Search results for "Detectors"

showing 10 items of 2229 documents

Equivalence of Open-Loop and Closed-Loop Operation of SAW Resonators and Delay Lines

2019

International audience; Surface acoustic wave (SAW) sensors in the form of two-port resonators or delay lines are widely used in various fields of application. The readout of such sensors is achieved by electronic systems operating either in an open-loop or in a closed-loop configuration. The mode of operation of the sensor system is usually chosen based on requirements like, e.g., bandwidth, dynamic range, linearity, costs, and immunity against environmental influences. Because the limit of detection (LOD) at the output of a sensor system is often one of the most important figures of merit, both readout structures, i.e., open-loop and closed-loop systems, are analyzed in terms of the minim…

[SPI.OTHER]Engineering Sciences [physics]/OtherPhysics - Instrumentation and DetectorsComputer scienceddc:621.3ResonatorPhase NoiseFOS: Physical sciencesSAW sensorslcsh:Chemical technology01 natural sciencesBiochemistryArticleAnalytical Chemistryfrequency detectionResonator0103 physical sciencesPhase noiseElectronic engineeringreadout systemsFigure of meritddc:6lcsh:TP1-1185[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Electrical and Electronic EngineeringReadout Systems010301 acousticsInstrumentationDelay LineDynamic rangeFrequency Detection010401 analytical chemistryBandwidth (signal processing)Surface acoustic waveOpen-loop controllerarticlePhase DetectionLinearityInstrumentation and Detectors (physics.ins-det)Open-loop Vs. Closed-loopdelay lineAtomic and Molecular Physics and Opticsphase noise0104 chemical sciencesSaw Sensorsopen-loop vs. closed-loopresonatorPhase-sensitive Sensorsphase detectionphase-sensitive sensors
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Residual Phase Noise Measurement of Optical Second Harmonic Generation in PPLN Waveguides

2017

We report on the characterization, including residual phase noise and fractional frequency instability, of fiber-coupled PPLN non-linear crystals. These components are devoted to frequency doubling 871 nm light from an extended-cavity diode laser to produce a 435.5 nm beam, corresponding to the ytterbium ion electric quadrupole clock transition. We measure doubling efficiencies of up to 117.5 %/W. Using a Mach-Zehnder interferometer and an original noise rejection technique, the residual phase noise of the doublers is estimated to be lower than ${\rm -35\, dBrad^2/Hz}$ at 1 Hz, making these modules compatible with up-to-date optical clocks and ultra-stable cavities. The influence of externa…

[SPI.OTHER]Engineering Sciences [physics]/OtherPhysics - Instrumentation and DetectorsMaterials scienceAtomic Physics (physics.atom-ph)Lithium niobateFOS: Physical sciencesPhysics::Optics01 natural sciences7. Clean energyPhysics - Atomic Physicslaw.invention010309 opticsOptical pumpingchemistry.chemical_compoundOpticslaw0103 physical sciencesPhase noise[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Electrical and Electronic Engineering010306 general physicsbusiness.industrySecond-harmonic generationInstrumentation and Detectors (physics.ins-det)LaserAtomic and Molecular Physics and OpticsAtomic clock[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Electronic Optical and Magnetic MaterialsInterferometrychemistrybusinessNoise (radio)Optics (physics.optics)Physics - Optics
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Phase-Noise and Amplitude-Noise Measurement of DACs and DDSs

2019

This article proposes a method for the measurement of Phase Noise (PN, or PM noise) and Amplitude Noise (AN, or AM noise) of Digital-to-Analog Converters (DAC) and Direct Digital Synthesizers (DDS) based on modulation-index amplification. The carrier is first reduced by a controlled amount (30-40 dB) by adding a reference signal of nearly equal amplitude and opposite in phase. Then, residual carrier and noise sidebands are amplified and sent to a conventional PN analyzer. The main virtues of our method are: (i) the noise specs of the PN analyzer are relaxed by a factor equal to the carrier suppression ratio; and, (ii) the capability to measure the AN using a PN analyzer, with no need for th…

[SPI.OTHER]Engineering Sciences [physics]/OtherSpectrum analyzerPhysics - Instrumentation and DetectorsAcoustics and UltrasonicsAtomic Physics (physics.atom-ph)AcousticsFast Fourier transformFOS: Physical sciences02 engineering and technology01 natural sciencesPhysics - Atomic PhysicsAmplitude modulationBackground noise0103 physical sciencesPhase noiseFlicker noise[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Electrical and Electronic Engineering010301 acousticsInstrumentationPhysicsNoise measurementFlicker010401 analytical chemistryInstrumentation and Detectors (physics.ins-det)Converters021001 nanoscience & nanotechnologyResidual carrier[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]0104 chemical sciencesNoiseAmplitudeDevice under test0210 nano-technology
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Frequency Stability Measurement of Cryogenic Sapphire Oscillators with a Multichannel Tracking DDS and the Two-Sample Covariance

2018

This article shows the first measurement of three 100 MHz signals exhibiting fluctuations from 2E-16 to parts in 1E-15 for integration time tau between 1 s and 1 day. Such stable signals are provided by three Cryogenic Sapphire Oscillators (CSOs) operating at about 10 GHz, also delivering the 100 MHz output via a dedicated synthesizer. The measurement is made possible by a 6-channel Tracking DDS (TDDS) and the two-sample covariance tool, used to estimate the Allan variance. The use of two TDDS channels per CSO enables high rejection of the instrument background noise. The covariance outperforms the Three-Cornered Hat (TCH) method in that the background converges to zero "out of the box," wi…

[SPI.OTHER]Engineering Sciences [physics]/OtherTime delay and integrationPhysicsPhysics - Instrumentation and DetectorsAcoustics and UltrasonicsNoise measurementAutomatic frequency controlFOS: Physical sciences020206 networking & telecommunicationsInstrumentation and Detectors (physics.ins-det)02 engineering and technologyCovarianceTopology01 natural sciencesStability (probability)Background noiseDirect digital synthesizer0103 physical sciences0202 electrical engineering electronic engineering information engineering[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Electrical and Electronic EngineeringAllan variance010301 acousticsInstrumentation
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Holes Interaction and Heterogeinity Distribution Effect for a Multiperforated Plate

2012

International audience; Originally used to protect classical sound absorbing materials from environmental degradation, multi-perforated plates are considered to be one of the next generation soundproof solutions. This paper investigates the effects of holes interaction and heterogeneity distribution on the acoustical properties of a multi-perforated plate. These effects are observable on the specimens with closely separated holes. Multi-perforated plates with different center-to-center holes distances (pitches) are built and tested using an impedance tube. The cases of closely separated holes are analyzed and compared to the cases of widely separated holes. It is observed that in the presen…

[SPI]Engineering Sciences [physics][SPI] Engineering Sciences [physics]Physics::Instrumentation and Detectors
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Search for Higgs boson pair production in the two bottom quarks plus two photons final state in pp collisions at a energy-of-centre of mass of 13 TeV…

2022

This thesis presents a physics analysis performed with the ATLAS detector at the Large Hadron Collider with data from the Run 2 (2015-2018) period of proton-proton collision at a center-of-mass energy of 13 TeV, corresponding to an integrated luminosity used for physics analyses of 139 inverse-fb. The analysis is a search for resonant and non-resonant Higgs boson pair production in the two bottom quarks and two photon final state. Special focus is given to the event selection strategy for the resonant search using multi-variate techniques. In addition, the ATLAS upgrade for the Run 3 (2022-2025) period where the software is migrated to a multi-threading framework is extensively covered alon…

accelerator physicsfísicaPhysics::Instrumentation and Detectors:FÍSICA [UNESCO]UNESCO::FÍSICAHigh Energy Physics::Experimentfísica de altas energíasparticle physicshiggs boson
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ATLAS Inner Detector alignment and analysis of the Wtb vertex structure with single top quarks

2018

Esta tesis puede ser dividida en dos partes diferentes: La primera trata sobre el alineamiento del detector interno de ATLAS, y la segunda sobre el estudio de la estructura del vértice Wtb mediante el uso de quarks top producidos en solitario. La primera parte presenta las técnicas utilizadas para alinear el detector interno de ATLAS, así como las mejoras implementadas en algoritmo de alineamiento durante el Run-II del LHC. Durante la toma de datos, tienen lugar en el detector interno diversos movimientos y deformaciones dinámicos que comprometen la calidad de los datos recogidos. Los dos más relevantes son un movimiento vertical del detector de Píxeles, y el combado del IBL. En el alineami…

anomalous couplingsweak interaction221502 - Física experimental de altas energíasalignment221500 - Física de altas energíasHigh Energy Physics::ExperimentATLASDetectors and Experimental TechniquesInner Detectortop quarksingle top220807 - Física de partículas
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Design of an Antimatter Large Acceptance Detector In Orbit (ALADInO)

2022

International audience; A new generation magnetic spectrometer in space will open the opportunity to investigate the frontiers in direct high-energy cosmic ray measurements and to precisely measure the amount of the rare antimatter component in cosmic rays beyond the reach of current missions. We propose the concept for an Antimatter Large Acceptance Detector In Orbit (ALADInO), designed to take over the legacy of direct measurements of cosmic rays in space performed by PAMELA and AMS-02. ALADInO features technological solutions conceived to overcome the current limitations of magnetic spectrometers in space with a layout that provides an acceptance larger than 10 m sr. A superconducting ma…

antimatter; cosmic rays; dark matter; particle detectors; space instrumentation;space instrumentationcosmic raysantimatter; cosmic rays; dark matter; particle detectors; space instrumentationAstrophysics::High Energy Astrophysical PhenomenaSettore FIS/01 - Fisica Sperimentaleantimatter[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]particle detectorsInstrumentationdark mattercosmic rays; antimatter; dark matter; particle detectors; space instrumentation
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Search for low-energy neutrinos from astrophysical sources with Borexino

2019

We report on searches for neutrinos and antineutrinos from astrophysical sources performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. Electron antineutrinos ($\bar{\nu}_e$) are detected in an organic liquid scintillator through the inverse $\beta$-decay reaction. In the present work we set model-independent upper limits in the energy range 1.8-16.8 MeV on neutrino fluxes from unknown sources that improve our previous results, on average, by a factor 2.5. Using the same data set, we first obtain experimental constraints on the diffuse supernova $\bar{\nu}_e$ fluxes in the previously unexplored region below 8 MeV. A search for $\bar{\nu}_e$ in the solar ne…

antineutrinosPhysics - Instrumentation and Detectorssolar flaresmagnetic field: highneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoscintillation counter: liquidelastic scatteringantineutrino/e: particle identification01 natural sciences7. Clean energyneutrino: fluxlaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: supernova26.65.+t010303 astronomy & astrophysicsBorexinoElastic scatteringPhysicsSolar flareSupernova Relic Neutrinosneutrino: energy spectrumS067EB8neutrinosInstrumentation and Detectors (physics.ins-det)neutrino: magnetic momentDiffuse Supernova Neutrino Background3. Good healthSupernovaHomestakeddc:540neutrino: flavorAntineutrinoBorexinoNeutrino97.60.BwHomestake experimentFlareantineutrino/e: fluxAntineutrinos13.15.+G; 26.65.+T; 29.40.Mc; 97.60.Bw; Antineutrinos; Diffuse supernova neutrino background; Neutrinos; Solar flares; Supernova relic neutrinosAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSupernova relic neutrinosupernova relic neutrinosNONuclear physics13.15.+gPE2_2Antineutrinos; Neutrinos; Diffuse supernova neutrino background; Supernova relic neutrinos; Solar flares0103 physical sciencesNeutrino[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinosdiffuse supernova neutrino background010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and Astrophysicsneutrino: particle source29.40.McGran SassoSolar flareSolar Flares13. Climate actionspectralHigh Energy Physics::Experimentexperimental results
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Borexino’s search for low-energy neutrino and antineutrino signals correlated with gamma-ray bursts

2017

International audience; A search for neutrino and antineutrino events correlated with 2350 gamma-ray bursts (GRBs) is performed with Borexino data collected between December 2007 and November 2015. No statistically significant excess over background is observed. We look for electron antineutrinos ( ν¯e ) that inverse beta decay on protons with energies from 1.8  MeV to 15  MeV and set the best limit on the neutrino fluence from GRBs below 8  MeV. The signals from neutrinos and antineutrinos from GRBs that scatter on electrons are also searched for, a detection channel made possible by the particularly radio-pure scintillator of Borexino. We obtain currently the best limits on the neutrino f…

antineutrinoselectronAntineutrinosneutrino: solarPhysics::Instrumentation and Detectorsdata acquisitionSolar neutrino[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical Phenomenalow energy/MeV neutrinosElectrongamma ray: burst01 natural sciencesNuclear physicsLow energy/MeV neutrino0103 physical sciencesNeutrinoLow energy/MeV neutrinosNeutrinosNuclear Experiment010303 astronomy & astrophysicsGamma-ray burstBorexinoscintillation counterPhysicsflavor010308 nuclear & particles physicsbackgroundgamma-ray burstsneutrinosAntineutrinos; Gamma-ray bursts; Low energy/MeV neutrinos; Neutrinos; Astronomy and AstrophysicsAstronomy and Astrophysicssemileptonic decayantineutrinocorrelation: timeNeutrino detectorInverse beta decayddc:540Scintillation counterreadoutHigh Energy Physics::ExperimentBorexinoGamma-ray burstsNeutrinoGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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