Search results for " LAB"

showing 10 items of 2393 documents

Gamma Ray Spectrum from Thermal Neutron Capture on Gadolinium-157

2018

International audience; We have measured the |$\gamma$|-ray energy spectrum from the thermal neutron capture, |${}^{157}$|Gd|$(n,\gamma)$|⁠, on an enriched |$^{157}$|Gd target (Gd|$_{2}$|O|$_{3}$|⁠) in the energy range from 0.11 MeV up to about 8 MeV. The target was placed inside the germanium spectrometer of the ANNRI detector at J-PARC and exposed to a neutron beam from the Japan Spallation Neutron Source (JSNS). Radioactive sources (⁠|$^{60}$|Co, |$^{137}$|Cs, and |$^{152}$|Eu) and the |$^{35}$|Cl(⁠|$n$|⁠,|$\gamma$|⁠) reaction were used to determine the spectrometer‘s detection efficiency for |$\gamma$| rays at energies from 0.3 to 8.5 MeV. Using a Geant4-based Monte Carlo simulation of …

PhotonPhysics - Instrumentation and DetectorsMonte Carlo methodGeneral Physics and Astronomy7. Clean energy01 natural sciencesnuclear reactionSpectral lineHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)H43 Software architectures[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]n: fissionNuclear Experiment (nucl-ex)n: captureNuclear ExperimentNuclear ExperimentPhysicsdensityJ-PARC LabphotonGamma rayInstrumentation and Detectors (physics.ins-det)Atomic physicsnumerical calculations: Monte CarloSpallation Neutron SourceNeutron captureAstrophysics::High Energy Astrophysical Phenomenaenergy spectrumchemistry.chemical_elementFOS: Physical sciencesGermanium[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]n: thermalF20 Instrumentation and technique0103 physical sciencesModels of nuclear reactions[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutron capture gamma ray cascade Models of nuclear reactions Neutrinos from supernova remnant010306 general physicsD21 Models of nuclear reactionsgamma ray cascadeSpectrometer010308 nuclear & particles physicsnucleusNeutron radiationH20 Instrumentation for underground experiments* Automatic Keywords *germaniumF22 Neutrinos from supernova remnant and other astronomical objectschemistryn: beamNeutrinos from supernova remnantefficiencygamma rayspectrometerC43 Underground experimentsgadolinium
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Atomic physics studies at the gamma factory at CERN

2020

The Gamma Factory initiative proposes to develop novel research tools at CERN by producing, accelerating and storing highly relativistic, partially stripped ion beams in the SPS and LHC storage rings. By exciting the electronic degrees of freedom of the stored ions with lasers, high-energy narrow-band photon beams will be produced by properly collimating the secondary radiation that is peaked in the direction of ions' propagation. Their intensities, up to $10^{17}$ photons per second, will be several orders of magnitude higher than those of the presently operating light sources in the particularly interesting $\gamma$--ray energy domain reaching up to 400 MeV. This article reviews opportuni…

Photonradiation: secondaryAtomic Physics (physics.atom-ph)atomic spectroscopyGeneral Physics and Astronomy02 engineering and technology01 natural sciences7. Clean energyPhysics - Atomic PhysicsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)propagation[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]particle sourcePhysicsLarge Hadron Collidercollimatorhep-phsecondary beam021001 nanoscience & nanotechnologyion: excited stateLHC storage ringsHigh Energy Physics - PhenomenologyCERN LHC CollSPS storage rings0210 nano-technologyParticle Physics - ExperimentAccelerator Physics (physics.acc-ph)CERN LabOrders of magnitude (temperature)[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]gamma–ray productionOther Fields of PhysicsFOS: Physical sciencesAtomic spectroscopyion: beamgamma ray: burstpartially stripped ionsphysics.atom-phIonNuclear physics0103 physical sciencesddc:530010306 general physicsSpectroscopyphoton: beamphysics.acc-phParticle Physics - PhenomenologyAccelerator physicsparticle source: proposedhep-exCERN SPSAccelerators and Storage Rings[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]laser* Automatic Keywords *ion: storage ringatomic physics[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Physics::Accelerator PhysicsPhysics - Accelerator PhysicsStorage ring
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Photoreceptor vitality in organotypic cultures of mature vertebrate retinas validated by light-dependent molecular movements

2006

AbstractVertebrate photoreceptor cells are polarized neurons highly specialized for light absorption and visual signal transduction. Photoreceptor cells consist of the light sensitive outer segment and the biosynthetic active inner segment linked by a slender connecting cilium. The function of mature photoreceptor cells is strictly dependent on this compartmentalization which is maintained in the specialized retinal environment. To keep this fragile morphologic and functional composition for further cell biological studies and treatments we established organotypic retina cultures of mature mice and Xenopus laevis. The organotypic retina cultures of both model organisms are created as co-cul…

Photoreceptorsgenetic structuresMouseXenopusCellved/biology.organism_classification_rank.speciesXenopusGene deliverySignal transductionRetinaMicechemistry.chemical_compoundOrgan Culture TechniquesOrganotypic retina cultureIn Situ Nick-End LabelingmedicineAnimalsPhotoreceptor CellsTransducinModel organismVision OcularRetinaArrestinbiologyved/biologyRetinalbiology.organism_classificationLight-dependent movementsSensory Systemseye diseasesCell biologyMice Inbred C57BLProtein TransportOphthalmologymedicine.anatomical_structureMicroscopy FluorescencechemistryCell cultureVertebratesTransducinsense organsPhotic StimulationVision Research
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Dependence of polytetrafluoroethylene reflectance on thickness at visible and ultraviolet wavelengths in air

2020

[EN] Polytetrafluoroethylene (PTFE) is an excellent diffuse reflector widely used in light collection systems for particle physics experiments. However, the reflectance of PTFE is a function of its thickness. In this work, we investigate this dependence in air for light of wavelengths 260 nm and 450 nm using two complementary methods. We find that PTFE reflectance for thicknesses from 5 mm to 10 mm ranges from 92.5% to 94.5% at 450 nm, and from 90.0% to 92.0% at 260 nm We also see that the reflectance of PIFE of a given thickness can vary by as much as 2.7% within the same piece of material. Finally, we show that placing a specular reflector behind the PTFE can recover the loss of reflectan…

Physics - Instrumentation and DetectorsFOS: Physical sciencesLibrary science7. Clean energy01 natural sciences030218 nuclear medicine & medical imagingSynthetic materialsTECNOLOGIA ELECTRONICA03 medical and health sciences0302 clinical medicinePolitical science0103 physical sciencesmedia_common.cataloged_instanceEuropean unionInstrumentationUltraviolet radiationMathematical Physicsmedia_common010308 nuclear & particles physicsEuropean researchTime projection Chambers (TPC)Instrumentation and Detectors (physics.ins-det)Visible radiationDouble-beta decay detectorsReflectivityDetector design and construction technologies and materialsNational laboratory
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Gamma Ray Spectra from Thermal Neutron Capture on Gadolinium-155 and Natural Gadolinium

2019

Natural gadolinium is widely used for its excellent thermal neutron capture cross section, because of its two major isotopes: $^{\rm 155}$Gd and $^{\rm 157}$Gd. We measured the $\gamma$-ray spectra produced from the thermal neutron capture on targets comprising a natural gadolinium film and enriched $^{\rm 155}$Gd (in Gd$_{2}$O$_{3}$ powder) in the energy range from 0.11 MeV to 8.0 MeV, using the ANNRI germanium spectrometer at MLF, J-PARC. The freshly analysed data of the $^{\rm 155}$Gd(n, $\gamma$) reaction are used to improve our previously developed model (ANNRI-Gd model) for the $^{\rm 157}$Gd(n, $\gamma$) reaction, and its performance confirmed with the independent data from the $^{\r…

Physics - Instrumentation and DetectorsGadoliniumMonte Carlo methodAnalytical chemistryenergy spectrumGeneral Physics and Astronomychemistry.chemical_elementFOS: Physical sciencesGermanium[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]n: thermal7. Clean energy01 natural sciencesSpectral lineHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)F20 Instrumentation and technique0103 physical sciencesH43 Software architectures[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)n: capture010306 general physicsNuclear ExperimentMonte CarloPhysicsD21 Models of nuclear reactionsIsotopeSpectrometer010308 nuclear & particles physicsJ-PARC LabGamma rayInstrumentation and Detectors (physics.ins-det)Gadolinium neutron capture gamma ray cascadeNeutron temperature3. Good healthparticle: interactionH20 Instrumentation for underground experimentsgermaniumF22 Neutrinos from supernova remnant and other astronomical objectsC42 Reactor experimentschemistrygamma rayC43 Underground experimentsspectrometergadoliniumperformance
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Cosmic-ray muon flux at Canfranc Underground Laboratory

2019

Residual flux and angular distribution of high-energy cosmic muons have been measured in two underground locations at the Canfranc Underground Laboratory (LSC) using a dedicated Muon Monitor. The instrument consists of three layers of fast scintillation detector modules operating as 352 independent pixels. The monitor has flux-defining area of 1 m${}^{2}$, covers all azimuth angles, and zenith angles up to $80^\circ$. The measured integrated muon flux is $(5.26 \pm 0.21) \times 10^{-3}$ m${}^{-2}$s${}^{-1}$ in the Hall A of the LAB2400 and $(4.29 \pm 0.17) \times 10^{-3}$ m${}^{-2}$s${}^{-1}$ in LAB2500. The angular dependence is consistent with the known profile and rock density of the sur…

Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsFOS: Physical sciencesFluxlcsh:AstrophysicsCosmic rayApplied Physics (physics.app-ph)hiukkasfysiikkaScintillator01 natural sciencesNuclear physicslcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010303 astronomy & astrophysicsEngineering (miscellaneous)ZenithPhysicsMuon010308 nuclear & particles physicsCanfranc Underground LaboratoryPhysics - Applied PhysicsInstrumentation and Detectors (physics.ins-det)Azimuthilmaisimethigh-energy cosmic muonsMuon fluxlcsh:QC770-798High Energy Physics::Experimentkosminen säteily
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A 4 tonne demonstrator for large-scale dual-phase liquid argon time projection chambers

2018

A 10 kilo-tonne dual-phase liquid argon TPC is one of the detector options considered for the Deep Underground Neutrino Experiment (DUNE). The detector technology relies on amplification of the ionisation charge in ultra-pure argon vapour and offers several advantages compared to the traditional single-phase liquid argon TPCs. A 4.2 tonne dual-phase liquid argon TPC prototype, the largest of its kind, with an active volume of \three has been constructed and operated at CERN. In this paper we describe in detail the experimental setup and detector components as well as report on the operation experience. We also present the first results on the achieved charge amplification, prompt scintillat…

Physics - Instrumentation and DetectorsPhysics::Instrumentation and Detectorshiukkasfysiikka01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNeutrino detectorHigh Energy Physics - Experiment (hep-ex)Ionization[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino detectorsDetectors and Experimental TechniquesNuclear ExperimentInstrumentationphysics.ins-detMathematical Physicsgas: admixtureLarge Hadron ColliderDetectorneutriinotInstrumentation and Detectors (physics.ins-det)experimental equipmentneutrino: detectorNeutrino detectorTime projection chamberilmaisimettime projection chambersLarge scale cryogenic liquid detectors [8]photon: yieldParticle Physics - ExperimentperformanceMaterials scienceCERN LabTime projection chambersParticle tracking detectors (Gaseous detectors)ionization: yieldparticle tracking detectors (gaseous detectors)tutkimuslaitteetFOS: Physical scienceschemistry.chemical_elementNeutrino detectors; Particle tracking detectors (Gaseous detectors); Time projection chambersOptics0103 physical sciencesDeep Underground Neutrino Experiment[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsScintillationArgon010308 nuclear & particles physicsbusiness.industryhep-extime projection chamber: liquid argonchemistrymuon: cosmic radiationHigh Energy Physics::ExperimentbusinessTonneneutrino detectors
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Search for Lorentz and CPT violation using sidereal time dependence of neutrino flavor transitions over a short baseline

2017

A class of extensions of the Standard Model allows Lorentz and CPT violations, which can be identified by the observation of sidereal modulations in the neutrino interaction rate. A search for such modulations was performed using the T2K on-axis near detector. Two complementary methods were used in this study, both of which resulted in no evidence of a signal. Limits on associated Lorentz and CPT-violating terms from the Standard Model extension have been derived by taking into account their correlations in this model for the first time. These results imply such symmetry violations are suppressed by a factor of more than 1020 at the GeV scale.

Physics and Astronomy (miscellaneous)CPT symmetryAstrophysicsKAMIOKANDE01 natural scienceshigh energy physicsPhysics Particles & FieldsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Standard-Model Extension[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: interactionPhysicssymmetry: violationPhysicsJ-PARC LabCPT symmetrysuppressionLorentz symmetryviolation: LorentzmodulationSidereal timePhysical Sciencesneutrino: flavorsymbolsNeutrinoupper limitParticle physicsdata analysis method530 PhysicsLorentz transformationFOS: Physical sciencesCPT: violationAstronomy & AstrophysicsStandard Modelsymbols.namesakenear detectorstatistical analysis0103 physical sciences010306 general physicsNeutrino oscillationneutrino oscillationsScience & Technology010308 nuclear & particles physicshep-exHigh Energy Physics::PhenomenologySymmetry (physics)neutrino/mu: secondary beamcorrelationtime dependenceHigh Energy Physics::Experimentneutrino: oscillationexperimental results
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Chemical Evolution of Interstellar Methanol Ice Analogs upon Ultraviolet Irradiation: The Role of the Substrate

2018

An important issue in the chemistry of interstellar ices is the role of dust materials. In this work, we study the effect of an amorphous water-rich magnesium silicate deposited onto ZnSe windows on the chemical evolution of ultraviolet-irradiated methanol ices. For comparison, we also irradiate similar ices deposited onto bare ZnSe windows. Silicates are produced at relatively low temperatures exploiting a sol-gel technique. The chemical composition of the synthesized material reflects the forsterite stoichiometry. Si-OH groups and magnesium carbonates are incorporated during the process. The results show that the substrate material does affect the chemical evolution of the ice. In particu…

PhysicsAstrochemistryastrochemistryExtinction (astronomy)methods: laboratory: molecularSubstrate (chemistry)Astronomy and AstrophysicsISM: moleculeAstronomy and AstrophysicPhotochemistryultraviolet: ISM01 natural sciencesChemical evolutionchemistry.chemical_compoundchemistrySpace and Planetary Science0103 physical sciencesUltraviolet irradiationdust extinctionMethanol010306 general physics010303 astronomy & astrophysicsThe Astrophysical Journal
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SOFT X-RAY IRRADIATION OF PURE CARBON MONOXIDE INTERSTELLAR ICE ANALOGUES

2012

There is an increasing evidence for the existence of large organic molecules in the interstellar and circumstellar medium. Very few among such species are readily formed in conventional gas-phase chemistry under typical conditions of interstellar clouds. Attention has therefore focused on interstellar ices as a potential source of these relatively complex species. Laboratory experiments show that irradiation of interstellar ice analogues by fast particles or ultraviolet radiation can induce significant chemical complexity. However, stars are sources of intense X-rays at almost every stage of their formation and evolution. Such radiation may thus provide chemical changes in regions where ult…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaInterstellar icePhotodissociationInterstellar cloudAstronomy and AstrophysicsAstrophysicsRadiationmolecules | X-rays: ISM | methods: laboratory [ISM]Starschemistry.chemical_compoundSettore FIS/05 - Astronomia E AstrofisicachemistrySpace and Planetary ScienceISM: molecules | X-rays: ISM | methods: laboratoryAstrophysics::Earth and Planetary AstrophysicsIrradiationAstrophysics::Galaxy AstrophysicsOrder of magnitudeCarbon monoxide
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