Search results for "sperimentale"

showing 10 items of 938 documents

NANO-EMETTITORI NIR A BASE DI SILICE PER APPLICAZIONI IN-VIVO E RELATIVO PROCESSO DI PRODUZIONE

2010

Realizzazione di nano-sonde paramagnetiche e fosforescenti, ottenibili a partire da particelle nanometriche di silice mediante procedure di sintesi e arricchimento di O2 a seguito di opportuni trattamenti termici in ambiente controllato. Le nano-sonde così ottenute presentano emissioni nel vicino infrarosso (NIR), sono eccitabili nel visibile e nel NIR, e sono caratterizzate da un tempo di vita nell’ordine del secondo. Tali nano-sonde presentano un notevole potenziale scientifico e commerciale nel mercato della spettroscopia confocale per bio-imaging e nel mercato delle applicazioni medico-farmaceutiche di drug-labelling e drug-delivery.

nano siliceprobe fluorescenti probe magnetici applicazioni in vivoNano emettitoriSettore FIS/01 - Fisica Sperimentale
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Developing emergent literacy in infant schools: a laboratory experience for the construction of the written language

2017

Research, including the educational neuroscience, has highlighted the close relationship between emerging literacy and subsequent learning of reading and writing. Early verification of symbolic and linguistic skills is essential to support the development, and recovery strategies are to be prepared in case of early signs of difficulty. In some infant schools in the Palermo area we carried out a laboratory of the last 45 hours, according to a specific methodological setting, with a dual aim: a) developing the emerging areas of literacy in preschool, b) providing teachers with an objective approach to detect in children reading and writing readiness. The study investigated phonological, lexic…

narrazioneemerging skillsstorytellingemerging skillmetodo fonematicocompetenze emergentimedia digitalilcsh:LSettore M-PED/04 - Pedagogia Sperimentaledigital mediaSettore M-PED/03 - Didattica E Pedagogia Specialephonemic methodlcsh:EducationForm@re : Open Journal per la Formazione in Rete
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GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

2017

On August 17, 2017 at 12-41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0×104 years. We infer the component masses of the binary to be between 0.86 and 2.26 M, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60 M, with the total mass of the system 2.74-0.01+0.04M. The source was localized within a sky region of 28 deg2 (90% probabili…

neutron star: binary[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]X-ray binaryADVANCED LIGOAstrophysicsKilonovagravitational waves; LIGO; binary neutron star inspiralspin01 natural sciencesLIGOGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Electromagnetic observationsGravitational-wave signals3100 General Physics and AstronomyPoint MassesAstrophysics - High Energy Astrophysical PhenomenaBlack-Hole MergersBinary neutron starsBlack HolesX-ray bursterCoalescing BinariesAstrophysics::High Energy Astrophysical Phenomena10192 Physics InstituteGeneral Relativity and Quantum Cosmology (gr-qc)Gravity wavesGravitational wavesNeutron starsPhysics and Astronomy (all)ddc:530Electromagnetic spectraNeutrons010308 nuclear & particles physicsVirgoGamma raysAstronomyRCUKVIRGOelectromagneticgravitational radiation: emissionStellar black holeGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Compact Binariesbinary: masscosmological modelAstronomyGeneral Physics and AstronomyAstrophysicsneutron starsGamma ray burstsGeneral Relativity and Quantum CosmologyGravitational wave detectorsUniverseDENSE MATTER010303 astronomy & astrophysicsastro-ph.HEPhysicsSignal to noise ratioSettore FIS/01 - Fisica SperimentaleGravitational effectsFalse alarm rateEQUATION-OF-STATEMergers and acquisitionsgravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]530 PhysicsMERGERSGeneral Relativity and Quantum Cosmology; General Relativity and Quantum Cosmology; astro-ph.HEFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstgravitational radiation: direct detectionMerging[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GAMMA-RAY BURSTLIGO (Observatory)binary: coalescenceGravitational waves neutron stars gamma-ray burst LIGO Virgo0103 physical sciencesGW151226MASSESSTFCAstrophysics::Galaxy AstrophysicsPhysiqueGravitational wavegravitational radiationPULSARgravitational radiation detectorNeutron starPhysics and AstronomygravitationRADIATIONDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikbinary neutron star inspiralSignal detectionPHYS REV LETT PHYSICAL REVIEW LETTERS
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O2-Loading Treatment of Ge-Doped Silica Fibers: A Radiation Hardening Process

2016

International audience; The effects of a high-pressure O2-loading treatment on the radiation response of Ge-doped optical fibers (OFs) were investigated. We found that the incorporation of high concentration of interstitial molecular oxygen remarkably enhances the resistance to ionizing radiation of Ge-doped OFs in the UV-Visible domain and, at the same time, improves the transmission of UV light in the unirradiated OF sample. By comparison with previously reported results, the O2-loading treatment turned out to increase the radiation resistance of Ge-doped OFs more efficiently than F or Ce codoping. The understanding of such amelioration relies in basic radiation-induced mechanisms that we…

optical fiberMaterials scienceAnalytical chemistrychemistry.chemical_elementGermanium02 engineering and technologygermanosilicate01 natural scienceslaw.inventionIonizing radiationOpticslaw0103 physical sciencesIrradiationElectron paramagnetic resonanceRadiation hardeningRadiation resistance[PHYS]Physics [physics]radiation effect010308 nuclear & particles physicsbusiness.industryDopingSettore FIS/01 - Fisica SperimentaleResonance021001 nanoscience & nanotechnologyAtomic and Molecular Physics and Opticschemistry0210 nano-technologybusiness
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Origins of radiation-induced attenuation in pure-silica-core and Ge-doped optical fibers under pulsed x-ray irradiation

2020

We investigated the nature, optical properties, and decay kinetics of point defects causing large transient attenuation increase observed in silica-based optical fibers exposed to short duration and high-dose rate x-ray pulses. The transient radiation-induced attenuation (RIA) spectra of pure-silica-core (PSC), Ge-doped, F-doped, and Ge + F-doped optical fibers (OFs) were acquired after the ionizing pulse in the spectral range of [∼0.8–∼3.2] eV (∼1500–∼380 nm), from a few ms to several minutes after the pulse, at both room temperature (RT) and liquid nitrogen temperature (LNT). Comparing the fiber behavior at both temperatures better highlights the thermally unstable point defects contribut…

optical fiberMaterials scienceOptical fiberAnalytical chemistryGeneral Physics and Astronomy02 engineering and technologymedicine.disease_cause01 natural scienceslaw.inventionx-ray irradiationlaw0103 physical sciencesmedicinepoint defectsRadiation induced absorptionFiberAbsorption (electromagnetic radiation)ComputingMilieux_MISCELLANEOUS010302 applied physics[PHYS]Physics [physics]F dopingAttenuationDopingSettore FIS/01 - Fisica SperimentaleLiquid nitrogen021001 nanoscience & nanotechnologyCrystallographic defectGe doping0210 nano-technologyUltraviolet
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Radiation Response of Ce-Codoped Germanosilicate and Phosphosilicate Optical Fibers

2016

We report an experimental investigation on the effects of Ce-codoping in determining the radiation response of germanosilicate and phosphosilicate Optical Fibers (OFs) in the UV-Visible domain and up to doses of $1~\hbox{MGy}({\rm SiO}_{2})$ . We show that the addition of Ce strongly impacts the Radiation Induced Attenuation (RIA) of both types of fibers. In the first case the radiation induced losses increase, whereas in the second one decrease. By combining the online RIA measurements with the Electron Paramagnetic Resonance (EPR) ones, we are able to infer the basic microscopic mechanisms taking place under irradiation, which involve the cerium codopant and some of the known Ge-related o…

optical fiberNuclear and High Energy PhysicsMaterials scienceMGy irradiationAnalytical chemistrychemistry.chemical_element02 engineering and technologyRadiationgermanosilicate01 natural sciencesradiation induced attenuationIonlaw.invention020210 optoelectronics & photonicsRadiation sensitivityOpticslaw0103 physical sciences0202 electrical engineering electronic engineering information engineeringphosphosilicateDosimetryIrradiationElectrical and Electronic EngineeringElectron paramagnetic resonanceNuclear and High Energy Physic[PHYS]Physics [physics]010308 nuclear & particles physicsbusiness.industrySettore FIS/01 - Fisica SperimentaleDopingCeriumCeriumNuclear Energy and EngineeringchemistrycodopingbusinessIEEE Transactions on Nuclear Science
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ORAL EXPRESSIVE COMPETENCE’S DEVELOPMENT BY USE OF MINDTOOLS

2015

The aim of this work is to verify the efficacy of a training programme focused on the enhancement of oral expressiveness (the generation of ideas and planning, pragmatic awareness), realized with a group of children between 10 and 12 years, in the last year of primary school and in the first year of secondary school in the Palermo area. The educational activities were conducted from January to June 2014. Action learning provided a learning environment based on real problem solving with team work; the active search for information, discussion and reflection, as well as decision-making, were assisted by semantic networks (concept maps) and knowledge construction tools. Oral presentation, or p…

oral presentation competence concepts map information technology evaluation criteriaSettore M-PED/04 - Pedagogia SperimentaleSettore M-PED/03 - Didattica E Pedagogia Speciale
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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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Gli esercizi ADVP realizzati dal liceo classico "Altavilla" di Palermo

2009

Il contributo presenta una serie di esercizi ADVP (Activaction du Developpement Vocationnel et Personnel) realizzati e sperimentati, all'interno del Progetto Aracne Due (P.O.R. Sicilia 2000/2006 - Asse III - Mis. 3.05), presso il liceo classico Altavilla di Palermo. L'originalità delle attività ADVP realizzate consiste nel fatto che i compiti svolti dagli studenti vertono principalmente sulle conoscenze e abilità disciplinari previste dai programmi ministeriali relativi al liceo.

orientamento maturazione personale e professionale disciplineSettore M-PED/04 - Pedagogia Sperimentale
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Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory

2019

The profile of the longitudinal development of showers produced by ultra-high energy cosmic rays carries information related to the interaction properties of the primary particles with atmospheric nuclei. In this work, we present the first measurement of the average shower profile in traversed atmospheric depth at the Pierre Auger Observatory. The shapes of profiles are well reproduced by the Gaisser-Hillas parametrization within the range studied, for E>10 17.8 eV .A detailed analysis of the systematic uncertainties is performed using ten years of data and a full detector simulation. The average shape is quantified using two variables related to the width and asymmetry of the profile, and …

p: showersphoton: Cherenkovinteraction: modelAstronomyHadronpiastro-ph.HE; astro-ph.HE01 natural sciencesnitrogenironParametrization (atmospheric modeling)Monte Carlomedia_commonPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Range (particle radiation)photomultiplierSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsDETETOREScosmic rays detectors; ultra high energy cosmic rays; Astronomy and AstrophysicsAugerobservatorycosmic rays detectorscosmic rays detectors; ultra high energy cosmic raysgeometricalAstrophysics - High Energy Astrophysical PhenomenaasymmetrylongitudinalCherenkov counter: waterairmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayheliumultra high energy cosmic raysnucleus: atmosphereAsymmetry0103 physical sciencesHigh Energy Physicscosmic radiation: UHEcosmic rays detectorFLUORESCENCEAstrophysiquePierre Auger Observatoryelectron positronshowers: atmosphere010308 nuclear & particles physicsbackgrounddetector: surfaceshowers: spatial distributionparametrizationAstronomy and AstrophysicsAstronomieComputational physics13. Climate actiongamma rayExperimental High Energy Physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)Journal of Cosmology and Astroparticle Physics
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