Search results for "astro nuclear physics"

showing 3 items of 3 documents

New accurate measurements of neutron emission probabilities for relevant fission products

2017

We have performed new accurate measurements of the beta-delayed neutron emission probability for ten isotopes of the elements Y, Sb, Te and I. These are fission products that either have a significant contribution to the fraction of delayed neutrons in reactors or are relatively close to the path of the astrophysical r process. The measurements were performed with isotopically pure radioactive beams using a constant and high efficiency neutron counter and a low noise beta detector. Preliminary results are presented for six of the isotopes and compared with previous measurements and theoretical calculations. peerReviewed

Neutron emissionQC1-999Nuclear physicsNeutronAstrophysics7. Clean energy01 natural sciencesNuclear physics0103 physical sciencesNeutron010306 general physicsNuclear Experimentastro nuclear physicsPhysicsNeutrons:Energies::Energia nuclear [Àrees temàtiques de la UPC]Fission productsPnta114Isotope:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsDetectorBeta (plasma physics)r-processFísica nuclearDelayed neutronNeutron emission
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Measurement of the heaviest Beta-delayed 2-neutron emitter: 136Sb

2017

The Beta-delayed neutron emission probability, Pn , of very exotic nuclei is crucial for the understanding of nuclear structure properties of many isotopes and astrophysical processes such as the rapid neutron capture process (r-process). In addition Beta-delayed neutrons are important in a nuclear power reactor operated in a prompt sub-critical, delayed critical condition, as they contribute to the decay heat inducing fission reactions after a shut down. The study of neutron-rich isotopes and the measurement of Beta-delayed one-neutron emitters (Beta1n) is possible thanks to the Rare Isotope Beam (RIB) facilities, where radioactive beams allow the production of exotic nuclei of interest, w…

FissionNeutron emissionQC1-999Astrophysics::High Energy Astrophysical PhenomenaNuclear TheoryNuclear physicsNeutronAstrophysics7. Clean energy01 natural sciencesNuclear physicsEmission0103 physical sciencesNeutronDecay heat010306 general physicsNuclear Experimentastro nuclear physicsPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsPnIsotopeta114:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsBranching fractionPhysicsNeutron capture13. Climate actionr-processPhysics::Accelerator PhysicsFísica nuclearAtomic physics
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Strong γ-ray emission from neutron unbound states populated in β-decay: Impact on (n,γ) cross-section estimates

2017

J. L. Taín et al. -- 6 pags., 7 figs., 1 tab. -- Open Access funded by Creative Commons Atribution Licence 4.0

Physicsta114010308 nuclear & particles physicsBranching fractionNeutron emissionAstrophysics::High Energy Astrophysical PhenomenaPhysicsQC1-999Nuclear Theory7. Clean energy01 natural sciences3. Good health0103 physical sciencesr-processNeutronAtomic physics010306 general physicsSpectroscopyNucleonNuclear ExperimentDelayed neutronRadioactive decayastro nuclear physics
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