Search results for "Detector"

showing 10 items of 3491 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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Searches for anisotropies in the arrival directions of the highest energy cosmic rays detected by the Pierre Auger Observatory

2015

We analyze the distribution of arrival directions of ultra-high energy cosmic rays recorded at the Pierre Auger Observatory in 10 years of operation. The data set, about three times larger than that used in earlier studies, includes arrival directions with zenith angles up to $80^\circ$, thus covering from $-90^\circ$ to $+45^\circ$ in declination. After updating the fraction of events correlating with the active galactic nuclei (AGNs) in the V��ron-Cetty and V��ron catalog, we subject the arrival directions of the data with energies in excess of 40 EeV to different tests for anisotropy. We search for localized excess fluxes and for self-clustering of event directions at angular scales up t…

acceleration of particles; astroparticle physicsNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Upper LimitAstronomyCiencias FísicasAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFieldCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsOtras Ciencias Físicas01 natural sciencesSettore FIS/04 - Fisica Nucleare e SubnucleareSettore FIS/05 - Astronomia e AstrofisicaObservatorySpectrum0103 physical sciencesacceleration of particles astroparticle physicsSurface Detector010303 astronomy & astrophysicsacceleration of particleAstrophysics::Galaxy Astrophysicsacceleration of particlesPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleArrayAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]astroparticle physicAstronomy and AstrophysicsASTROFÍSICANucleiSpace and Planetary Scienceastroparticle physicsExperimental High Energy Physicsacceleration of particles; astroparticle physics; Nuclear and High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearCatalogSkyAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS
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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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The Pros and Cons of Beyond Standard Model Interpretations of ANITA Events

2019

The Antarctic Impulsive Transient Antenna (ANITA) experiment has observed two air shower events with energy $\sim 500~{\rm PeV}$ emerging from the Earth with exit angles $\sim 30^\circ$ above the horizon. As was immediately noted by the ANITA Collaboration, these events (in principle) could originate in the atmospheric decay of an upgoing $\tau$-lepton produced through a charged current interaction of a $\nu_\tau$ inside the Earth. However, the relatively steep arrival angles of these perplexing events create tension with the standard model (SM) neutrino-nucleon interaction cross section. Deepening the conundrum, the IceCube neutrino telescope and the Pierre Auger Observatory with substanti…

airAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesparticle: messengerAstrophysics01 natural scienceshorizonneutrino nucleon: interactioncharged currentIceCubeHigh Energy Physics - Phenomenology (hep-ph)Observatory0103 physical sciences010306 general physicsCharged currentHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger Observatoryneutrino/tauCOSMIC cancer databaseshowers: atmosphere010308 nuclear & particles physicsHorizonANITAAstrophysics::Instrumentation and Methods for AstrophysicstensionsensitivityAugerfluxobservatoryHigh Energy Physics - Phenomenologyneutrino: detectorAir showerNeutrino detector[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Astrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)Proceedings of 36th International Cosmic Ray Conference — PoS(ICRC2019)
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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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