0000000000313205

AUTHOR

T. Hensel

showing 3 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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Measurement of the H2(p,γ)He3 S factor at 265–1094 keV

2021

Recent astronomical data have provided the primordial deuterium abundance with percent precision. As a result, big bang nucleosynthesis may provide a constraint on the universal baryon to photon ratio that is as precise as, but independent from, analyses of the cosmic microwave background. However, such a constraint requires that the nuclear reaction rates governing the production and destruction of primordial deuterium are sufficiently well known. Here, a new measurement of the $^{2}\mathrm{H}{(p,\ensuremath{\gamma})}^{3}\mathrm{He}$ cross-section is reported. This nuclear reaction dominates the error on the predicted big bang deuterium abundance. A proton beam of 400--1650 keV beam energy…

PhysicsNuclear reactionProton010308 nuclear & particles physics01 natural sciencesNuclear physicsBaryonDeuteriumBig Bang nucleosynthesis0103 physical sciencesContent (measure theory)Production (computer science)Nuclear Experiment010306 general physicsEnergy (signal processing)Physical Review C
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Measurement of the H2(p,γ)He3 S factor at 265–1094 keV

2021

Recent astronomical data have provided the primordial deuterium abundance with percent precision. As a result, big bang nucleosynthesis may provide a constraint on the universal baryon to photon ratio that is as precise as, but independent from, analyses of the cosmic microwave background. However, such a constraint requires that the nuclear reaction rates governing the production and destruction of primordial deuterium are sufficiently well known. Here, a new measurement of the 2H(p,γ)3He cross-section is reported. This nuclear reaction dominates the error on the predicted big bang deuterium abundance. A proton beam of 400–1650 keV beam energy was incident on solid titanium deuteride targe…

vetyastrofysiikkaalkuräjähdysheliumNuclear Experimentydinfysiikka
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