0000000000181652

AUTHOR

Christoph Langer

showing 19 related works from this author

Exclusive measurements of nuclear breakup reactions of 17Ne

2014

F. Wamers et al.; 4 pags.; 2 figs. Open Access funded by Creative Commons Atribution Licence 2.0

Nuclear reactionPhysicsIsotopePhysicsQC1-999HadronNuclear Theorychemistry.chemical_elementBreakup530Nuclear physicsBaryonchemistryIsotopes of neonPhysics::Accelerator Physicsddc:530Statistical physicsNucleonNuclear ExperimentCarbon
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Comparison of electromagnetic and nuclear dissociation of Ne-17

2018

8 pags., 10 figs., 3 tabs.

PhysicsCOLLISIONSInternal energy010308 nuclear & particles physics01 natural sciences7. Clean energySTATEDissociation (chemistry)CoincidenceCAPTUREReaction ratemedicine.anatomical_structureFragmentation (mass spectrometry)0103 physical sciencesmedicineHaloAtomic physics010306 general physicsGround stateDECAYNucleus
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Thermonuclear reactionS30(p,γ)Cl31studied via Coulomb breakup ofCl31

2014

Coulomb breakup at high energy in inverse kinematics of proton-rich Cl-31 was used to constrain the thermonuclear S-30(p,gamma)Cl-31 capture reaction rate under typical Type I x-ray burst conditions. This reaction is a bottleneck during rapid proton-capture nucleosynthesis (rp process), where its rate depends predominantly on the nuclear structure of Cl-31. Two low-lying states just above the proton-separation threshold of S-p = 296( 50) keV in Cl-31 have been identified experimentally using the (RB)-B-3-LAND setup at the GSI Helmholtzzentrum fur Schwerionenforschung GmbH. Both states are considered to play a key role in the thermonuclear S-30( p,gamma)Cl-31 capture reaction. Excitation ene…

PhysicsNuclear physicsReaction rateNuclear and High Energy PhysicsThermonuclear fusionProtonNucleosynthesisNuclear structureCoulomb excitationAtomic physicsrp-processExcitationPhysical Review C
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Determination of the Bi209(n,γ)Bi210g cross section using the NICE detector

2021

The capture cross section of $^{209}\mathrm{Bi}(n,\ensuremath{\gamma})^{210g}\mathrm{Bi}$ was measured at different astrophysically relevant energies including thermal capture cross section (25 meV), resonance integral, and the Maxwellian averaged cross section at a thermal energy of $kT=30$ keV. The partial capture cross section $({\ensuremath{\sigma}}_{g})$ was determined using the activation technique and by measuring the $^{210}\mathrm{Po}$ activity. The newly developed and tested NICE detector setup was used to measure the $\ensuremath{\alpha}$ activity of the $^{210}\mathrm{Po}$. Using this setup the thermal and resonance integral cross sections were determined to be $16.2\phantom{\ru…

PhysicsCross section (physics)Activation techniqueResonanceAtomic physicsPhysical Review C
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Measurement of the92,93,94,100Mo(γ,n) reactions by Coulomb Dissociation

2016

6th Nuclear Physics in Astrophysics Conference (NPA), Lisbon, Portugal, 19 May 2013 - 24 May 2013; Journal of physics / Conference Series 665, 012034 (2016). doi:10.1088/1742-6596/665/1/012034

PhysicsHistoryPhoton010504 meteorology & atmospheric sciencesIsotopeStable isotope ratiochemistry.chemical_element53001 natural sciencesDissociation (chemistry)Computer Science ApplicationsEducationNuclear physicschemistryNucleosynthesisMolybdenum0103 physical sciencesCoulombddc:530Atomic physics010303 astronomy & astrophysicsProduction chain0105 earth and related environmental sciencesJournal of Physics: Conference Series
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Neutron capture cross section measurement ofU238at the CERN n_TOF facility in the energy region from 1 eV to 700 keV

2017

The aim of this work is to provide a precise and accurate measurement of the U238(n,γ) reaction cross section in the energy region from 1 eV to 700 keV. This reaction is of fundamental importance for the design calculations of nuclear reactors, governing the behavior of the reactor core. In particular, fast reactors, which are experiencing a growing interest for their ability to burn radioactive waste, operate in the high energy region of the neutron spectrum. In this energy region most recent evaluations disagree due to inconsistencies in the existing measurements of up to 15%. In addition, the assessment of nuclear data uncertainty performed for innovative reactor systems shows that the u…

Physics010308 nuclear & particles physicsGamma rayNuclear dataScintillator7. Clean energy01 natural sciencesResonance (particle physics)Nuclear physicsNeutron captureNuclear reactor core0103 physical sciencesNeutron cross sectionNeutron010306 general physicsPhysical Review C
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The Nuclear astrophysics program at n_TOF (CERN)

2017

An important experimental program on Nuclear Astrophysics is being carried out at the n_TOF since several years, in order to address the still open issues in stellar and primordial nucleosynthesis. Several neutron capture reactions relevant to s-process nucleosynthesis have been measured so far, some of which on important branching point radioisotopes. Furthermore, the construction of a second experimental area has recently opened the way to challenging measurements of (n, charged particle) reactions on isotopes of short half-life. The Nuclear Astrophysics program of the n_TOF Collaboration is here described, with emphasis on recent results relevant for stellar nucleosynthesis, stellar neut…

Nuclear reactionAstrofísicaAstrophysics and AstronomyCross-sectionnTOFQC1-999Astrophysics::High Energy Astrophysical PhenomenaNeutron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Astrophysics01 natural sciences7. Clean energyn_TOF nuclear astrophysics CERNNuclear physicsPhysics and Astronomy (all)Stellar nucleosynthesisBig Bang nucleosynthesisNucleosynthesis0103 physical sciencesCERNNuclear astrophysicsAstrophysics::Solar and Stellar AstrophysicsNuclear Physics - ExperimentNeutronNeutron induced nuclear reactions010306 general physicsNuclear ExperimentAstrophysics::Galaxy AstrophysicsPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]Neutrons:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsNuclear reactionNeutron capture13. Climate actionNeutron sourceAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]NucleosynthesisNucleosíntesi
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Study of the $^{15}$O(2p, γ )$^{17}$Ne cross section by Coulomb dissociation of $^{17}$Ne for the rp process of nucleosynthesis

2014

Acta physica Polonica / B 45(2), 229 - 234 (2014). doi:10.5506/APhysPolB.45.229

PhysicsRadiative captureNuclear structureGeneral Physics and AstronomySigma25.40.Lw 25.70.De 26.30.Ca 27.20.+nrp-process[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]530Dissociation (chemistry)Nuclear physicsNucleosynthesisTheoryofComputation_ANALYSISOFALGORITHMSANDPROBLEMCOMPLEXITYCoulombddc:530Atomic physicsExcitationComputingMilieux_MISCELLANEOUS
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Experimental study of the 15O(2p, γ)17Ne cross section by Coulomb Dissociation for the rp process

2016

6th Nuclear Physics in Astrophysics Conference (NPA), Lisbon, Portugal, 19 May 2013 - 24 May 2013; Journal of physics / Conference Series 665, 012046 (2016). doi:10.1088/1742-6596/665/1/012046

HistoryChemistryNuclear structurechemistry.chemical_elementrp-process[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]530Dissociation (chemistry)Computer Science ApplicationsEducationIonSubatomär fysikFragmentation (mass spectrometry)Subatomic PhysicsCoulombNuclear Physics - ExperimentBerylliumAtomic physicsNuclear Experiment[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Excitation
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Nuclear Data for the Thorium Fuel Cycle and the Transmutation of Nuclear Waste

2016

Neutron-induced reaction cross sections play an important role in a wide variety of research fields, ranging from stellar nucleosynthesis, the investigation of nuclear level density studies, to applications of nuclear technology, including the transmutation of nuclear waste, accelerator-driven systems, and nuclear fuel cycle investigations. Simulations of nuclear technology applications largely rely on evaluated nuclear data libraries. These libraries are based both on experimental data and theoretical models. An outline of experimental nuclear data activities at CERN’s neutron time-of-flight facility, n_TOF, will be presented.

Nuclear fuel cycleNuclear technologyStellar nucleosynthesisNuclear transmutationChemistryNuclear engineeringNuclear TheoryRadioactive wasteNuclear dataNeutronNuclear ExperimentThorium fuel cycle
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The 236U neutron capture cross-section measured at the n TOF CERN facility

2016

International audience; The $^{236}$U isotope plays an important role in nuclear systems, both for future and currently operating ones. The actual knowledge of the capture reaction of this isotope is satisfactory in the thermal region, but it is considered insufficient for Fast Reactor and ADS applications. For this reason the $^{236} \text{U}(n, \gamma)$ reaction cross-section has been measured for the first time in the whole energy region from thermal energy up to 1 MeV at the n_TOF facility with two different detection systems: an array of C$_6$D$_6$ detectors, employing the total energy deposited method, and a 4$\pi$ total absorption calorimeter (TAC), made of 40 BaF$_2$ crystals. The t…

Nuclear reactionnTOFQC1-999Neutron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyNuclear physicsPhysics and Astronomy (all)Cross section (physics)0103 physical sciencesCERNNeutron cross sectionNuclear Physics - Experimentddc:530Neutron010306 general physicsAbsorption (electromagnetic radiation)PhysicsNeutrons:Energies::Energia nuclear [Àrees temàtiques de la UPC]IsotopeCross sectionReaccions nuclears:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsResonanceNuclear reactionCalorimeter13. Climate actionNuclear reactions
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High precision measurement of the radiative capture cross section of 238U at the n_TOF CERN facility

2016

The importance of improving the accuracy on the capture cross-section of 238U has been addressed by the Nuclear Energy Agency, since its uncertainty significantly affects the uncertainties of key design parameters for both fast and thermal nuclear reactors. Within the 7th framework programme ANDES of the European Commission three different measurements have been carried out with the aim of providing the 238U(n,γ) cross-section with an accuracy which varies from 1 to 5%, depending on the energy range. Hereby the final results of the measurement performed at the n-TOF CERN facility in a wide energy range from 1 eV to 700 keV will be presented. © The Authors, published by EDP Sciences, 2017.

Nuclear reactionnTOFQC1-999Neutron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyNuclear physicsCross section (physics)Physics and Astronomy (all)Nuclear reactorsReactors nuclears0103 physical sciencesThermalCERNNeutronddc:530Nuclear Physics - Experiment010306 general physicsPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsRange (particle radiation)Large Hadron Collider:Física [Àrees temàtiques de la UPC]Cross section010308 nuclear & particles physicsPhysicsRadiative captureNuclear energyNuclear reactionEnergia nuclearEnergy (signal processing)
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Fission fragment angular distribution of 232Th(n,f) at the CERN n TOF facility

2014

The angular distribution of fragments emitted in neutron-induced fission of 232Th was measured in the white spectrum neutron beam at the n_TOF facility at CERN. A reaction chamber based on Parallel Plate Avalanche Counters (PPAC) was used, where the detectors and the targets have been tilted 45 degrees with respect to the neutron beam direction in order to cover the full angular range of the fission fragments. A GEANT4 simulation has been developed to study the setup efficiency. The data analysis and the preliminary results obtained for the 232Th(n,f) between fission threshold and 100 MeV are presented here.

PhysicsNuclear reaction:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsNuclear and High Energy PhysicsLarge Hadron Collidercross sectionFragment (computer graphics)FissionPhysics::Instrumentation and DetectorsNuclear TheoryTOFNuclear data232Th; n_TOF; fission fragments; angular distributionNuclear physicsCross section (physics)Angular distributionneutronPhysics::Accelerator PhysicsfissionNeutronNuclear Experimentnuclear reactions
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Coulomb dissociation of P 27 at 500 MeV/u

2016

J. Marganiec et al. ; 15 págs.; 14 figs.; 6 tabs.

Physics010308 nuclear & particles physicsS-factorMonte Carlo methodNuclear structureResonance[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesDissociation (chemistry)Intruder stateNuclear physics0103 physical sciencesCoulombAtomic physics010306 general physicsNuclear ExperimentExcitation
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First Observation of the Unbound NucleusNe15

2014

We report on the first observation of the unbound proton-rich nucleus Ne-15. Its ground state and first excited state were populated in two-neutron knockout reactions from a beam of 500 MeV/u Ne-17. The Ne-15 ground state is found to be unbound by 2.522(66) MeV. The decay proceeds directly to O-13 with simultaneous two-proton emission. No evidence for sequential decay via the energetically allowed 2(-) and 1(-) states in F-14 is observed. The Ne-15 ground state is shown to have a strong configuration with two protons in the (sd) shell around O-13 with a 63(5)% (1s(1/2))(2) component.

Physicsmedicine.anatomical_structureExcited stateNuclear TheorymedicineShell (structure)Physics::Accelerator PhysicsGeneral Physics and AstronomyAtomic physicsNuclear ExperimentGround stateNucleusBeam (structure)Physical Review Letters
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Measurement of the 241Am neutron capture cross section at the n-TOF facility at CERN

2016

New neutron cross section measurements of minor actinides have been performed recently in order to reduce the uncertainties in the evaluated data, which is important for the design of advanced nuclear reactors and, in particular, for determining their performance in the transmutation of nuclear waste. We have measured the 241 Am(n,γ) cross section at the n TOF facility between 0.2 eV and 10 keV with a BaF2 Total Absorption Calorimeter, and the analysis of the measurement has been recently concluded. Our results are in reasonable agreement below 20 eV with the ones published by C. Lampoudis et al. in 2013, who reported a 22% larger capture cross section up to 110 eV compared to experimental …

Nuclear reactionNuclear transmutationnTOFQC1-999Neutron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyNuclear physicsPhysics and Astronomy (all)Cross section (physics)Nuclear reactorsReactors nuclears0103 physical sciencesCERNNeutron cross sectionNuclear Physics - Experimentddc:530Neutron010306 general physicsAbsorption (electromagnetic radiation)PhysicsNeutrons:Energies::Energia nuclear [Àrees temàtiques de la UPC]Large Hadron ColliderCross section:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsNuclear reactionCalorimeter
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Coulomb and nuclear excitations of narrow resonances in 17Ne

2016

Physics letters / B 759, 200 - 205 (2016). doi:10.1016/j.physletb.2016.05.073

PhysicsNuclear and High Energy PhysicsTeoría de los quantaInternal energySpins010308 nuclear & particles physicsProjectile310601 natural sciences530lcsh:QC1-999Mass formulaNuclear physics0103 physical sciencesPhysical SciencesCoulombIsobaric processFysikddc:530Atomic physics010306 general physicsMultipletExcitationlcsh:PhysicsPhysics Letters B
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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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Unveiling the two-proton halo character of 17Ne: Exclusive measurement of quasi-free proton-knockout reactions

2022

7 pags., 5 figs.

Subatomär fysikNuclear and High Energy PhysicsFísica-Modelos matemáticosSubatomic PhysicsNuclear TheoryPartículasFOS: Physical sciencesddc:530Nuclear Experiment (nucl-ex)Nuclear experimentNuclear ExperimentNuclear Experiment530
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