0000000000313201

AUTHOR

Jan Glorius

showing 4 related works from this author

Neutron transmission measurements at nELBE

2020

International Conference on Nuclear Data for Science and Technology, ND 2019, Bejing, China, 19 May 2019 - 24 May 2019; The European physical journal / Web of Conferences 239, 01006 (2020). doi:10.1051/epjconf/202023901006

Astrophysics::High Energy Astrophysical PhenomenaQC1-999FluxNeutron transmission53001 natural sciences238UNuclear physicsXe0103 physical sciencesNeutronddc:530High pressure gas010306 general physicsPhysicsHe010308 nuclear & particles physicsNePhysicsOPtnELBE time of flight faciltiyneutron total cross sectionstransmission measurementNatBar (unit)
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Behavior of a trapezoid-based data acquisition system up to 100 kHz and beyond

2016

In this work, we investigated the ability of a high-purity germanium detector connected to a trapezoid-filter-based data acquisition system to reliably record signals in spite of high sample activities. By activating multiple Na$_{2}$CO$_{3}$ samples with different Na content, we were able to deduce efficiency, resolution and dead time of the system used as a function of the sample activity. Based on the results, we were able to find a setting which allows measurements of event rates up to 35~kHz per readout channel with an energy resolution of 0.3\% at the 2754 keV $^{24}$Na line.

PhysicsNuclear and High Energy PhysicsPhysics - Instrumentation and Detectorsbusiness.industryResolution (electron density)FOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)Dead timeSample (graphics)Semiconductor detectorData acquisitionOpticsLine (text file)Nuclear Experiment (nucl-ex)businessNuclear ExperimentInstrumentationEnergy (signal processing)Communication channel
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Thermal neutron capture cross section of the radioactive isotopeFe60

2015

Background: Fifty percent of the heavy element abundances are produced via slow neutron capture reactions in different stellar scenarios. The underlying nucleosynthesis models need the input of neutron capture cross sections.Purpose: One of the fundamental signatures for active nucleosynthesis in our galaxy is the observation of long-lived radioactive isotopes, such as $^{60}\mathrm{Fe}$ with a half-life of $2.60\ifmmode\times\else\texttimes\fi{}{10}^{6}$ yr. To reproduce this $\ensuremath{\gamma}$ activity in the universe, the nucleosynthesis of $^{60}\mathrm{Fe}$ has to be understood reliably.Methods: An $^{60}\mathrm{Fe}$ sample produced at the Paul Scherrer Institut (Villigen, Switzerla…

PhysicsNuclear and High Energy PhysicsThermal neutron captureResonance7. Clean energyGalaxyNuclear physicsNeutron captureCross section (physics)13. Climate actionNucleosynthesisAtomic physicss-processEnergy (signal processing)Physical Review C
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Thermal (n,γ) cross section and resonance integral ofTm171

2019

PhysicsCross section (physics)010308 nuclear & particles physics0103 physical sciencesThermalAtomic physics010306 general physics01 natural sciencesResonance (particle physics)Physical Review C
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