Search results for "FOS"

showing 10 items of 15075 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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Reliable numerical solution of a class of nonlinear elliptic problems generated by the Poisson-Boltzmann equation

2020

We consider a class of nonlinear elliptic problems associated with models in biophysics, which are described by the Poisson-Boltzmann equation (PBE). We prove mathematical correctness of the problem, study a suitable class of approximations, and deduce guaranteed and fully computable bounds of approximation errors. The latter goal is achieved by means of the approach suggested in [S. Repin, A posteriori error estimation for variational problems with uniformly convex functionals. Math. Comp., 69:481-500, 2000] for convex variational problems. Moreover, we establish the error identity, which defines the error measure natural for the considered class of problems and show that it yields computa…

a priori error estimatesClass (set theory)Correctness010103 numerical & computational mathematics01 natural sciencesMeasure (mathematics)guaranteed and efficient a posteriori error boundsFOS: MathematicsApplied mathematicsPolygon meshMathematics - Numerical Analysis0101 mathematicserror indicators and adaptive mesh refinementMathematicsNumerical AnalysisApplied MathematicsRegular polygonNumerical Analysis (math.NA)convergence of finite element approximationsLipschitz continuity010101 applied mathematicsComputational MathematicsNonlinear systemexistence and uniqueness of solutionssemilinear partial differential equations65J15 49M29 65N15 65N30 65N50 35J20MathematikA priori and a posterioriPoisson-Boltzmann equationdifferentiaaliyhtälöt
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Excitons in few-layer hexagonal boron nitride: Davydov splitting and surface localization

2018

Hexagonal boron nitride (hBN) has been attracting great attention because of its strong excitonic effects. Taking into account few-layer systems, we investigate theoretically the effects of the number of layers on quasiparticle energies, absorption spectra, and excitonic states, placing particular focus on the Davydov splitting of the lowest bound excitons. We describe how the inter-layer interaction as well as the variation in electronic screening as a function of layer number $N$ affects the electronic and optical properties. Using both \textit{ab initio} simulations and a tight-binding model for an effective Hamiltonian describing the excitons, we characterize in detail the symmetry of t…

ab-initio many-body perturbation theoryAb initio02 engineering and technology01 natural sciences[SPI.MAT]Engineering Sciences [physics]/MaterialsTight bindingtight-bindingGeneral Materials ScienceOPTICAL ABSORPTIONWave functionmedia_commonPhysicsCondensed Matter - Materials ScienceCondensed matter physics021001 nanoscience & nanotechnologyCondensed Matter PhysicsCondensed Matter::Mesoscopic Systems and Quantum Hall Effect: Physique [G04] [Physique chimie mathématiques & sciences de la terre]Mechanics of MaterialsMATERIAUX 2DTIGHT-BINDINGQuasiparticlesymbols0210 nano-technologyHamiltonian (quantum mechanics)excitonsAbsorption spectroscopyExcitonmedia_common.quotation_subject: Physics [G04] [Physical chemical mathematical & earth Sciences]HEXAGONAL BORON NITRIDEFOS: Physical sciencesEXCITONAsymmetryBNsymbols.namesakeCondensed Matter::Materials ScienceFIRST-PRINCIPLES CALCULATIONS0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)hexagonal boron nitride010306 general physicsCondensed Matter::Quantum GasesCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed Matter::OtherEXCITONSMechanical EngineeringMaterials Science (cond-mat.mtrl-sci)Davydov splittingGeneral Chemistry
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Time-dependent screening explains the ultrafast excitonic signal rise in 2D semiconductors

2020

We calculate the time evolution of the transient reflection signal in an MoS$_2$ monolayer on a SiO$_2$/Si substrate using first-principles out-of-equilibrium real-time methods. Our simulations provide a simple and intuitive physical picture for the delayed, yet ultrafast, evolution of the signal whose rise time depends on the excess energy of the pump laser: at laser energies above the A- and B-exciton, the pump pulse excites electrons and holes far away from the K valleys in the first Brillouin zone. Electron-phonon and hole-phonon scattering lead to a gradual relaxation of the carriers towards small $\textit{Active Excitonic Regions}$ around K, enhancing the dielectric screening. The acc…

ab-initio many-body perturbation theoryMaterials scienceExciton: Physics [G04] [Physical chemical mathematical & earth Sciences]General Physics and AstronomyFOS: Physical sciences02 engineering and technology010402 general chemistry01 natural sciencesSignalCondensed Matter::Materials ScienceMonolayerGeneral Materials ScienceCondensed Matter - Materials Sciencebusiness.industryGeneral EngineeringTime evolutionMaterials Science (cond-mat.mtrl-sci)Computational Physics (physics.comp-ph)021001 nanoscience & nanotechnologytime-dependent spectroscopy0104 chemical sciencesReflection (mathematics)Semiconductor: Physique [G04] [Physique chimie mathématiques & sciences de la terre]OptoelectronicsTransient (oscillation)0210 nano-technologybusinessUltrashort pulsePhysics - Computational Physicsexciton-phonon couplingPhysics - OpticsOptics (physics.optics)
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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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Study of the accretion torque during the 2014 outburst of the X-ray pulsar GRO J1744−28

2017

We present the spectral and timing analysis of the X-ray pulsar GRO J1744-28 during its 2014 outburst using data collected with the X-ray satellites Swift, INTEGRAL, Chandra, and XMM-Newton. We derived, by phase-connected timing analysis of the observed pulses, an updated set of the source ephemeris. We were also able to investigate the spin-up of the X-ray pulsar as a consequence of the accretion torque during the outburst. Relating the spin-up rate and the mass accretion rate as $\dot{\nu}\propto\dot{M}^{\beta}$, we fitted the pulse phase delays obtaining a value of $\beta=0.96(3)$. Combining the results from the source spin-up frequency derivative and the flux estimation, we constrained …

accretion accretion discAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsEphemeris01 natural sciencesstars: neutronQuadratic equationPulsar0103 physical sciencesTorque010303 astronomy & astrophysicsGroup delay and phase delayHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsneutron; X-rays: binaries; X-rays: individual: GRO J1744-28 [accretion accretion disc; stars]Static timing analysisAstronomy and AstrophysicsX-rays: binarieAccretion (astrophysics)Space and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaX-rays: individual: GRO J1744-28X-ray pulsarMonthly Notices of the Royal Astronomical Society
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The enigmatic young brown dwarf binary FU Tau: accretion and activity

2010

FU Tau belongs to a rare class of young, wide brown dwarf binaries. We have resolved the system in a Chandra X-ray observation and detected only the primary, FU Tau A. Hard X-ray emission, presumably from a corona, is present but, unexpectedly, we detect also a strong and unusually soft component from FU Tau A. Its X-ray properties, so far unique among brown dwarfs, are very similar to those of the T Tauri star TW Hya. The analogy with TW Hya suggests that the dominating soft X-ray component can be explained by emission from accretion shocks. However, the typical free-fall velocities of a brown dwarf are too low for an interpretation of the observed X-ray temperature as post-shock region. O…

accretion accretion discs stars: activity brown dwarfs stars: pre-main-sequence X-rays: starsSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Solar and Stellar AstrophysicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)
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