Search results for "Spectral Analysis"

showing 10 items of 105 documents

Inclusion of Instantaneous Influences in the Spectral Decomposition of Causality: Application to the Control Mechanisms of Heart Rate Variability

2021

Heart rate variability is the result of several physiological regulation mechanisms, including cardiovascular and cardiorespiratory interactions. Since instantaneous influences occurring within the same cardiac beat are commonplace in this regulation, their inclusion is mandatory to get a realistic model of physiological causal interactions. Here we exploit a recently proposed framework for the spectral decomposition of causal influences between autoregressive processes [2] and generalize it by introducing instantaneous couplings in the vector autoregressive model (VAR). We show the effectiveness of the proposed approach on a toy model, and on real data consisting of heart period (RR), syst…

Network physiology020206 networking & telecommunicationsSpectral analysis02 engineering and technologyBaroreflexTime–frequency analysisCausality (physics)Stochastic processesAutoregressive modelFrequency domain0202 electrical engineering electronic engineering information engineeringHeart rate variability020201 artificial intelligence & image processingVagal toneBiological systemRegression analysisBeat (music)Mathematics2020 28th European Signal Processing Conference (EUSIPCO)
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Multimode OPOs as Sources for Multipartite Entanglement

2009

We present here multimode OPOs as a source of multimode squeezing and multipartite entanglement of continuous-wave light beams, with applications to the engineering of multimode states of light in the spatial and spectral domains.

OPOSPhysicsQuantum opticsMulti-mode optical fiberInformationSystems_INFORMATIONINTERFACESANDPRESENTATION(e.g.HCI)business.industryComputer Science::Human-Computer InteractionQuantum PhysicsQuantum entanglementMultipartite entanglementOpticsComputerApplications_MISCELLANEOUSQuantum mechanicsLight beamSpectral analysisbusinessOptical filterConference on Lasers and Electro-Optics/International Quantum Electronics Conference
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Operators on Partial Inner Product Spaces: Towards a Spectral Analysis

2014

Given a LHS (Lattice of Hilbert spaces) $V_J$ and a symmetric operator $A$ in $V_J$, in the sense of partial inner product spaces, we define a generalized resolvent for $A$ and study the corresponding spectral properties. In particular, we examine, with help of the KLMN theorem, the question of generalized eigenvalues associated to points of the continuous (Hilbertian) spectrum. We give some examples, including so-called frame multipliers.

Partial inner product spacesPure mathematicsGeneral MathematicsFOS: Physical sciencesresolventLattice (discrete subgroup)01 natural sciencessymbols.namesakeInner product spaceSettore MAT/05 - Analisi MatematicaPIP-spaceframe multipliers}lattices of Hilbert spacesSpectral analysis0101 mathematicsEigenvalues and eigenvectorsMathematical PhysicsMathematicsResolventframe multipliers010102 general mathematicsSpectrum (functional analysis)Spectral propertiesHilbert spaceMathematical Physics (math-ph)010101 applied mathematicssymbolsspectral properties of symmetric operatorsSpectral theory46Cxx 47A10 47B37
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Comparison of proton shower developments in the BGO calorimeter of the Dark Matter Particle Explorer between GEANT4 and FLUKA simulations

2020

The DArk Matter Particle Explorer (DAMPE) is a satellite-borne detector for high-energy cosmic rays and $\gamma$-rays. To fully understand the detector performance and obtain reliable physical results, extensive simulations of the detector are necessary. The simulations are particularly important for the data analysis of cosmic ray nuclei, which relies closely on the hadronic and nuclear interactions of particles in the detector material. Widely adopted simulation softwares include the GEANT4 and FLUKA, both of which have been implemented for the DAMPE simulation tool. Here we describe the simulation tool of DAMPE and compare the results of proton shower properties in the calorimeter from t…

Physics - Instrumentation and DetectorsProton85Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHadronDark matterS-General Physics and AstronomyFOS: Physical sciencesCosmic rayNuclear physicsSpectral analysisInstrumentation and Methods for Astrophysics (astro-ph.IM)Monte Carlo simulationPhysicsTp9550Calorimeter (particle physics)96DetectorInstrumentation and Detectors (physics.ins-det)5513Cosmic Rays-n-tParticleHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for Astrophysics
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SPI/INTEGRAL observation of the Cygnus region

2003

We present the analysis of the first observations of the Cygnus region by the SPI spectrometer onboard the Integral Gamma Ray Observatory, encompassing ${\sim}$ 600 ks of data. Three sources namely Cyg X-1, Cyg X-3 and EXO 2030+375 were clearly detected. Our data illustrate the temporal variability of Cyg X-1 in the energy range from 20 keV to 300 keV. The spectral analysis shows a remarkable stability of the Cyg X-1 spectra when averaged over one day timescale. The other goal of these observations is SPI inflight calibration and performance verification. The latest objective has been achieved as demonstrated by the results presented in this paper.

Physics010504 meteorology & atmospheric sciencesSpectrometerAstrophysics (astro-ph)Gamma rayFOS: Physical sciencesobservations [gamma rays]Astronomy and AstrophysicsAstrophysicsphysics [black hole]Astrophysics01 natural sciencesSpectral line[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Space and Planetary ScienceObservatory0103 physical sciencesCalibrationindividual : Cyg X-1 Cyg X-3 EXO 2030+375 [X-ray stars]INTEGRAL : SPI [space telescope]Spectral analysis010303 astronomy & astrophysics0105 earth and related environmental sciences
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Analytic solutions and Singularity formation for the Peakon b--Family equations

2012

This paper deals with the well-posedness of the b-family equation in analytic function spaces. Using the Abstract Cauchy-Kowalewski theorem we prove that the b-family equation admits, locally in time, a unique analytic solution. Moreover, if the initial data is real analytic and it belongs to H s with s>3/2, and the momentum density u 0-u 0, xx does not change sign, we prove that the solution stays analytic globally in time, for b≥1. Using pseudospectral numerical methods, we study, also, the singularity formation for the b-family equations with the singularity tracking method. This method allows us to follow the process of the singularity formation in the complex plane as the singularity a…

PhysicsAbstract Cauchy-Kowalewski theoremApplied MathematicsNumerical analysisComplex singularitiesNumerical Analysis (math.NA)Spectral analysisFourier spectrumRate of decayPeakonAnalytic solutionMomentumSingularityMathematics - Analysis of PDEsb-family equationFOS: MathematicsSpectral analysis Complex singularities b-family equation Analytic solution Abstract Cauchy-Kowalewski theoremMathematics - Numerical AnalysisComplex planeSettore MAT/07 - Fisica MatematicaMathematical physicsSign (mathematics)Analysis of PDEs (math.AP)
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On the origin of the X-ray emission from Herbig Ae/Be stars

2006

We performed a systematic search for Chandra archival observations of Herbig Ae/Be stars. These stars are fully radiative and not expected to support dynamo action analogous to their convective lower-mass counterparts, the T Tauri stars. Their X-ray emission has remained unexplained. The superior spatial resolution of Chandra with respect to previous X-ray instrumentation has allowed us to examine the possible role of late-type companions in generating the observed X-rays. In the total sample of 17 Herbig Ae/Be stars, 8 are resolved from X-ray emitting faint companions or other unrelated X-ray bright objects within 10". The detection fraction of Herbig Ae/Be stars is 76 %, but lowers to 35 …

PhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)X-rayFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsLarge rangeAstrophysicsStarsT Tauri starSpace and Planetary ScienceRadiative transferAstrophysics::Solar and Stellar AstrophysicsSpectral analysisAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy AstrophysicsDynamoSystematic searchAstronomy & Astrophysics
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Spectral Analysis of Individual Terrestrial Gamma-ray Flashes Detected by ASIM

2021

The Atmosphere-Space Interactions Monitor (ASIM) is the first instrument in space specifically designed to observe terrestrial gamma-ray flashes (TGFs). TGFs are high energy photons associated with lightning flashes and we perform the spectral analysis of 17 TGFs detected by ASIM. The TGF sample is carefully selected by rigorous selection criteria to keep a clean sample suitable for spectral analysis, that is, suitable count statistics, low instrumental effects, and reliable source location. Monte Carlo modeling of individual TGFs has been compared to the observed energy spectra to study the possible source altitudes and beaming geometries. A careful model of the instrumental effects has be…

PhysicsAtmospheric ScienceGeophysicsSpace and Planetary ScienceEarth and Planetary Sciences (miscellaneous)Gamma raySpectral analysisAstrophysicsLightning
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Analysis of high-harmonic generation in terms of complex Floquet spectral analysis

2017

Recent developments on intense laser sources is opening a new field of optical sciences. An intense coherent light beam strongly interacting with the matter causes a coherent motion of a particle, forming a strongly dressed excited particle. A photon emission from this dressed excited particle is a strong nonlinear process causing high-harmonic generation (HHG), where the perturbation analysis is broken down. In this work, we study a coherent photon emission from a strongly dressed excited atom in terms of complex spectral analysis in the extended Floquet-Hilbert-space. We have obtained the eigenstates of the total Hamiltonian with use of Feshbach-Brilloiun-Wigner projection method. In this…

PhysicsFloquet theoryQuantum PhysicsPhotonElectromagneticsFloquet spectral analysisTime evolutionFOS: Physical sciencesHigh harmonic generationsymbols.namesakeSingularityExcited statesymbolsHigh harmonic generationPhysics::Atomic PhysicsAtomic physicsHamiltonian (quantum mechanics)Quantum Physics (quant-ph)Physics - OpticsOptics (physics.optics)
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Broadband spectral analysis of MXB 1659−298 in its soft and hard state

2018

The X-ray transient eclipsing source MXB 1659-298 went into outburst in 1999 and 2015. During these two outbursts the source was observed by XMM-Newton, nuSTAR, and Swift/XRT. Using these observations, we studied the broadband spectrum of the source to constrain the continuum components and to verify whether it had a reflection component, as is observed in other X-ray eclipsing transient sources. We combined the available spectra to study the soft and hard state of the source in the 0.45-55 keV energy range. We report a reflection component in the soft and hard state. The direct emission in the soft state can be modeled with a thermal component originating from the inner accretion disk plus…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)stars: individual: MXB 1659−298010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical Phenomenaaccretion disksFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics01 natural sciencesAccretion (astrophysics)stars: neutronX-rays: binariesAccretion discaccretionSpace and Planetary ScienceAccretion disk0103 physical sciencesBroadbandAstrophysics::Solar and Stellar AstrophysicsSpectral analysisAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]010303 astronomy & astrophysicsStars: individual: MXB 1659-298
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