Search results for "wave"

showing 10 items of 6009 documents

Zewnątrzustrojowa Fala Uderzeniowa (ESW) jako alternatywna metoda wspomagająca terapię porażenia spastycznego mięśni kończyn w wyniku udaru mózgu - p…

2017

Zewnątrzustrojowa fala uderzeniowa (ESW – Extracorporeal Shock Wave) jest czynnikiem fizykalnym, którego zastosowanie kliniczne obserwowane jest w szerokiej gamie zaburzeń chorobowych, szczególnie dysfunkcji narządu ruchu. Obecnie zaobserwować można, iż lista wskazań do zabiegów ESW stale rośnie i obejmuje swym zasięgiem coraz to bardziej odmienne pod względem etiologii i patomechanizmu schorzenia ogólnoustrojowe. Niemniej jednak pamiętać należy, iż potencjalne mechanizmy biologiczne stymulacji ESW, warunkujące korzystne i pożądane efekty terapeutyczne, nie są jednoznacznie wyjaśnione. W świecie nauki w dalszym ciągu obserwowany jest brak niepodważalnych dowodów popartych zaawansowanymi bad…

post-stroke spasticitymuscles’ hypertonianeurorehabilitationpoudarowa spastycznośćprzegląd piśmiennictwaliterature reviewfizjoterapiashock wavesneurorehabilitacjahipertonia mięśniowaphysiotherapyfala uderzeniowaWiadomości Lekarskie
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Evaluation of Clutch Plate Integrity with Non-Destructive Methods

2009

Abstract Nondestructive evaluation (NDE) represents an important phase in the life cycle of a product to detect defects both in service and in production. NDE techniques most commonly used to detect surface defects are visual inspection and methods based on eddy current and ultrasound. Laser and non-contact sensors have been recently used to inspect ultrasonically without contact. Components with complex geometry are usually inspected combining several NDE techniques, or simply visually where analysis and evaluation of results are performed by an operator based on specific parameters of acceptance. This last method is currently used to inspect the clutch plates since their complex geometry,…

product life cycle product control laser ultrasound guided wavesSettore ING-IND/15 - Disegno E Metodi Dell'Ingegneria Industriale
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Cubic color charge correlator in a proton made of three quarks and a gluon

2022

The three point correlation function of color charge densities is evaluated explicitly in light cone gauge for a proton on the light cone. This includes both $C$-conjugation even and odd contributions. We account for perturbative corrections to the three-quark light cone wave function due to the emission of an internal gluon which is not required to be soft. We verify the Ward identity as well as the cancellation of UV divergences in the sum of all diagrams so that the correlator is independent of the renormalization scale. It does, however, exhibit the well known soft and collinear singularities. The expressions derived here provide the $C$-odd contribution to the initial conditions for hi…

protonitGLASS CONDENSATEkvarkitMESON PRODUCTIONFOS: Physical sciencesELECTROPRODUCTIONhiukkasfysiikka114 Physical sciencesEVOLUTIONHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)ODDERONEQUATIONINELASTIC EP SCATTERINGWAVE-FUNCTIONBEHAVIOR
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Controlling Atom-Photon Bound States in an Array of Josephson-Junction Resonators

2022

Engineering the electromagnetic environment of a quantum emitter gives rise to a plethora of exotic light -matter interactions. In particular, photonic lattices can seed long-lived atom-photon bound states inside photonic band gaps. Here, we report on the concept and implementation of a novel microwave architecture consisting of an array of compact superconducting resonators in which we have embedded two frequency -tunable artificial atoms. We study the atom-field interaction and access previously unexplored coupling regimes, in both the single-and double-excitation subspace. In addition, we demonstrate coherent interactions between two atom-photon bound states, in both resonant and dispers…

quantumPhotonics:Física [Àrees temàtiques de la UPC]latticesFotònicaedgeGeneral Physics and Astronomylight-matter interactionsCircuit QED. Waveguide QED. Quantum information processing implementationsSettore FIS/03 - Fisica Della Materia
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Numerical treatment of radiation processes in the internal shocks of magnetized relativistic outflows

2017

Los blázares son un tipo de núcleo activo de galaxia (AGN, por sus siglas en inglés) que se encuentran entre los objetos astrofísicos más energéticos y violentos, a la par de los brotes de rayos gamma (GRB por sus siglas en inglés). Los procesos físicos y, en particular, el escenario del chorro relativista en el que se genera la radiación ultraenergética detectada por observatorios terrestres y en órbita, han conseguido atraer la atención e interés de los astrónomos y astrofísicos desde su descubrimiento. En la presente tesis investigamos el modelo de choques internos (IS) cuya hipótesis consta del choque de dos capas de plasma con geometría cilíndrica, formando dos ondas de choque que atra…

radiation mechanisms: thermalradiation mechanisms: nonthermalradiative transferthermal [radiation mechanisms]numerical methodsgeneral [bl lacertae objects]nonthermal [radiation mechanisms]shock wavesUNESCO::ASTRONOMÍA Y ASTROFÍSICAmagnetohydrodynamics:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]bl lacertae objects: general
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Generalized wave propagation problems and discrete exterior calculus

2018

We introduce a general class of second-order boundary value problems unifying application areas such as acoustics, electromagnetism, elastodynamics, quantum mechanics, and so on, into a single framework. This also enables us to solve wave propagation problems very efficiently with a single software system. The solution method precisely follows the conservation laws in finite-dimensional systems, whereas the constitutive relations are imposed approximately. We employ discrete exterior calculus for the spatial discretization, use natural crystal structures for three-dimensional meshing, and derive a “discrete Hodge” adapted to harmonic wave. The numerical experiments indicate that the cumulat…

raja-arvotHelmholtz equationDiscretizationWave propagationboundary value problemssähkömagnetismielectromagnetism010103 numerical & computational mathematics02 engineering and technologyalgebra01 natural sciencesdiscrete exterior calculusdifferentiaaligeometriaakustiikka0202 electrical engineering electronic engineering information engineeringApplied mathematicsBoundary value problemkvanttimekaniikkadifferential geometry0101 mathematicsacousticsMathematicsta113Numerical AnalysisConservation lawfinite differenceApplied MathematicsFinite difference020206 networking & telecommunicationsFinite element methodComputational MathematicsDiscrete exterior calculusModeling and SimulationelasticityAnalysisexterior algebra
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Topological canal foliations

2019

Regular canal surfaces of $\mathbb{R}^3$ or $\mathbb{S}^3$ admit foliations by circles: the characteristic circles of the envelope. In order to build a foliation of $\mathbb{S}^3$ with leaves being canal surfaces, one has to relax the condition “canal” a little (“weak canal condition”) in order to accept isolated umbilics. Here, we define a topological condition which generalizes this “weak canal” condition imposed on leaves, and classify the foliations of compact orientable 3-manifolds we can obtain this way.

rational parametrizationsQuantitative Biology::Tissues and OrgansGeneral MathematicsPhysics::Medical PhysicssurfacesTopology01 natural sciencesQuantitative Biology::Cell Behavior0103 physical sciencesotorhinolaryngologic diseases57R30[MATH]Mathematics [math]0101 mathematicsMathematicsEnvelope (waves)griddlingQuantitative Biology::Molecular Networks010102 general mathematicsOrder (ring theory)53C12foliationFoliation (geology)sense organsMathematics::Differential Geometry010307 mathematical physicscanal surfaceJournal of the Mathematical Society of Japan
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Acoustic wave guides as infinite-dimensional dynamical systems

2015

We prove the unique solvability, passivity/conservativity and some regularity results of two mathematical models for acoustic wave propagation in curved, variable diameter tubular structures of finite length. The first of the models is the generalised Webster's model that includes dissipation and curvature of the 1D waveguide. The second model is the scattering passive, boundary controlled wave equation on 3D waveguides. The two models are treated in an unified fashion so that the results on the wave equation reduce to the corresponding results of approximating Webster's model at the limit of vanishing waveguide intersection.

regularityControl and OptimizationDynamical systems theoryWave propagationwave propagationDynamical Systems (math.DS)Curvaturelaw.inventionMathematics - Analysis of PDEslawWebster’s horn modelFOS: MathematicspassivityMathematics - Dynamical SystemsMathematicstubular domainMathematical modelta111Mathematical analysisAcoustic waveDissipationWave equationPrimary 35L05 secondary 35L20 93C20 47N70Computational MathematicsControl and Systems Engineering: Mathematics [G03] [Physical chemical mathematical & earth Sciences]wave equation: Mathématiques [G03] [Physique chimie mathématiques & sciences de la terre]WaveguideAnalysis of PDEs (math.AP)ESAIM: Control, Optimisation and Calculus of Variations
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Rotational effects on the oscillation frequencies of newly born proto-neutron stars

2003

In this paper we study the effects of rotation on the frequencies of the quasi-normal modes of a proto-neutron star (PNS) born in a gravitational collapse during the first minute of life. Our analysis starts a few tenths of seconds after the PNS formation, when the stellar evolution can be described by a sequence of equilibrium configurations. We use the evolutionary models developed by Pons et al. (1999; 2001) that describe how a non rotating star cools down and contracts while neutrino diffusion and thermalization processes dominate the stellar dynamics. For assigned values of the evolution time, we set the star into slow rotation and integrate the equations of stellar perturbations in th…

relativityFOS: Physical sciencesmethods : numericalAstrophysicsAstrophysicsInstabilitystars : oscillationsmethods: numericalstars: neutronstars: rotationstars : rotationStellar dynamicsGravitational collapseAstrophysics::Solar and Stellar AstrophysicsTime domainStellar evolutionPhysicsgravitational waves; methods : numerical; methods: numerical; relativity; stars : neutron; stars : oscillations; stars : rotation; stars: neutron; stars: oscillations; stars: rotationAstrophysics (astro-ph)Astronomy and Astrophysicsstars : neutronNeutron stargravitational wavesSpace and Planetary ScienceFrequency domainstars: oscillationsAstrophysics::Earth and Planetary AstrophysicsNeutrinoMonthly Notices of the Royal Astronomical Society
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8-parameter solutions of fifth order to the Johnson equation

2019

We give different representations of the solutions of the Johnson equation with parameters. First, an expression in terms of Fredholm determinants is given; we give also a representation of the solutions written as a quotient of wronskians of order 2N. These solutions of order N depend on 2N − 1 parameters. When one of these parameters tends to zero, we obtain N order rational solutions expressed as a quotient of two polyno-mials of degree 2N (N +1) in x, t and 4N (N +1) in y depending on 2N −2 parameters. Here, we explicitly construct the expressions of the rational solutions of order 5 depending on 8 real parameters and we study the patterns of their modulus in the plane (x, y) and their …

rogue waves PACS numbers : 33Q55ratio- nal solutionswronskiansrational solutions[MATH.MATH-MP]Mathematics [math]/Mathematical Physics [math-ph]Johnson equation4710A-[MATH.MATH-MP] Mathematics [math]/Mathematical Physics [math-ph]37K104735Fg4754BdFredholm determinants
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