Search results for "Applied Mathematic"

showing 10 items of 4398 documents

Estimating the temperature evolution of foodstuffs during freezing with a 3D meshless numerical method

2015

Abstract Freezing processes are characterised by sharp changes in specific heat capacity and thermal conductivity for temperatures close to the freezing point. This leads to strong nonlinearities in the governing PDE that may be difficult to resolve using traditional numerical methods. In this work we present a meshless numerical method, based on a local Hermite radial basis function collocation approach in finite differencing mode, to allow the solution of freezing problems. By introducing a Kirchhoff transformation and solving the governing equations in Kirchhoff space, the strength of nonlinearity is reduced while preserving the structure of the heat equation. In combination with the hig…

Work (thermodynamics)Regularized meshless methodRadial basis functionNonlinear heat conductionApplied MathematicsNumerical analysisMathematical analysisGeneral EngineeringMeshleKirchhoff transformationFreezing pointPiecewise linear functionComputational MathematicsNonlinear systemThermal conductivityFreezingSettore ING-IND/10 - Fisica Tecnica IndustrialeHeat equationPhase changeAnalysisMathematicsEngineering Analysis with Boundary Elements
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About the reliability, efficiency, and meaning of the error estimates of a LAOCOON3-type NMR analysis system

1977

Abstract The statistical error estimates of a LAOCOON3-type system are tested. The analyzabilities of a spectrum and spectral parameters are described by a new measure. The variation in the uncertainties of the parameters can be explained by correlation coefficients. According to the calculations made, the error estimates are normally quite reliable if the accuracy of the observed spectrum is known. In some cases the Newton-Raphson type of iteration does not converge or the confidence limits of the parameters are enormous or both; an example is discussed. It seems clear that one cannot avoid differing uncertainties of the parameters by changing the method of analysis, or that one can avoid …

Work (thermodynamics)Spectrum (functional analysis)Line (geometry)General EngineeringApplied mathematicsMeasure (mathematics)QuantumEigenvalues and eigenvectorsConfidence intervalReliability (statistics)MathematicsJournal of Magnetic Resonance (1969)
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Layer-Wise Discontinuous Galerkin Methods for Piezoelectric Laminates

2020

In this work, a novel high-order formulation for multilayered piezoelectric plates based on the combination of variable-order interior penalty discontinuous Galerkin methods and general layer-wise plate theories is presented, implemented and tested. The key feature of the formulation is the possibility to tune the order of the basis functions in both the in-plane approximation and the through-the-thickness expansion of the primary variables, namely displacements and electric potential. The results obtained from the application to the considered test cases show accuracy and robustness, thus confirming the developed technique as a supplementary computational tool for the analysis and design o…

Work (thermodynamics)plate theoriesComputer sciencecomposite materialsdiscontinuous Galerkin methodBasis function02 engineering and technologycomposite material021001 nanoscience & nanotechnologypiezoelectric laminatesPiezoelectricity020303 mechanical engineering & transportsColloid and Surface ChemistryTest case0203 mechanical engineeringRobustness (computer science)Discontinuous Galerkin methodPlate theorypiezoelectric laminateplate theorieApplied mathematicsElectric potentialPhysical and Theoretical ChemistrySettore ING-IND/04 - Costruzioni E Strutture Aerospaziali0210 nano-technologyModelling
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XIPE: the x-ray imaging polarimetry explorer

2016

XIPE, the X-ray Imaging Polarimetry Explorer, is a mission dedicated to X-ray Astronomy. At the time of writing XIPE is in a competitive phase A as fourth medium size mission of ESA (M4). It promises to reopen the polarimetry window in high energy Astrophysics after more than 4 decades thanks to a detector that efficiently exploits the photoelectric effect and to X-ray optics with large effective area. XIPE uniqueness is time-spectrally-spatially- resolved X-ray polarimetry as a breakthrough in high energy astrophysics and fundamental physics. Indeed the payload consists of three Gas Pixel Detectors at the focus of three X-ray optics with a total effective area larger than one XMM mirror bu…

X-ray AstronomyHigh-energy astronomyPolarimetryX-ray opticsX-ray telescopeCondensed Matter Physic01 natural sciencesObservatory0103 physical sciencesPolarimetryElectronicOptical and Magnetic MaterialsSpectral resolutionElectrical and Electronic Engineering010303 astronomy & astrophysicsGas Pixel DetectorPhysicsX-ray astronomyta115X-ray optics010308 nuclear & particles physicsElectronic Optical and Magnetic MaterialApplied MathematicsVegaAstronomyComputer Science Applications1707 Computer Vision and Pattern RecognitionGas Pixel Detector; Polarimetry; X-ray Astronomy; X-ray opticsCondensed Matter PhysicsComputer Science ApplicationsApplied MathematicGas Pixel Detector; Polarimetry; X-ray Astronomy; X-ray optics; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringGas Pixel Detector; Polarimetry; X-ray Astronomy; X-ray optics; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications; Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringComputer Vision and Pattern RecognitionX-ray optic
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ATHENA WFI optical blocking filters development status toward the end of the instrument phase-A

2018

Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. The Wide Field Imager (WFI) is one of the two instruments of the ATHENA astrophysics space mission approved by ESA as the second large mission in the Cosmic Vision 2015-2025 Science Programme. The WFI, based on a large array of depleted field effect transistors (DEPFET), will provide imaging in the 0.2-15 keV band over a 40'x40' field of view, simultaneously with spectrally an…

X-ray detectorCosmic VisionPhotonX-ray detectorWide Field ImagerField of viewCondensed Matter Physic7. Clean energy01 natural sciences010309 opticsX-ray astronomyOpticsSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesAthenaSpectral resolutionElectrical and Electronic EngineeringOptical blocking filter010303 astronomy & astrophysicsPhysicsCMOS sensorbusiness.industryElectronic Optical and Magnetic MaterialDetectorComputer Science Applications1707 Computer Vision and Pattern RecognitionPhoton countingApplied MathematicActive pixel sensor13. Climate actionbusinessDEPFET
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ATHENA X-IFU thermal filters development status toward the end of the instrument phase-A

2018

Copyright 2018 Society of Photo-Optical Instrumentation Engineers (SPIE). One print or electronic copy may be made for personal use only. Systematic reproduction and distribution, duplication of any material in this paper for a fee or for commercial purposes, or modification of the content of the paper are prohibited. The X-ray Integral Field Unit (X-IFU) is one of the two instruments of the Athena astrophysics space mission approved by ESA in the Cosmic Vision 2015-2025 Science Programme. The X-IFU consists of a large array of transition edge sensor micro-calorimeters that will operate at 100 mK inside a sophisticated cryostat. A set of thin filters, highly transparent to X-rays, will be m…

X-ray detectorCryostatCosmic VisionPhotonComputer scienceShieldsCondensed Matter Physicmicrocalorimeter01 natural sciences7. Clean energySettore FIS/05 - Astronomia E AstrofisicaX-ray Integral Field Unit (X-IFU)0103 physical sciencesthermal thin-film filterElectrical and Electronic EngineeringAerospace engineering010306 general physics010303 astronomy & astrophysicsbusiness.industryElectronic Optical and Magnetic MaterialDetectorAstrophysics::Instrumentation and Methods for AstrophysicsShot noiseComputer Science Applications1707 Computer Vision and Pattern RecognitionTransition Edge SensorApplied MathematicATHENA X-ray observatoryRadio frequencyTransition edge sensorbusinessSpace Telescopes and Instrumentation 2018: Ultraviolet to Gamma Ray
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The LOFT mission concept: a status update

2016

The Large Observatory For x-ray Timing (LOFT) is a mission concept which was proposed to ESA as M3 and M4 candidate in the framework of the Cosmic Vision 2015-2025 program. Thanks to the unprecedented combination of effective area and spectral resolution of its main instrument and the uniquely large field of view of its wide field monitor, LOFT will be able to study the behaviour of matter in extreme conditions such as the strong gravitational field in the innermost regions close to black holes and neutron stars and the supra-nuclear densities in the interiors of neutron stars. The science payload is based on a Large Area Detector (LAD, >8m2 effective area, 2-30 keV, 240 eV spectral resolut…

X-ray timing[ SDU.ASTR.GA ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Field of viewAstrophysics01 natural scienceslaw.inventionlawObservatorytiming010303 astronomy & astrophysicsQBPhysicsmicrochannel plates. PROPORTIONAL COUNTER ARRAYCALIBRATIONX-ray astronomyElectronic Optical and Magnetic MaterialApplied MathematicsAstrophysics::Instrumentation and Methods for AstrophysicsComputer Science Applications1707 Computer Vision and Pattern RecognitionX-ray detectorsCondensed Matter Physicscompact objectsX-ray spectroscopy[SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]spectroscopyCosmic Vision[ INFO ] Computer Science [cs]Silicon detectorAstrophysics::High Energy Astrophysical PhenomenaCondensed Matter PhysicTelescopeX-rayX-ray astronomySilicon detectors; spectroscopy; timing; X-ray astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Applied Mathematics; Electrical and Electronic EngineeringSettore FIS/05 - Astronomia e Astrofisica0103 physical sciencesElectronic[INFO]Computer Science [cs]Optical and Magnetic MaterialsSpectral resolutionElectrical and Electronic EngineeringDETECTORta115X-ray astronomy Silicon detectors timing spectroscopy010308 nuclear & particles physicsX-ray imagingX-ray timing; X-ray spectroscopy; X-ray imaging; compact objects; X-ray detectors; microchannel plates. PROPORTIONAL COUNTER ARRAY; CALIBRATION; DETECTORApplied MathematicNeutron starQB460-466 AstrophysicsSilicon detectors; spectroscopy; timing; X-ray astronomy; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringSilicon detectors; spectroscopy; timing; X-ray astronomySilicon detectorsLarge Observatory For x-ray Timing (LOFT) Large Area Detector (LAD) Wide Field Monitor (WFM) Large Area Silicon Drift Detectors (SDD)Gamma-ray burst
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On finite involutive Yang–Baxter groups

2021

[EN] A group G is said to be an involutive Yang¿Baxter group, or simply an IYB-group, if it is isomorphic to the permutation group of an involutive, nondegenerate set-theoretic solution of the Yang-Baxter equation. We give new sufficient conditions for a group that can be factorised as a product of two IYB-groups to be an IYB-group. Some earlier results are direct consequences of our main theorem.

Yang–Baxter equationApplied MathematicsGeneral MathematicsYang-Baxter equationInvolutive nondegenerate solutionsInvolutive Yang-Baxter groupMATEMATICA APLICADAMatemàticaFinite left braceMathematical physicsMathematicsProceedings of the American Mathematical Society
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Irregular Time Dependent Obstacles

2010

Abstract We study the obstacle problem for the Evolutionary p-Laplace Equation when the obstacle is discontinuous and does not have regularity in the time variable. Two quite different procedures yield the same solution.

Yield (engineering)Parabolic obstacle problemVariational inequalities35K55 31B15 31B05Irregular obstacleLeast solutionComputer Science::RoboticsParabolic balayageLavrentiev phenomenonMathematics - Analysis of PDEsSupersolutionp-ParabolicObstacleVariational inequalityObstacle problemFOS: MathematicsApplied mathematicsTime variablePotentialAnalysisAnalysis of PDEs (math.AP)Mathematics
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Effect of internal noise on the relaxation time of an yttria stabilized zirconia-based memristor

2022

The effects of temperature on the switching kinetics of an yttrium-stabilized zirconia-based memristor from a low-resistance state to a high-resistance state have been experimentally investigated. It was found that the memristor relaxation time depends on the temperature in a non-monotonous way, with a maximum observed at the temperature close to 55 °C. This nonmonotonic behavior is a signature of the noise-enhanced stability phenomenon observed in all physical and complex systems characterized by metastable states.

Yttria stabilized zirconiaMetastabilitySettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciGeneral MathematicsApplied MathematicsBeneficiary role of noiseGeneral Physics and AstronomyResistive switchingStatistical and Nonlinear PhysicsMemristorNoise induced stabilizationChaos, Solitons & Fractals
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