Search results for " DETECTOR."

showing 10 items of 2685 documents

Risk assessment of beauvericin, enniatins and fusaproliferin present in follow-up infant formula by in vitro evaluation of the duodenal and colonic b…

2014

Abstract In this study, 72 samples of follow-up infant formula of Spanish origin were analyzed for the presence of the mycotoxins beauvericin (BEA), enniatins (ENs) (A, A1, B, B1), and fusaproliferin (FUS). The samples analyzed were extracted three times with ethyl acetate and then the mycotoxins were identified and quantified using a liquid chromatography (LC) coupled to a diode array detector (DAD). The positive samples analyzed in this study were digested through a simulated gastrointestinal digestion model, which permit to simulate the physiological condition of the human gastrointestinal tract (duodenal and colonic compartments) in order to assess the bioaccessibility of the bioactive …

chemistry.chemical_compoundFusaproliferinChromatographychemistryInfant formulaChromatography detectorEthyl acetateDigestionMycotoxinBeauvericinIn vitroFood ScienceBiotechnologyFood Control
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The detection efficiency of the clover Ge-detectors array at the RITU-GREAT facility

2015

Absolute detection efficiency depending upon its position along the beam line is determined for three germanium detectors, that are part of the GREAT spectrometer at the RITU separator focal plane. The efficiency is determined for an energy range from 80 keV to 1400 keV for all three detectors as an array and also individually using digital electronics. The optimal position for the detector array has been defined for two configurations of the GREAT spectrometer: with planar detector and without it. The obtained results have been compared with three references: a simulation prepared especially for this setup by another student, a previous study that was carried out by applying analogue elect…

clover detectorsPhysics::Instrumentation and DetectorsGe-detectorsspektrometritexperimental nuclear physicsRITUGREATgamma-spectroscopydetction efficiencyydinfysiikka
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Solid-state-biased coherent detection of ultra-broadband terahertz pulses

2017

Significant progress in nonlinear and ultrafast optics has recently opened new and exciting opportunities for terahertz (THz) science and technology, which require the development of reliable THz sources, detectors, and supporting devices. In this work, we demonstrate the first solid-state technique for the coherent detection of ultra-broadband THz pulses (0.1-10 THz), relying on the electric-field-induced second-harmonic generation in a thin layer of ultraviolet fused silica. The proposed CMOS-compatible devices, which can be realized with standard microfabrication techniques, allow us to perform ultra-broadband detection with a high dynamic range by employing probe laser powers and bias v…

coherent detectionTA1501Nonlinear opticTerahertzFar infrared or terahertzFour-wave mixingUltrafast opticDevicePhysics::OpticsUltrafast laserSolid state detectorSettore ING-INF/01 - ElettronicaQC0350Optica
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Progress in the Development of CdTe and CdZnTe Semiconductor Radiation Detectors for Astrophysical and Medical Applications

2009

Over the last decade, cadmium telluride (CdTe) and cadmium zinc telluride (CdZnTe) wide band gap semiconductors have attracted increasing interest as X-ray and gamma ray detectors. Among the traditional high performance spectrometers based on silicon (Si) and germanium (Ge), CdTe and CdZnTe detectors show high detection efficiency and good room temperature performance and are well suited for the development of compact and reliable detection systems. In this paper, we review the current status of research in the development of CdTe and CdZnTe detectors by a comprehensive survey on the material properties, the device characteristics, the different techniques for improving the overall detector…

compound semiconductorsSiliconcompound semiconductorchemistry.chemical_elementNanotechnologyGermaniumReviewlcsh:Chemical technologyBiochemistryAnalytical Chemistrychemistry.chemical_compoundX-ray and gamma ray spectroscopylcsh:TP1-1185Electrical and Electronic EngineeringInstrumentationcompound semiconductors; CdTe and CdZnTe detectors; X-ray and gamma ray spectroscopyPhysicsSpectrometerbusiness.industryDetectorSettore FIS/01 - Fisica SperimentaleWide-bandgap semiconductorCdTe and CdZnTe detectorCdTe and CdZnTe detectorsSemiconductor radiation detectorsAtomic and Molecular Physics and OpticsCadmium telluride photovoltaicsSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Cadmium zinc telluridechemistryOptoelectronicsbusiness
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Thermoelectric Radiation Detector Based on Superconductor-Ferromagnet Systems

2017

We suggest an ultrasensitive detector of electromagnetic fields exploiting the giant thermoelectric effect recently found in superconductor-ferromagnet hybrid structures. Compared with other types of superconducting detectors where the detected signal is based on variations of the detector impedance, the thermoelectric detector has the advantage of requiring no external driving fields. This is especially relevant in multipixel detectors, where the number of bias lines and the heating induced by them are an issue. We propose different material combinations to implement the detector and provide a detailed analysis of its sensitivity and speed. In particular, we perform a proper noise analysis…

cosmic microwave backgroundsuprajohtavuusoptoelectronicsPhysics::Instrumentation and Detectorsultrasensitive detectortutkimuslaitteetCosmic microwave backgroundFOS: Physical sciencesGeneral Physics and Astronomycosmic ray and astroparticle detectors02 engineering and technology01 natural sciences7. Clean energyParticle detectorsuprajohteetSuperconductivity (cond-mat.supr-con)Operating temperaturethermoelectric detectorsCondensed Matter::Superconductivity0103 physical sciencesThermoelectric effectthermoelectric effectssuperconductor-ferromagnet hybrid structures010306 general physicsSuperconductivityPhysicsta114business.industryCondensed Matter - SuperconductivityDetectorRangingoptoelektroniikka021001 nanoscience & nanotechnologyferromagnetismkosminen taustasäteilyFerromagnetismilmaisimetOptoelectronicsHigh Energy Physics::Experiment0210 nano-technologybusinessPhysical Review Applied
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Measurement of the cosmic-ray energy spectrum above 2.5×1018  eV using the Pierre Auger Observatory

2020

We report a measurement of the energy spectrum of cosmic rays for energies above 2.5×10^18 eV based on 215,030 events recorded with zenith angles below 60°. A key feature of the work is that the estimates of the energies are independent of assumptions about the unknown hadronic physics or of the primary mass composition. The measurement is the most precise made hitherto with the accumulated exposure being so large that the measurements of the flux are dominated by systematic uncertainties except at energies above 5×10^19 eV. The principal conclusions are(1) The flattening of the spectrum near 5×10^18 eV, the so-called "ankle,"is confirmed.(2) The steepening of the spectrum at around 5×10^19…

cosmic ray; astroparticle detectors; cosmic ray spectraEnergy SpectrumSettore FIS/01 - Fisica SperimentaleUltra-high energy cosmic rays energy spectrum Cherenkov detectorsUHE Cosmic Rays
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Status of Advanced Virgo

2017

The LIGO and the Virgo collaborations have recently announced the first detections of Gravitational Waves. Due to their weak amplitude, Gravitational Waves are expected to produce a very small effect on free-falling masses, which undergo a displacement of the order of 10-18 m for a Km-scale mutual distance. This discovery showed that interferometric detectors are suitable to reveal such a feeble effect, and therefore represent a new tool for astronomy, astrophysics and cosmology in the understanding of the Universe. To better reconstruct the position of the Gravitational Wave source and increase the signal-to-noise ratio of the events by means of multiple coincidence, a network of detectors…

cosmological modeldetector: performanceVirgo LIGO gravitational waveAstronomyinterferometerQC1-999detector: networkgravitational radiation: direct detection01 natural sciencesCoincidenceCosmologyPhysics and Astronomy (all)0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]LIGO010306 general physicsSettore FIS/01Physics010308 nuclear & particles physicsGravitational wavePhysicsDetectorgravitational radiationAstrophysics::Instrumentation and Methods for AstrophysicsAstronomygravitational radiation detectorLIGOdetector: sensitivityInterferometryVIRGOAmplitudePhysics and Astronomygravitational radiation: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Physics reach of the XENON1T dark matter experiment.

2016

The XENON1T experiment is currently in the commissioning phase at the Laboratori Nazionali del Gran Sasso, Italy. In this article we study the experiment's expected sensitivity to the spin-independent WIMP-nucleon interaction cross section, based on Monte Carlo predictions of the electronic and nuclear recoil backgrounds. The total electronic recoil background in $1$ tonne fiducial volume and ($1$, $12$) keV electronic recoil equivalent energy region, before applying any selection to discriminate between electronic and nuclear recoils, is $(1.80 \pm 0.15) \cdot 10^{-4}$ ($\rm{kg} \cdot day \cdot keV)^{-1}$, mainly due to the decay of $^{222}\rm{Rn}$ daughters inside the xenon target. The nu…

dark matter simulationsPhysics - Instrumentation and DetectorsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics::Instrumentation and Detectorsdark matter experimentFOS: Physical scienceschemistry.chemical_elementCosmic ray7. Clean energy01 natural sciencesdark matter simulationNuclear physicsRecoilXenonIonization0103 physical sciencesNeutronNuclear Experiment010306 general physicsPhysicsMuon010308 nuclear & particles physicsdark matter experimentsAstronomy and AstrophysicsInstrumentation and Detectors (physics.ins-det)dark matter experiments; dark matter simulationschemistryNeutrinoNucleonAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Computational Techniques for the Analysis of Small Signals in High-Statistics Neutrino Oscillation Experiments

2020

The current and upcoming generation of Very Large Volume Neutrino Telescopes – collecting unprecedented quantities of neutrino events – can be used to explore subtle effects in oscillation physics, such as (but not restricted to) the neutrino mass ordering. The sensitivity of an experiment to these effects can be estimated from Monte Carlo simulations. With the high number of events that will be collected, there is a trade-off between the computational expense of running such simulations and the inherent statistical uncertainty in the determined values. In such a scenario, it becomes impractical to produce and use adequately-sized sets of simulated events with traditional methods, such as M…

data analysis methodNuclear and High Energy PhysicsMonte Carlo methodFVLV nu TData analysis; Detector; KDE; MC; Monte Carlo; Neutrino; Neutrino mass ordering; Smoothing; Statistics; VLVνTData analysisKDEFOS: Physical sciences01 natural sciencesIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)statistical analysisnumerical methods0103 physical sciencesStatisticsNeutrinoddc:530Sensitivity (control systems)MC010306 general physicsNeutrino oscillationInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationMonte CarloPhysicsVLVνT010308 nuclear & particles physicsOscillationStatisticsoscillation [neutrino]ObservableDetectorMonte Carlo [numerical calculations]WeightingNeutrino mass orderingPhysics and AstronomyPhysics - Data Analysis Statistics and ProbabilityPhysique des particules élémentairesNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsMATTERData Analysis Statistics and Probability (physics.data-an)SmoothingSmoothing
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Measurement of θ13 in Double Chooz using neutron captures on hydrogen with novel background rejection techniques

2016

The Double Chooz collaboration presents a measurement of the neutrino mixing angle θ[subscript 13] using reactor [bar over ν[subscript e]] observed via the inverse beta decay reaction in which the neutron is captured on hydrogen. This measurement is based on 462.72 live days data, approximately twice as much data as in the previous such analysis, collected with a detector positioned at an average distance of 1050 m from two reactor cores. Several novel techniques have been developed to achieve significant reductions of the backgrounds and systematic uncertainties. Accidental coincidences, the dominant background in this analysis, are suppressed by more than an order of magnitude with respec…

data analysis methodNuclear and High Energy PhysicsParticle physicsPhysics - Instrumentation and DetectorsNeutrino Detectors and TelescopeGadoliniumnuclear reactor [antineutrino/e]energy spectrumchemistry.chemical_elementFluxmixing angle: measured [neutrino]CHOOZ7. Clean energy01 natural sciencesHigh Energy Physics - Experimentflux [antineutrino]Flavor physicscapture [n]0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Electroweak interactionddc:530Neutron010306 general physicsPhysicsNeutrino Detectors and Telescopesbackground010308 nuclear & particles physicsoscillation [neutrino]suppressionDouble ChoozNeutron captureOscillationchemistryhydrogenInverse beta decayFlavor physicspectralHigh Energy Physics::ExperimentgadoliniumNeutrinoOrder of magnitudeexperimental results
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