Search results for "methods"

showing 10 items of 4526 documents

Overview of Other Results and Open Problems

2014

This chapter presents an overview of results related to error control methods, which were not considered in previous chapters. In the first part, we discuss possible extensions of the theory exposed in Chaps. 3 and 4 to nonconforming approximations and certain classes of nonlinear problems. Also, we shortly discuss some results related to explicit evaluation of modeling errors. The remaining part of the chapter is devoted to a posteriori estimates of errors in iteration methods. Certainly, the overview is not complete. A posteriori error estimation methods are far from having been fully explored and this subject contains many unsolved problems and open questions, some of which we formulate …

Nonlinear systemComputer scienceIterative methodSection (archaeology)Variational inequalityCalculusA priori and a posterioriSubject (documents)Estimation methodsError detection and correction
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Gain-scheduled H-infinity observer design for nonlinear stochastic systems with time-delay and actuator saturation

2012

In this paper, we propose a method for designing continuous gain-scheduled robust H ∞ observer on a class of extended stochastic nonlinear systems subject to time delay and actuator saturation. Initially, gradient linearization procedure is applied to describe such extended nonlinear systems into several model-based linear systems. Next, a robust linear H ∞ observer is designed to such linear stochastic models. Subsequently, a convex hull set is investigated and sufficient condition is derived in terms of feedback observer to determine whether a given initial condition belongs to an ellipsoid invariant set. Finally, continuous gain-scheduled approach is employed to design continuous nonline…

Nonlinear systemH-infinity methods in control theoryObserver (quantum physics)Stochastic modellingLinearizationControl theoryLinear systemInitial value problemRobust controlMathematics2012 American Control Conference (ACC)
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MAST-2D diffusive model for flood prediction on domains with triangular Delaunay unstructured meshes

2011

Abstract A new methodology for the solution of the 2D diffusive shallow water equations over Delaunay unstructured triangular meshes is presented. Before developing the new algorithm, the following question is addressed: it is worth developing and using a simplified shallow water model, when well established algorithms for the solution of the complete one do exist? The governing Partial Differential Equations are discretized using a procedure similar to the linear conforming Finite Element Galerkin scheme, with a different flux formulation and a special flux treatment that requires Delaunay triangulation but entire solution monotonicity. A simple mesh adjustment is suggested, that attains t…

Nonlinear systemMathematical optimizationDiscretizationDelaunay triangulationCourant–Friedrichs–Lewy conditionshallow waters numerical methods finite element method diffusive model unstructured meshes Delaunay triangulations Voronoi cells unsteady flow backwater effect analytical solutionLinear systemApplied mathematicsGalerkin methodShallow water equationsFinite element methodWater Science and TechnologyMathematics
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640-Slice CT Measurement of Superior Orbital Fissure as Gateway for Light into the Brain: Statistical Evaluation of Area and Distance.

2016

Objective Our aim was to provide normative data concerning superior orbital fissure area (SOFA), ocular skin and the substantia nigra (D-SS) and orbital fissure and the substantia nigra (D-SOF-S) distances by CT scan in adult Caucasian population. Methods The area of the superior orbital fissure (SOF), the distance between the ocular skin and the substantia nigra and the distance between the superior orbital fissure and the substantia nigra using CT and 3D-CT images. Results Normative data stratified for age and gender were obtained. The data here reported show that some degree of variability in SOFA, D-SS and D-SOF-S measurements can be observed healthy Caucasian subjects. Gender stratifie…

Normal Distributionlcsh:MedicineComputed tomographyDistance MeasurementNervous System030218 nuclear medicine & medical imagingDiagnostic RadiologyMidbrain0302 clinical medicineMedicine and Health SciencesMedicineCaucasian populationlcsh:ScienceTomographyMeasurementMultidisciplinaryMovement Disordersmedicine.diagnostic_testNervesOrbital fissureRadiology and ImagingCranial NervesBrainNeurodegenerative DiseasesParkinson DiseaseSubstantia Nigramedicine.anatomical_structureNeurologySuperior orbital fissurePhysical SciencesEngineering and TechnologyAnatomyBrainstemBright lightResearch ArticleImaging TechniquesOcular AnatomySubstantia nigraNeuroimagingResearch and Analysis MethodsMidbrain03 medical and health sciencesDiagnostic MedicineOcular SystemPathologicalbusiness.industrylcsh:RBiology and Life SciencesProbability TheoryProbability DistributionComputed Axial Tomographylcsh:QbusinessNuclear medicine030217 neurology & neurosurgeryMathematicsNeurosciencePloS one
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SEARCHES FOR POINT-LIKE AND EXTENDED NEUTRINO SOURCES CLOSE TO THE GALACTIC CENTER USING THE ANTARES NEUTRINO TELESCOPE

2014

A search for cosmic neutrino sources using six years of data collected by the ANTARES neutrino telescope has been performed. Clusters of muon neutrinos over the expected atmospheric background have been looked for. No clear signal has been found. The most signal-like accumulation of events is located at equatorial coordinates R.A. = -46º.8 and decl. = -64º.9 and corresponds to a 2.2 sigma background fluctuation. In addition, upper limits on the flux normalization of an E-2 muon neutrino energy spectrum have been set for 50 pre-selected astrophysical objects. Finally, motivated by an accumulation of seven events relatively close to the Galactic Center in the recently reported neutrino sample…

Normalization (statistics)AstrofísicaParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Physics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicslaw.inventionHigh Energy Physics - ExperimentTelescopeHigh Energy Physics - Experiment (hep-ex)neutrinolaw[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Point (geometry)Muon neutrinoNeutrinsNeutrinosInstrumentation and Methods for Astrophysics (astro-ph.IM)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuonCOSMIC cancer databaseGalaxy: center[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]astroparticle physicFísicaneutrinosAstronomy and Astrophysicscenter [Galaxy]Galaxy centerNeutrino astrophysics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]13. Climate actionSpace and Planetary Scienceastroparticle physicsFISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]High Energy Physics::ExperimentNeutrinoAstroparticle physicsMATEMATICA APLICADAAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsastroparticle physics; Galaxy: center; neutrinos
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Biproportional methods of structural change analysis: A typological survey

2004

International audience; Analysts often are interested in learning how much an exchange system has changed over time or how two different exchange systems differ. Identifying structural difference in exchange matrices can be performed using either 'directed' or 'undirected' methods. Directed methods are based on the computation and comparison of column- or row-normalizations of the matrices. The choice of row or column for the normalization implies a specific direction of the exchanges, so that the column-wise normalized results should not be compared to the row-wise normalized results. In this category fall the simple comparison of coefficient matrices and the causative method. Undirected m…

Normalization (statistics)JEL : C - Mathematical and Quantitative Methods/C.C6 - Mathematical Methods • Programming Models • Mathematical and Simulation Modeling/C.C6.C67 - Input–Output ModelsEconomics and EconometricsJEL: C - Mathematical and Quantitative Methods/C.C6 - Mathematical Methods • Programming Models • Mathematical and Simulation Modeling/C.C6.C67 - Input–Output Modelscausative matrixComputationJEL: D - Microeconomics/D.D5 - General Equilibrium and Disequilibrium/D.D5.D57 - Input–Output Tables and AnalysisStructural difference[SHS.ECO]Humanities and Social Sciences/Economics and Financemathematical economicsinput-output analysisJEL: C - Mathematical and Quantitative Methods/C.C6 - Mathematical Methods • Programming Models • Mathematical and Simulation Modeling/C.C6.C63 - Computational Techniques • Simulation ModelingJEL : C - Mathematical and Quantitative Methods/C.C6 - Mathematical Methods • Programming Models • Mathematical and Simulation Modeling/C.C6.C63 - Computational Techniques • Simulation ModelingbiproportionMedian filterJEL : D - Microeconomics/D.D5 - General Equilibrium and Disequilibrium/D.D5.D57 - Input–Output Tables and Analysis[ SHS.ECO ] Humanities and Social Sciences/Economies and finances[SHS.ECO] Humanities and Social Sciences/Economics and FinanceAlgorithmMathematicsRAS
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Oscillating nuclear electric dipole moments inside atoms

2019

Interaction with the axion dark matter (DM) field generates an oscillating nuclear electric dipole moment (EDM) with a frequency corresponding to the axion's Compton frequency. Within an atom, an oscillating EDM can drive electric dipole transitions in the electronic shell. In the absence of radiation, and if the axion frequency matches a dipole transition, it can promote the electron into the excited state. The excitation events can be detected, for example, via subsequent uorescence or photoionization. Here we calculate the rates of such transitions. For a single light atom and an axion Compton frequency resonant with a transition energy corresponding to 1 eV, the rate is on the order of …

Nuclear Theory (nucl-th)Nuclear TheoryAtomic Physics (physics.atom-ph)FOS: Physical sciencesPhysics::Atomic PhysicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics - Atomic Physics
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Determination of accurate rest frequencies and hyperfine structure parameters of cyanobutadiyne, HC5N

2020

Very accurate transition frequencies of HC$_5$N were determined between 5.3 and 21.4 GHz with a Fourier transform microwave spectrometer. The molecules were generated by passing a mixture of HC$_3$N and C$_2$H$_2$ highly diluted in neon through a discharge valve followed by supersonic expansion into the Fabry-Perot cavity of the spectrometer. The accuracies of the data permitted us to improve the experimental $^{14}$N nuclear quadrupole coupling parameter considerably and the first experimental determination of the $^{14}$N nuclear spin-rotation parameter. The transition frequencies are also well suited to determine in astronomical observations the local speed of rest velocities in molecula…

Nuclear TheoryFOS: Physical scienceschemistry.chemical_element010402 general chemistry01 natural sciencesNeonsymbols.namesakePhysics - Chemical Physics0103 physical sciencesPhysics - Atomic and Molecular ClustersPhysical and Theoretical ChemistryInstrumentation and Methods for Astrophysics (astro-ph.IM)Hyperfine structureSpectroscopyChemical Physics (physics.chem-ph)CouplingPhysics010304 chemical physicsSpectrometerAstrophysics - Astrophysics of GalaxiesAtomic and Molecular Physics and Optics0104 chemical sciencesFourier transformchemistryCoupling parameterAstrophysics of Galaxies (astro-ph.GA)QuadrupolesymbolsRotational spectroscopyAtomic physicsAstrophysics - Instrumentation and Methods for AstrophysicsAtomic and Molecular Clusters (physics.atm-clus)Journal of Molecular Spectroscopy
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First Results on the Scalar WIMP-Pion Coupling, Using the XENON1T Experiment

2018

We present first results on the scalar coupling of weakly interacting massive particles (WIMPs) to pions from 1 t yr of exposure with the XENON1T experiment. This interaction is generated when the WIMP couples to a virtual pion exchanged between the nucleons in a nucleus. In contrast to most nonrelativistic operators, these pion-exchange currents can be coherently enhanced by the total number of nucleons and therefore may dominate in scenarios where spin-independent WIMP-nucleon interactions are suppressed. Moreover, for natural values of the couplings, they dominate over the spin-dependent channel due to their coherence in the nucleus. Using the signal model of this new WIMP-pion channel, …

Nuclear TheoryPhysics::Instrumentation and DetectorsNuclear TheoryGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)WIMPPions[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentS030UDMPhysicsStarke Wechselwirkung und exotische Kerne – Abteilung BlaumAstrophysics::Instrumentation and Methods for AstrophysicsnucleonsuppressionHigh Energy Physics - PhenomenologyWeakly interacting massive particlesmedicine.anatomical_structureWeakly interacting massive particlesNucleonCoherence (physics)Astrophysics - Cosmology and Nongalactic AstrophysicsWIMP nucleon: interactionParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]FOS: Physical sciencesWIMP: massspin: dependenceGravitation and Astrophysicsoperator: nonrelativisticDark matter Particle dark matter Pions Weakly interacting massive particles Dark matter detectorsNuclear Theory (nucl-th)PionParticle dark matter0103 physical sciencesmedicineDark mattercross section: upper limit010306 general physicsCouplingDark matter detectorsnucleusScalar (physics)coherenceDark Matter WIMP-Pion coupling Xenon Direct seartch[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Experiment[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Nucleus
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What is the final state of a black hole merger?

2018

In this short paper we discuss the possibility of testing the nature of astrophysical black holes using the recently observed black hole mergers. We investigate the possibility that a secondary black hole is created in the merger of two astrophysical black holes and discuss potential astrophysical signatures. We point out that black hole mergers are a possible astrophysical mechanism for the creation of quantum black holes with masses close to the Planck mass.

Nuclear and High Energy PhysicsBlack holeAstrophysics::High Energy Astrophysical PhenomenaShort paperPlanck massFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical sciencesquantum black holes.10. No inequality010306 general physicsQuantumQBPhysics010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsBlack holeblack hole mergerquantum gravityQuantum gravityModern Physics Letters A
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