0000000001302085

AUTHOR

B. Schulz

showing 7 related works from this author

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
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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
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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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A first search for coincident gravitational waves and high energy neutrinos using LIGO, Virgo and ANTARES data from 2007

2013

A search for high-energy neutrinos coming from the direction of the Sun has been performed using the data recorded by the ANTARES neutrino telescope during 2007 and 2008. The neutrino selection criteria have been chosen to maximize the selection of possible signals produced by the self-annihilation of weakly interacting massive particles accumulated in the centre of the Sun with respect to the atmospheric background. After data unblinding, the number of neutrinos observed towards the Sun was found to be compatible with background expectations. The 90% CL upper limits in terms of spin-dependent and spin-independent WIMP-proton cross-sections are derived and compared to predictions of two sup…

AstrofísicaEXPLOSIONSHigh energyPhotonPOINT SOURCESSUPERCONDUCTING COSMIC STRINGSGravitational waves / experimentsGravitational waves/experimentsAstrophysics01 natural scienceshigh energy neutrinosgravitational wavesgravitational waves / experiment010303 astronomy & astrophysicsQCmedia_commonLine (formation)QBPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)GAMMA-RAY BURSTSdark matter detectorsGravitational waves / experiments; Neutrino astronomy; Astronomy and Astrophysicshigh energy neutrinos[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsgravitational waves; gravitational waves / experiments; neutrino astronomy; high energy neutrinos; high energy neutrinosgravitational wavesgravitational wavesparticle physics - cosmology connectionNeutrino astronomyCOSMIC STRINGSRELATIVISTIC JETSNeutrinoAstrophysics - High Energy Astrophysical Phenomenasupersymmetry and cosmology[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]gravitational waves / experiments; neutrino astronomyTELESCOPEmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaSCIENCE RUNFOS: Physical sciencesddc:500.2GAMMA-RAY BURSTS; CORE-COLLAPSE SUPERNOVAE; SUPERCONDUCTING COSMIC STRINGS; MAGNETAR GIANT FLARES; SCIENCE RUN; RELATIVISTIC JETS; POINT SOURCES; BLACK-HOLES; LOCAL-RATE; TELESCOPEGravitational wavesGeneral Relativity and Quantum CosmologyCORE-COLLAPSE SUPERNOVAESettore FIS/05 - Astronomia e AstrofisicaCoincidentneutrino experiments0103 physical sciences010306 general physicsMAGNETAR GIANT FLARESBLACK-HOLESHigh Energy Astrophysical PhenomenaGravitational waveAstronomy[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsDRIVENUniverseLIGOGIANT FLARESLOCAL-RATEFISICA APLICADALUMINOSITYRADIATIONHigh Energy Physics::Experiment[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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CCDC 780779: Experimental Crystal Structure Determination

2013

Related Article: F.Emmerling, I.Orgzall, B.Dietzel, B.Schulz, J.Larrucea|2012|J.Mol.Struct.|1030|209|doi:10.1016/j.molstruc.2012.04.040

2-(Biphenyl-4-yl)-5-(4-t-butylphenyl)-134-oxadiazoleSpace GroupCrystallographyCrystal SystemCrystal StructureCell ParametersExperimental 3D Coordinates
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CCDC 780778: Experimental Crystal Structure Determination

2013

Related Article: F.Emmerling, I.Orgzall, B.Dietzel, B.Schulz, J.Larrucea|2012|J.Mol.Struct.|1030|209|doi:10.1016/j.molstruc.2012.04.040

2-(Biphenyl-4-yl)-5-phenyl-134-oxadiazoleSpace GroupCrystallographyCrystal SystemCrystal StructureCell ParametersExperimental 3D Coordinates
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CCDC 780777: Experimental Crystal Structure Determination

2013

Related Article: F.Emmerling, I.Orgzall, B.Dietzel, B.Schulz, J.Larrucea|2012|J.Mol.Struct.|1030|209|doi:10.1016/j.molstruc.2012.04.040

Space GroupCrystallographyCrystal SystemCrystal StructureCell Parameters2-(Biphenyl-4-yl)-5-(26-dimethylphenyl)-134-oxadiazoleExperimental 3D Coordinates
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