Search results for "Scintillator"

showing 10 items of 172 documents

Luminescence of divalent lanthanide doped BaBrI single crystal under synchrotron radiation excitations

2020

Abstract Luminescence excitation spectra of BaBrI single crystals doped by divalent lanthanide ions are studied using synchrotron radiation excitations from the MAX IV 1.5 GeV storage ring. The energy of the edge and the formation of core cation exciton as well as the energy threshold of the multiplications of electronic excitations is found. It was clearly established the energy transfer from intrinsic luminescence centers to Sm2+ and Eu2+ ions.

010302 applied physicsLanthanideNuclear and High Energy PhysicsMaterials scienceExcitonDopingSynchrotron radiation02 engineering and technologyScintillator021001 nanoscience & nanotechnology01 natural sciencesMolecular physicsIonCondensed Matter::Materials Science0103 physical sciences0210 nano-technologyLuminescenceInstrumentationSingle crystalNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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Emerging blue-UV luminescence in cerium doped YAG nanocrystals

2016

Physica status solidi / Rapid research letters 10(6), 475 - 479(2016). doi:10.1002/pssr.201600041

010302 applied physicsMaterials sciencebusiness.industryDopingchemistry.chemical_elementSynchrotron radiationPhosphor02 engineering and technologyScintillator021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciences530CeriumchemistryNanocrystal0103 physical sciencesOptoelectronicsGeneral Materials Scienceddc:5300210 nano-technologybusinessLuminescence
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Electron Spin Resonance study of charge trapping in α-ZnMoO4 single crystal scintillator

2015

The origin and properties of electron and hole traps simultaneously appearing in a-ZnMoO4 scintillator after X-ray irradiation at low temperatures (T < 35 K) were studied by Electron Spin Resonance (ESR). ESR spectrum of the electron type trap shows pronounced superhyperfine structure due to the interaction of electron spin with nuclear magnetic moments of 95,97Mo and 67Zn lattice nuclei. Considering the nearly tetragonal symmetry of the center this allows us to identify the electron trap as an electron self-trapped at the (Mo(1)O4) 2 complex. Nearly 60% reduction of the spin–orbit coupling at the Mo(1) ion is caused by the overlap of the Mo and ligand oxygen orbitals indicating an essentia…

02 engineering and technologyElectronCharge trapsElectron Spin Resonance010402 general chemistry01 natural sciencesIonlaw.inventionInorganic ChemistryDelocalized electronTetragonal crystal systemAtomic orbitallawElectrical and Electronic EngineeringPhysical and Theoretical ChemistryElectron paramagnetic resonanceSpectroscopyZinc molybdateChemistryOrganic ChemistryScintillator021001 nanoscience & nanotechnologyAtomic and Molecular Physics and Optics0104 chemical sciencesElectronic Optical and Magnetic MaterialsCrystal field theoryAtomic physics0210 nano-technologySingle crystalOptical Materials
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Topological track reconstruction in unsegmented, large-volume liquid scintillator detectors

2018

Unsegmented, large-volume liquid scintillator (LS) neutrino detectors have proven to be a key technology for low-energy neutrino physics. The efficient rejection of radionuclide background induced by cosmic muon interactions is of paramount importance for their success in high-precision MeV neutrino measurements. We present a novel technique to reconstruct GeV particle tracks in LS, whose main property, the resolution of topological features and changes in the differential energy loss $\mathrm{d}E/\mathrm{d}x$, allows for improved rejection strategies. Different to common track reconstruction approaches, our method does not rely on concrete track / topology hypotheses. Instead, based on a r…

Astroparticle physicsPhysicsPhysics - Instrumentation and DetectorsPhotonMuonPhysics::Instrumentation and Detectors010308 nuclear & particles physicsDetectorFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)ScintillatorTopology01 natural sciencesNeutrino detector0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsInstrumentationImage resolutionMathematical PhysicsJournal of Instrumentation
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Position-sensitive neutron detector

2002

Abstract A position-sensitive neutron detector has been developed for use in nuclear physics research. The detector consists of a ∅5.5 cm×100 cm long quartz tube filled with liquid scintillator viewed from both ends by photomultipliers and enclosed in a light-tight titanium container. The properties of the detector were determined both experimentally and by Monte Carlo simulations (EFEN code). A time resolution of 0.4 ns was reached resulting in the position resolution of less than 4 cm. The neutron registration efficiency varies from 36% to 20% within neutron energy range 1–10 MeV and is practically independent of the position along the detector length. Good n–γ separation is achieved for …

Bonner spherePhysicsNuclear and High Energy PhysicsPhotomultiplierPhysics::Instrumentation and Detectorsbusiness.industryNuclear TheoryMonte Carlo methodDetectorScintillatorNeutron temperatureNuclear physicsOpticsNeutron detectionNeutronNuclear ExperimentbusinessInstrumentationNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Perspectives for CNO neutrino detection in Borexino

2018

International audience; Borexino measured with unprecedented accuracy the fluxes of solar neutrinos emitted at all the steps of the pp fusion chain. Still missing is the measurement of the flux of neutrinos produced in the CNO cycle. A positive measurement of the CNO neutrino flux is of fundamental importance for understanding the evolution of stars and addressing the unresolved controversy on the solar abundances. The measurement of the CNO neutrino flux in Borexino is challenging because of the low intensity of this component (CNO cycle accounts for about 1% of the energy emitted by Sun), the lack of prominent spectral features and the presence of background sources. The main background c…

CNO cycleexperimental methodsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical Phenomenascintillation counter: liquidSolar neutrinosbismuth: admixtureAstrophysics[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energySolar neutrinoCNO-cycleneutrino: fluxAstrophysics::Solar and Stellar Astrophysics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Stellar evolutionBorexinoliquid scintillatorAstrophysics::Galaxy AstrophysicsPhysicsEnergy distributiondetectorbackgroundbismuth: nuclideCNO cycleNeutrino detector13. Climate actionBorexinoExperimental methodsNeutrino
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Rayleigh scattering of linear alkylbenzene in large liquid scintillator detectors.

2015

Rayleigh scattering poses an intrinsic limit for the transparency of organic liquid scintillators. This work focuses on the Rayleigh scattering length of linear alkylbenzene (LAB), which will be used as the solvent of the liquid scintillator in the central detector of the Jiangmen Underground Neutrino Observatory. We investigate the anisotropy of the Rayleigh scattering in LAB, showing that the resulting Rayleigh scattering length will be significantly shorter than reported before. Given the same overall light attenuation, this will result in a more efficient transmission of photons through the scintillator, increasing the amount of light collected by the photosensors and thereby the energy…

Chemical Physics (physics.chem-ph)PhysicsPhysics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorsbusiness.industryAttenuationDetectorFOS: Physical sciencesPhotodetectorScattering lengthInstrumentation and Detectors (physics.ins-det)ScintillatorHigh Energy Physics - ExperimentPhysics::Fluid DynamicsHigh Energy Physics - Experiment (hep-ex)symbols.namesakeOpticsPhysics - Chemical PhysicsScintillation countersymbolsRayleigh scatteringbusinessInstrumentationJiangmen Underground Neutrino ObservatoryThe Review of scientific instruments
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&lt;title&gt;Photostimulated recombination processes in x-irradiated CsCdF&lt;formula&gt;&lt;inf&gt;&lt;roman&gt;3&lt;/roman&gt;&lt;/inf&gt;&lt;/form…

2005

Fluoride crystals with the perovskite structure doped with rare-earth ions and other activators are interesting materials for laser hosts, scintillators, and detectors of ionizing radiation. Therefore, an actual task is to clarify the structure of the radiation-induced defects and recombination processes in these crystals. Compared to other fluoroperovskites, considerably less information is available concerning to the radiation-induced processes in the CsCdF3 crystals. We present a study of photostimulated luminescence (PSL) in the previously x-irradiated CsCdF3 crystal doped with Mn (0.05%). After the x-irradiation of the crystal, optical stimulation at 320 nm leads to the appearance of 3…

CrystalChemistryPhotostimulated luminescenceInorganic chemistryDopingAnalytical chemistryIrradiationScintillatorLuminescencePerovskite (structure)IonSPIE Proceedings
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Observations of Forbush Decreases of cosmic ray electrons and positrons with the Dark Matter Particle Explorer

2021

The Forbush Decrease (FD) represents the rapid decrease of the intensities of charged particles accompanied with the coronal mass ejections (CMEs) or high-speed streams from coronal holes. It has been mainly explored with ground-based neutron monitors network which indirectly measure the integrated intensities of all species of cosmic rays by counting secondary neutrons produced from interaction between atmosphere atoms and cosmic rays. The space-based experiments can resolve the species of particles but the energy ranges are limited by the relative small acceptances except for the most abundant particles like protons and helium. Therefore, the FD of cosmic ray electrons and positrons have …

Dark Matter cosmic raysAstrophysics::High Energy Astrophysical PhenomenaDark matterCoronal holeFOS: Physical sciencesCosmic rayAstrophysicsdisturbancesCoronal mass ejectionForbush decreaseNeutronplastic scintillator detectorPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Neutron monitordriftSettore FIS/01 - Fisica SperimentaleAstronomy and AstrophysicsdependenceForbush decrease cosmic rayscalibrationsolarCharged particlemodulationSpace and Planetary SciencetransportPhysics::Space PhysicsintensityAstrophysics - High Energy Astrophysical Phenomenaenergy
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Electron paramagnetic resonance study of exchange coupled Ce3+ ions in Lu2SiO5 single crystal scintillator

2016

Abstract The Ce 3+ ions incorporation inside lutetium oxyorthosilicate (Lu 2 SiO 5 ) single crystals was studied by electron paramagnetic resonance. Already known Ce1 and Ce2 centers originating from the lattice peculiarity allowing two lutetium sites coordinated by different number of the oxygen ions were detected. Remarkably, for the Ce2 center, the determined g 2 tensor is asymmetric and could not be diagonalized as compared to the Ce1 center, for which the three principal values and corresponding axes orientation have been determined and reported previously. Besides, the much weaker resonance lines found in spectra close to those coming from the Ce1 and Ce2, and following them under cry…

Dimerchemistry.chemical_element02 engineering and technology01 natural sciencesSpectral linelaw.inventionIonchemistry.chemical_compoundlaw0103 physical sciencesExchange coupled ionsLutetium oxyorthosilicateElectron paramagnetic resonanceInstrumentationCoupling constantRadiation010308 nuclear & particles physics021001 nanoscience & nanotechnologyLutetiumMagnetic fieldchemistryScintillatorsElectron paramagnetic resonanceAtomic physicsCerium ions0210 nano-technologySingle crystalRadiation Measurements
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