^\mathrm{83m}$Kr conversion electrons with the KATRIN experiment

2020

In this work, we present the first spectroscopic measurements of conversion electrons originating from the decay of metastable gaseous $^\mathrm{83m}$Kr with the Karlsruhe Tritium Neutrino (KATRIN) experiment. The results obtained in this calibration measurement represent a major commissioning milestone for the upcoming direct neutrino mass measurement with KATRIN. The successful campaign demonstrates the functionalities of the full KATRIN beamline. The KATRIN main spectrometer's excellent energy resolution of ~ 1 eV made it possible to determine the narrow K-32 and L$_3$-32 conversion electron line widths with an unprecedented precision of ~ 1 %.

Nuclear and High Energy PhysicsSpeichertechnik - Abteilung BlaumPhysics - Instrumentation and DetectorsResolution (mass spectrometry)Physics::Instrumentation and Detectorsenergy resolutionFOS: Physical sciencesElectron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]KATRIN7. Clean energy01 natural sciencesAtomicneutrino massNuclear physicsParticle and Plasma Physicsconversion electronsMetastability0103 physical sciencesNuclearddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)010306 general physicsSpectroscopyNuclear ExperimentPhysicsSpectrometerelectrostatic spectrometer010308 nuclear & particles physicsPhysicskrypton: decayMolecularInstrumentation and Detectors (physics.ins-det)krypton: nuclide530 PhysikcalibrationNuclear & Particles Physicsddc:3. Good healthBeamlineelectron: energy spectrumNeutrinoperformanceKATRIN
researchProduct

Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory

2011

Erratum: Phys. Rev. D 85, 029902(E) (2012) [http://dx.doi.org/10.1103/PhysRevD.85.029902]

Physics::Instrumentation and DetectorsSolar neutrinoAstrophysicsUPPER LIMITPHOTON FRACTION01 natural sciences7. Clean energyneutrinoObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsORIGINPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]pionAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryCOSMIC-RAYScosmic ray detectorsand other elementary particle detectorsCosmic neutrino backgroundNEUTRINOSFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaFLUXFERMI-LATNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]TELESCOPEAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayEXTENSIVE AIR-SHOWERSSURFACE DETECTORCosmic RayPionmuon0103 physical sciencesNeutrino010306 general physicsCosmic raysPierre Auger ObservatoryMuon010308 nuclear & particles physicsFísicaand other elementary particlesUltra-high energy cosmic raysPERFORMANCECosmic rayneutrino flavor; air showers; surface detector; observatory; atmosphere; Auger; cosmic radiation; energy spectrum13. Climate actionHigh Energy Physics::Experiment
researchProduct

The effect of the geomagnetic field on cosmic ray energy estimates and large scale anisotropy searches on data from the Pierre Auger Observatory

2011

We present a comprehensive study of the influence of the geomagnetic field on the energy estimation of extensive air showers with a zenith angle smaller than $60^\circ$, detected at the Pierre Auger Observatory. The geomagnetic field induces an azimuthal modulation of the estimated energy of cosmic rays up to the ~2% level at large zenith angles. We present a method to account for this modulation of the reconstructed energy. We analyse the effect of the modulation on large scale anisotropy searches in the arrival direction distributions of cosmic rays. At a given energy, the geomagnetic effect is shown to induce a pseudo-dipolar pattern at the percent level in the declination distribution t…

[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencescosmic ray experimentCosmic rayAstrophysicsultra high energy cosmic raysEXTENSIVE AIR-SHOWERS01 natural sciencesDeclinationultra high energy cosmic ray0103 physical sciencescosmic rays detectors; cosmic ray experiments; ultra high energy cosmic rayscosmic rays detectorAnisotropyInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsZenithParticle detectors.Pierre Auger ObservatoryPhysics010308 nuclear & particles physicsPhysicsOBSERVATÓRIOSAstrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomy and Astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AzimuthMODELEarth's magnetic fieldPhysics::Space PhysicsLarge detector systems for particle and astroparticle physicARRAYFísica nuclearcosmic rays detectorscosmic ray experimentsAstrophysics - Instrumentation and Methods for AstrophysicsEnergy (signal processing)Cherenkov detectorJournal of Cosmology and Astroparticle Physics
researchProduct

Impact of a cryogenic baffle system on the suppression of radon-induced background in the KATRIN Pre-Spectrometer

2018

The KATRIN experiment will determine the effective electron anti-neutrino mass with a sensitivity of 200 meV/c2 at 90% CL. The energy analysis of tritium β-decay electrons will be performed by a tandem setup of electrostatic retarding spectrometers which have to be operated at very low background levels of <10−2 counts per second. This benchmark rate can be exceeded by background processes resulting from the emanation of single 219,220Rn atoms from the inner spectrometer surface and an array of non-evaporable getter strips used as main vacuum pump. Here we report on the impact of a cryogenic technique to reduce this radon-induced background in electrostatic spectrometers. It is based on ins…

Materials scienceFlux tubeSpectrometer010308 nuclear & particles physicsbusiness.industryBaffleCryogenicsLiquid nitrogen01 natural scienceslaw.inventionOpticslawGetter0103 physical sciencesVacuum pump010306 general physicsbusinessInstrumentationMathematical PhysicsKATRINJournal of Instrumentation
researchProduct

Commissioning of the vacuum system of the KATRIN Main Spectrometer

2016

The KATRIN experiment will probe the neutrino mass by measuring the β-electron energy spectrum near the endpoint of tritium β-decay. An integral energy analysis will be performed by an electro-static spectrometer (``Main Spectrometer''), an ultra-high vacuum vessel with a length of 23.2 m, a volume of 1240 m[superscript 3], and a complex inner electrode system with about 120 000 individual parts. The strong magnetic field that guides the β-electrons is provided by super-conducting solenoids at both ends of the spectrometer. Its influence on turbo-molecular pumps and vacuum gauges had to be considered. A system consisting of 6 turbo-molecular pumps and 3 km of non-evaporable getter strips ha…

010302 applied physicsPhysicsLight nucleusPhysics - Instrumentation and DetectorsSpectrometerSpectrometersPhysics::Instrumentation and DetectorsVacuum-basedFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)01 natural sciencesEnergy analysisNuclear physics0103 physical sciencesEnergy spectrumGas systems and purificationNeutrino detectorsddc:620010306 general physicsInstrumentationMathematical PhysicsEngineering & allied operationsKATRINdetectors
researchProduct

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
researchProduct

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
researchProduct

Impact of a cryogenic baffle system on the suppression of radon-induced background in the KATRIN Pre-Spectrometer

2018

The KATRIN experiment will determine the effective electron anti-neutrino mass with a sensitivity of 200 meV/c$^2$ at 90% CL. The energy analysis of tritium $\beta$-decay electrons will be performed by a tandem setup of electrostatic retarding spectrometers which have to be operated at very low background levels of $<10^{-2}$ counts per second. This benchmark rate can be exceeded by background processes resulting from the emanation of single $^{219,220}$Rn atoms from the inner spectrometer surface and an array of non-evaporable getter strips used as main vacuum pump. Here we report on a the impact of a cryogenic technique to reduce this radon-induced background in electrostatic spectrometer…

Physics - Instrumentation and DetectorsFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)Nuclear Experiment (nucl-ex)Astrophysics - Instrumentation and Methods for AstrophysicsNuclear ExperimentInstrumentation and Methods for Astrophysics (astro-ph.IM)
researchProduct