Search results for "CLEAR"

showing 10 items of 27042 documents

Near‐IR Radiation‐Induced Attenuation of Aluminosilicate Optical Fibers

2021

The X-ray radiation-induced attenuation (RIA) growth kinetics are studied online in different single-mode aluminosilicate optical fibers in the near-IR (NIR) domain to evaluate their potential in terms of dosimetry. The optical fibers differ by Al contents, core sizes, drawing parameters, and also by a preform deposition process. The data show no dependence of the RIA on all these parameters, a positive result for the design of point or distributed radiation detectors exploiting RIA to monitor the dose. The RIA growth rate is unchanged for dose rates changing from 0.073 to 6.25 Gy(SiO2) s−1, and the RIA linearly increases with the dose up to 2 kGy(SiO2). Small but noticeable RIA changes are…

optical fibersMaterials scienceOptical fiberRadiation induced02 engineering and technology01 natural scienceslaw.inventionX-ray irradiations[SPI]Engineering Sciences [physics]020210 optoelectronics & photonicsAluminosilicatelaw0103 physical sciences0202 electrical engineering electronic engineering information engineeringMaterials Chemistryradiation-induced attenuationElectrical and Electronic EngineeringComposite materialComputingMilieux_MISCELLANEOUS010308 nuclear & particles physicsAttenuationSurfaces and InterfacesCondensed Matter PhysicsSurfaces Coatings and FilmsElectronic Optical and Magnetic Materialsaluminosilicate glassesradiation effectsphysica status solidi (a)
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Internal conversion from excited electronic states of 229Th ions

2017

The process of internal conversion from excited electronic states is investigated theoretically for the case of the vacuum-ultraviolet nuclear transition of 229 Th . Due to the very low transition energy, the 229 Th nucleus offers the unique possibility to open the otherwise forbidden internal conversion nuclear decay channel for thorium ions via optical laser excitation of the electronic shell. We show that this feature can be exploited to investigate the isomeric state properties via observation of internal conversion from excited electronic configurations of Th + and Th 2 + ions. A possible experimental realization of the proposed scenario at the nuclear laser spectroscopy facility IGISO…

optical laser excitationNuclear Experimentthorium ionsinternal conversionexcited electronic states
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Structural and optical characterization of ZnS ultrathin films prepared by low-temperature ALD from diethylzinc and 1.5-pentanedithiol after various …

2019

The structural and optical evolution of the ZnS thin films prepared by atomic layer deposition (ALD) from the diethylzinc (DEZ) and 1,5-pentanedithiol (PDT) as zinc and sulfur precursors was studied. A deposited ZnS layer (of about 60 nm) is amorphous, with a significant S excess. After annealing, the stoichiometry improved for annealing temperatures &ge

optical propertiesMaterials scienceAnnealing (metallurgy)Analytical chemistryEpitaxylcsh:TechnologyArticleAnnealingAtomic layer depositionatomic layer deposition (ALD)General Materials ScienceThin filmlcsh:Microscopylcsh:QC120-168.85lcsh:QH201-278.5Optical propertieslcsh:TAtmospheric temperature rangeatomikerroskasvatusAmorphous solidAtomic layer deposition (ALD)lcsh:TA1-2040lcsh:Descriptive and experimental mechanicsannealinglcsh:Electrical engineering. Electronics. Nuclear engineeringCrystalliteohutkalvotlcsh:Engineering (General). Civil engineering (General)lcsh:TK1-9971StoichiometryZnS thin films
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Synthesis, Optical, and Morphological Studies of ZnO Powders and Thin Films Fabricated by Wet Chemical Methods

2020

Zinc oxide nanoparticles were prepared from Zn5(CO3)2(OH)6 precursor, capped with poly(vinylpyrrolidone) (PVP), and annealed at 600 &deg

optical propertiesMaterials scienceScanning electron microscopeAnalytical chemistryNanoparticleInfrared spectroscopy02 engineering and technology010402 general chemistrylcsh:Technology01 natural sciencesArticlesymbols.namesakeMicroscopyGeneral Materials ScienceThin filmlcsh:MicroscopyThermal analysisComputingMilieux_MISCELLANEOUSlcsh:QC120-168.85[PHYS]Physics [physics][PHYS.PHYS.PHYS-OPTICS]Physics [physics]/Physics [physics]/Optics [physics.optics]lcsh:QH201-278.5lcsh:T021001 nanoscience & nanotechnology0104 chemical scienceswet chemical methodsthin filmspoly(vinylpyrrolidone)lcsh:TA1-2040Transmission electron microscopyZnOsymbolsnanoparticleslcsh:Descriptive and experimental mechanics[PHYS.PHYS.PHYS-CHEM-PH]Physics [physics]/Physics [physics]/Chemical Physics [physics.chem-ph]lcsh:Electrical engineering. Electronics. Nuclear engineeringlcsh:Engineering (General). Civil engineering (General)0210 nano-technologyRaman spectroscopylcsh:TK1-9971poly(vinylpyrrolidone) optical propertiesMaterials
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Optimization of the JUNO liquid scintillator composition using a Daya Bay antineutrino detector

2021

To maximize the light yield of the liquid scintillator (LS) for the Jiangmen Underground Neutrino Observatory (JUNO), a 20 t LS sample was produced in a pilot plant at Daya Bay. The optical properties of the new LS in various compositions were studied by replacing the gadolinium-loaded LS in one antineutrino detector. The concentrations of the fluor, PPO, and the wavelength shifter, bis-MSB, were increased in 12 steps from 0.5 g/L and <0.01 mg/L to 4 g/L and 13 mg/L, respectively. The numbers of total detected photoelectrons suggest that, with the optically purified solvent, the bis-MSB concentration does not need to be more than 4 mg/L. To bridge the one order of magnitude in the detect…

organic compounds: admixtureNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsLiquid scintillatorscintillation counter: liquidAnalytical chemistryFOS: Physical sciencesmodel: opticalScintillatorWavelength shifterantineutrino: detector01 natural sciencesNOHigh Energy Physics - Experimentwavelength shifterHigh Energy Physics - Experiment (hep-ex)PE2_2Daya BayNeutrino0103 physical sciencesfluorine: admixture[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530neutrino oscillation[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentationJiangmen Underground Neutrino ObservatoryPhysicsJUNO010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleDetectorLight yield; Liquid scintillator; NeutrinoInstrumentation and Detectors (physics.ins-det)Yield (chemistry)Scintillation counterComposition (visual arts)photon: yieldNeutrinoLight yieldNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Suomen viidennen ydinvoimalan lobbaus kansanedustajan näkökulmasta

2003

organisaatioviestintälobbauspoliittinen viestintäorganizational communicationnuclear powerlobbyingkansanedustajatpolitical communicationydinvoimamembers of Parliamenteturyhmät
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Sex steroid hormone receptors, their ligands, and nuclear and non-nuclear pathways

2015

The ability of a cell to respond to a particular hormone depends on the presence of specific receptors for those hormones. Once the hormone has bound to its receptor, and following structural and biochemical modifications to the receptor, it separates from cytoplasmic chaperone proteins, thereby exposing the nuclear localization sequences that result in the activation of the receptor and initiation of the biological actions of the hormone on the target cell. In addition, recent work has demonstrated new pathways of steroid signaling through orphan and cell surface receptors that contribute to more rapid, “non-nuclear” or non-transcriptional effects of steroid hormones, often involving G-pro…

orphan receptorreceptorreceptorsandrogenBiologyprogesteronegenomic pathwaySettore BIO/10 - Biochimicaestrogensex steroid hormoneReceptorlcsh:Science (General)Orphan receptorHormone response elementsex steroid hormones; receptors; estrogens; androgens; progesterone; genomic pathway; non-genomic pathway; orphan receptorandrogensSex hormone receptornon-genomic pathwayBiochemistryNuclear receptorSex steroidHormone receptorsex steroid hormonesEstrogen-related receptor gammaestrogenslcsh:Q1-390AIMS Molecular Science
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Direct P-functionalization of azobenzene by a cationic phosphidozirconocene complex.

2016

International audience; We report that the cationic phosphidozirconocene complex [(eta(5)-C5H5)(2)Zr(PCy2)][CH3B(C6F5)(3)] (II) reacts with azobenzene, resulting in the expedient formation of Zr complex (2) bound to a tridentate PNN ligand. This reaction proceeds by a mechanism of cooperative nucleophilic substitution of hydrogen. The intermediate sigma(H) adduct (1) has been characterized by NMR spectroscopy.

ortho-acylationHydrogenaromatic azo-compoundschemistry.chemical_element[CHIM.INOR]Chemical Sciences/Inorganic chemistry010402 general chemistryBioinformatics01 natural sciences[ CHIM ] Chemical SciencesAdductalcoholsInorganic Chemistrychemistry.chemical_compoundc-h functionalizationPolymer chemistryNucleophilic substitution[CHIM]Chemical Sciences010405 organic chemistryChemistryLigandCationic polymerizationcinnolinium salts[ CHIM.INOR ] Chemical Sciences/Inorganic chemistryNuclear magnetic resonance spectroscopy0104 chemical sciences3. Good healthAzobenzeneazoxybenzenesalpha-oxocarboxylic acidsazoareneshydrogennucleophilic-substitutionSurface modificationDalton transactions (Cambridge, England : 2003)
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STUDIES OF VARIABILITY IN PROTO-PLANETARY NEBULAE. II. LIGHT AND VELOCITY CURVE ANALYSES OF IRAS 22272+5435 AND 22223+4327

2013

We have carried out a detailed observational study of the light, color, and velocity variations of two bright, carbon-rich proto-planetary nebulae, IRAS 22223+4327 and 22272+5435. The light curves are based upon our observations from 1994 to 2011, together with published data by Arkhipova and collaborators. They each display four significant periods, with primary periods for IRAS 22223+4327 and 22272+5435 being 90 and 132 days, respectively. For each of them, the ratio of secondary to primary period is 0.95, a value much different from that found in Cepheids, but which may be characteristic of post-asymptotic giant branch (AGB) stars. Fewer significant periods are found in the smaller radia…

oscillations [stars]Cepheid variableFOS: Physical sciencesAstrophysics01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsgeneral [planetary nebulae]010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsGalaxy rotation curvePhysicsNebula010308 nuclear & particles physicsAstronomy and AstrophysicsLight curveAGB and post-AGB [stars]Planetary nebulaRadial velocityStarsAmplitudeAstrophysics - Solar and Stellar Astrophysicsvariables: general [stars]Space and Planetary Scienceindividual (IRAS 22223+4327 IRAS 22272+5435) [stars]Astrophysics::Earth and Planetary AstrophysicsThe Astrophysical Journal
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Pulsating B and Be stars in the Small Magellanic Cloud

2008

Context: Stellar pulsations in main-sequence B-type stars are driven by the kappa-mechanism due to the Fe-group opacity bump. The current models do not predict the presence of instability strips in the B spectral domain at very low metallicities. As the metallicity of the SMC is lower than Z=0.005, it constitutes a very suitable object to test these predictions. Aims: The main objective is to investigate the existence of B-type pulsators at low metallicities, searching for short-term periodic variability in absorption-line B and Be stars in the SMC. The analysis has been performed in a sample of 313 B and Be stars with fundamental astrophysical parameters accurately determined from high-res…

oscillations [stars]statistics [Stars]Be starHertzsprung–Russell diagramMetallicityFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesStars : emission-line Be; stars : oscillations; Stars : early-type; Stars : statistics; Galaxies : Magellanic Cloudssymbols.namesakeMagellanic Clouds [Galaxies]early-type [Stars]0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::GalaxiasAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsAstrophysics (astro-ph)Astronomy and AstrophysicsLight curveGalaxy:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Galaxias [UNESCO]Stars13. Climate actionSpace and Planetary Scienceemission-line Be [Stars]symbolsSmall Magellanic CloudAstrophysics::Earth and Planetary AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::EstrellasInstability strip:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]
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