Search results for "methods"

showing 10 items of 4526 documents

Ab initio modelling of the initial stages of the ODS particle formation process

2018

Abstract Oxide-Dispersion Strengthened (ODS) steels with Y2O3 nanoparticles are promising structural materials for fision and future fusion reactors. A large number of experimental as well as theoretical studies provided valuable information on the ODS particle formation process. However, some important details of this process still remain unexplained. We present the results of ab initio VASP calculations of the initial steps of the ODS particle formation. At these steps Y solute atoms are stabilized in the Fe lattice by vacancies, which create a basis for the future growth of Y2O3-particle. Interaction of multiple vacancies and solution Y and O atoms has been studied in various combination…

Nuclear and High Energy PhysicsStructural materialMaterials scienceAb initioNanoparticle02 engineering and technologyFusion power021001 nanoscience & nanotechnology01 natural sciences7. Clean energyChemical physicsAb initio quantum chemistry methodsLattice (order)0103 physical sciences010306 general physics0210 nano-technologyInstrumentationNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Search for Galactic PeV gamma rays with the IceCube Neutrino Observatory

2013

Gamma-ray induced air showers are notable for their lack of muons, compared to hadronic showers. Hence, air shower arrays with large underground muon detectors can select a sample greatly enriched in photon showers by rejecting showers containing muons. IceCube is sensitive to muons with energies above ~500 GeV at the surface, which provides an efficient veto system for hadronic air showers with energies above 1 PeV. One year of data from the 40-string IceCube configuration was used to perform a search for point sources and a Galactic diffuse signal. No sources were found, resulting in a 90% C.L. upper limit on the ratio of gamma rays to cosmic rays of 1.2 x 10^(-3)for the flux coming from …

Nuclear and High Energy PhysicsTELESCOPEPoint sourcePhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsddc:500.201 natural sciences7. Clean energyIceCube Neutrino ObservatoryIceCubeHESS0103 physical sciencesddc:530MILAGRO010306 general physics010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuonGamma rayAstrophysics::Instrumentation and Methods for AstrophysicsPLANEGalactic planeAir showerPhysics and Astronomy13. Climate actionDISCOVERYMilagroMOLECULAR CLOUDSTEVRADIATIONHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaEMISSION
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Response of the XENON100 dark matter detector to nuclear recoils

2013

Results from the nuclear recoil calibration of the XENON100 dark matter detector installed underground at the Laboratori Nazionali del Gran Sasso (LNGS), Italy are presented. Data from measurements with an external 241AmBe neutron source are compared with a detailed Monte Carlo simulation which is used to extract the energy dependent charge-yield Qy and relative scintillation efficiency Leff. A very good level of absolute spectral matching is achieved in both observable signal channels - scintillation S1 and ionization S2 - along with agreement in the 2-dimensional particle discrimination space. The results confirm the validity of the derived signal acceptance in earlier reported dark matte…

Nuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Cosmology and Nongalactic Astrophysics (astro-ph.CO)[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsMonte Carlo methodDark matterFOS: Physical sciences01 natural sciencesdark matterParticle detectorNuclear physics[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]RecoilIonization0103 physical sciences010306 general physicsNuclear ExperimentInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsScintillation010308 nuclear & particles physicsDetectorAstrophysics::Instrumentation and Methods for Astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Neutron sourceAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics
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The data acquisition system for the ANTARES neutrino telescope

2006

The ANTARES neutrino telescope is being constructed in the Mediterranean Sea. It consists of a large three-dimensional array of photo-multiplier tubes. The data acquisition system of the detector takes care of the digitisation of the photo-multiplier tube signals, data transport, data filtering, and data storage. The detector is operated using a control program interfaced with all elements. The design and the implementation of the data acquisition system are described.

Nuclear and High Energy Physics[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsData managementAstrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONFOS: Physical sciencesAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Data filteringData acquisition0103 physical sciences14. Life underwaterElectronics010306 general physicsInstrumentationdata acquisition system; neutrino telescopeRemote sensingAstroparticle physicsPhysicsneutrino telescope data acquisition system[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics (astro-ph)Astrophysics::Instrumentation and Methods for AstrophysicsAstronomyneutrino telescopedata acquisition systemComputer data storageFísica nuclearbusiness
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Polarimetry at MAMI

2013

Moller and Mott polarimeters have been compared concerning their measurement accuracy in a dedicated "spin dance" experiment. The results obtained with the different polarimeters at vastly different energy ranges were in agreement with each other within the given systematic uncertainties of a few percent. We discuss investigations of background conditions which may allow to reduce this important contribution to the uncertainties in the Mott polarimeter to a value below 1.0%.

Nuclear physicsPhysicsAccuracy and precisionOpticsParticle propertiesbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsPolarimetryCondensed Matter::Strongly Correlated ElectronsPolarimeterbusinessLinear particle acceleratorSpin-½AIP Conference Proceedings
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Cold fusion of heavy ions paving the way to superheavy elements

2001

Abstract Significant progress has been made approaching superheavy elements. A shell-stabilized region near hassium has been discovered. Element 112 has been synthesized. Recently evidence for the creation of elements 114, 116, and 118 has been reported. The way to these superheavy nuclei was paved by the cold fusion of heavy ions. In this paper experimental methods for heavy-element research, which is essentially physics with single atoms, are presented together with recent experimental results. The observed nuclear properties are discussed in the framework of theoretical models. New instrumental developments including accelerators and radioactive beams are be addressed.

Nuclear physicsPhysicsNuclear and High Energy PhysicschemistryTheoretical modelschemistry.chemical_elementSuperheavy ElementsAtomic physicsExperimental methodsHassiumCold fusionIonNuclear Physics A
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Interpretation of the Anomalous NaI Events

2001

Anomalous events, with scintillation decay times shorter than nuclear recoils, have been observed by the UKDMC and Saclay NaI experiments. By using the event categories observed in the EDELWEISS experiment, we propose to interpret the anomalous NaI events as surface nuclear recoils accompanied with a small energy loss of an escaping alpha particle. The discrimination performances of the NaI experiments which have not taken into account these events in their analysis, notably for axial WIMP interactions, must then be reevaluated.

Nuclear physicsPhysicsScintillationEnergy lossWIMPPhysics::Instrumentation and DetectorsAstrophysics::Instrumentation and Methods for AstrophysicsAlpha particleEDELWEISSEvent (particle physics)Interpretation (model theory)
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Simulations of the stopping efficiencies of fission ion guides

2017

With the Ion Guide Isotope Separator On-Line (IGISOL) facility, located at the University of Jyväskylä, products of nuclear reactions are separated by mass. The high resolving power of the JYFLTRAP Penning trap, with full separation of individual nuclides, capacitates the study of nuclides far from the line of stability. For the production of neutron-rich medium-heavy nuclides, fissioning of actinides is a feasible reaction. This can be achieved with protons from an in-house accelerator or, alternatively, with neutrons through the addition of a newly developed Be(p,xn)-converter. The hereby-obtained fission products are used in nuclear data measurements, for example fission yields, nuclear …

Nuclear reactionCold fissionFissionQC1-999Nuclear TheoryFission product yield01 natural sciencesmethodsSubatomär fysikNuclear physicsmenetelmätSubatomic Physics0103 physical sciencesNeutronNuclideNuclear Experiment010306 general physicsFission productsexperimental facilitiesta114010308 nuclear & particles physicsChemistryPhysicsRadiochemistryvarusteettekniikattechniquesLong-lived fission productequipmentEPJ Web of Conferences
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Measurement of the production cross-section of positive pions in the collision of 8.9 GeV/c protons on beryllium

2007

The double-differential production cross-section of positive pions, $d^2\sigma^{\pi^{+}}/dpd\Omega$, measured in the HARP experiment is presented. The incident particles are 8.9 GeV/c protons directed onto a beryllium target with a nominal thickness of 5% of a nuclear interaction length. The measured cross-section has a direct impact on the prediction of neutrino fluxes for the MiniBooNE and SciBooNE experiments at Fermilab. After cuts, 13 million protons on target produced about 96,000 reconstructed secondary tracks which were used in this analysis. Cross-section results are presented in the kinematic range 0.75 GeV/c < $p_{\pi}$ < 6.5 GeV/c and 30 mrad < $\theta_{\pi}$ < 210 mrad in the l…

Nuclear reactionParticle physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics and Astronomy (miscellaneous)HadronFOS: Physical scienceschemistry.chemical_elementddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsMiniBooNEHigh Energy Physics - Experiment (hep-ex)Pion0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Fermilab010306 general physicsNuclear ExperimentEngineering (miscellaneous)PhysicsTime projection chamber010308 nuclear & particles physicsSettore FIS/01 - Fisica Sperimentalecross section particle physicsFísica[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]chemistryHigh Energy Physics::ExperimentBerylliumNeutrinoParticle Physics - Experiment
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Few-body problems in nuclear astrophysics

2005

Few-body methods provide very useful tools to solve different problems important for nuclear astrophysics. Some of them are discussed below.

Nuclear reactionPhysicsNuclear and High Energy PhysicsComputerSystemsOrganization_COMPUTERSYSTEMIMPLEMENTATIONComputingMethodologies_SIMULATIONANDMODELINGNuclear TheoryAstrophysics::Instrumentation and Methods for AstrophysicsNuclear structure8B formation; nuclear reactions; triple collisionsComputerApplications_COMPUTERSINOTHERSYSTEMSFew-body systemsNuclear physicsNuclear astrophysicsNuclear ExperimentJournal of Physics G: Nuclear and Particle Physics
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