Search results for "Dynamic"

showing 10 items of 12329 documents

Knee joint loading in the open and square stance tennis forehands

2013

Sandamas, Paul 2013. Knee joint loading in the open and square stance tennis forehands. Department of Biology of Physical Activity, University of Jyväskylä. Master's Thesis in Biomechanics. 80 pages. The aim of this study was to calculate and compare the resultant forces and moments in the knee joint of the open and square stance tennis forehands. An additional aim was to incorporate the ground reaction forces to shed light on the role of the lower body in aiding pelvic rotation in these two different forehands. The two types of forehand strokes hit by 7 right-handed university team level tennis players were filmed and the ground reaction forces on each foot were measured simultaneously. A …

free moment.niveletpolvetknee joint loadingtennisinverse dynamicstennis forehand
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Free-volume Study in GeS2-Ga2S3-CsCl Chalcohalide Glasses Using Positron Annihilation Technique

2015

Abstract Positron annihilation lifetime spectroscopy combined with Doppler broadening of annihilation radiation was applied to study free-volume entities in Ge-Ga-S glasses having different amount of CsCl additives. It is shown that the structural changes caused by CsCl additives can be adequately described by positron trapping modes determined within two-state model. The results testify in a favor of rather unchanged nature of corresponding free-volume voids responsible for positron trapping in the studied glasses, when mainly concentration of these traps is a subject to most significant changes with composition.

free-volume entitiesMaterials scienceChalcogenidePhysics and Astronomy(all)Positron trappingMolecular physicschemistry.chemical_compoundchalcogenideVolume (thermodynamics)chemistryAnnihilation radiationchalcohalidepositron trappingSpectroscopyDoppler broadeningPositron annihilationglassPhysics Procedia
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B–T phase diagram of Pd/Fe/Ir(111) computed with parallel tempering Monte Carlo

2017

We use an atomistic spin model derived from density functional theory calculations for the ultra-thin film Pd/Fe/Ir(111) to show that temperature induces coexisting non-zero skyrmion and antiskyrmion densities. We apply the parallel tempering Monte Carlo method in order to reliably compute thermodynamical quantities and the B-T phase diagram in the presence of frustrated exchange interactions. We evaluate the critical temperatures using the topological susceptibility. We show that the critical temperatures depend on the magnetic field in contrast to previous work. In total, we identify five phases: spin spiral, skyrmion lattice, ferromagnetic phase, intermediate region with finite topologic…

frustration of magnetic exchangemagnetic skyrmionsMonte Carlo methodthermodynamic studyFOS: Physical sciencesGeneral Physics and Astronomy02 engineering and technology53001 natural sciences7. Clean energyMonte Carlo simulationsPhase (matter)0103 physical sciencesSpin model010306 general physicsTopological quantum numberPhase diagramPhysicsCondensed Matter - Materials ScienceCondensed matter physicsSkyrmionMaterials Science (cond-mat.mtrl-sci)021001 nanoscience & nanotechnologyCondensed Matter::Strongly Correlated ElectronsDensity functional theoryParallel tempering0210 nano-technologyNew Journal of Physics
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"Semmonen siitä tuli Hitlerinki hommista" : ihmissuhteiden merkitykset skitsofreenistyyppisen psykoosin yhteydessä

2004

functional characteristicscase studytapaustutkimusskitsofreniamielenterveyssosiaaliset verkostotpsykoositpsychodynamic frameworkschizophrenia-like nonaffective psychosissocial networkpsykodynamiikka
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Approche d'un territoire de montagne : occupations humaines et contexte pédo-sédimentaire des versants du col du Petit-Saint-Bernard, de la Préhistoi…

2014

As part of a multi-year programme, survey campaigns have been carried out on both slopes of the Petit-Saint-Bernard pass (2188 m, western Alps), at an altitude of between 750 and 3000 m. The method employed abandons ground-based surveying in favour of multiple manual surveys carried out on selected topographic contexts down to the base of the Holocene fill. The results obtained document the longterm development of the pedo-sedimentary dynamic and the occupation of the different altitude stages. The significance of the archaeological data collected is discussed in relation to the state of knowledge in a comparison area including the neighbouring valleys of the western Alps, to existing settl…

funerary practicesBronze Agepédogenèsepratiques funérairesIron Age[SDE.MCG]Environmental Sciences/Global Changesdynamique du peuplement alpin[SHS.GEO] Humanities and Social Sciences/GeographyNéolithiquesédentarisationâge du FerAlpine settlement dynamicssites perchéshabitatspedo-sedimentary dynamicsNeolithicalpagesdynamique pédo-sédimentaireAlpes occidentales[SDE.IE]Environmental Sciences/Environmental Engineering[SHS.GEO]Humanities and Social Sciences/Geographyhabitationpedogenesis[SDE.ES]Environmental Sciences/Environmental and Societyalpine pasturespastoralismewestern Alpscirculations transalpines[SDE.BE] Environmental Sciences/Biodiversity and Ecologytrans-Alpine circulation[SDE.MCG] Environmental Sciences/Global Changesâge du Bronzesedentism[SDE.ES] Environmental Sciences/Environmental and Society[SDE.IE] Environmental Sciences/Environmental Engineering[SDE.BE]Environmental Sciences/Biodiversity and Ecologypastoralism
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Two‐dimensional metric spheres from gluing hemispheres

2022

We study metric spheres (Z,dZ) obtained by gluing two hemispheres of S2 along an orientation-preserving homeomorphism g:S1→S1, where dZ is the canonical distance that is locally isometric to S2 off the seam. We show that if (Z,dZ) is quasiconformally equivalent to S2, in the geometric sense, then g is a welding homeomorphism with conformally removable welding curves. We also show that g is bi-Lipschitz if and only if (Z,dZ) has a 1-quasiconformal parametrization whose Jacobian is comparable to the Jacobian of a quasiconformal mapping h:S2→S2. Furthermore, we show that if g−1 is absolutely continuous and g admits a homeomorphic extension with exponentially integrable distortion, then (Z,dZ) …

funktioteoriaMathematics::Dynamical SystemsMathematics::Complex VariablesGeneral MathematicsgeometriamittateoriaMathematics::Geometric Topologymetriset avaruudetJournal of the London Mathematical Society
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Sobolev homeomorphic extensions onto John domains

2020

Given the planar unit disk as the source and a Jordan domain as the target, we study the problem of extending a given boundary homeomorphism as a Sobolev homeomorphism. For general targets, this Sobolev variant of the classical Jordan-Schoenflies theorem may admit no solution - it is possible to have a boundary homeomorphism which admits a continuous $W^{1,2}$-extension but not even a homeomorphic $W^{1,1}$-extension. We prove that if the target is assumed to be a John disk, then any boundary homeomorphism from the unit circle admits a Sobolev homeomorphic extension for all exponents $p<2$. John disks, being one sided quasidisks, are of fundamental importance in Geometric Function Theory.

funktioteoriaMathematics::Dynamical SystemsSobolev extensionsMathematics - Complex Variables46E35 58E20quasidisksFOS: MathematicsMathematics::General TopologySobolev homeomorphismsComplex Variables (math.CV)John domainsfunktionaalianalyysiMathematics::Geometric Topology
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High-energy monitoring of NGC 4593 II. Broad-band spectral analysis: testing the two-corona model

2019

It is widely believed that the primary X-ray emission of AGN is due to the Comptonisation of optical-UV photons from a hot electron corona, while the origin of the 'soft-excess' is still uncertain and matter of debate. A second Comptonisation component, called warm corona, was therefore proposed to account for the soft-excess, and found in agreement with the optical-UV to X-ray emission of a sample of Seyfert galaxies. In this context, we exploit the broadband XMM-Newton and NuSTAR simultaneous observations of the Seyfert galaxy NGC 4593 to further test the so called "two corona model". The NGC 4593 spectra are well reproduced by the model, from the optical/UV to the hard X-rays. Moreover, …

galaxie [X-rays]High energyPhotonAstrophysics::High Energy Astrophysical Phenomenablack hole physicsgalaxies: activeFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesmagnetohydrodynamics (MHD)Spectral lineCorona (optical phenomenon)X-rays: binariesaccretionPrimary (astronomy)Seyfert [galaxies]0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsSpectral analysis010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)individuals: (NGC 4593) [X-rays][SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsaccretion disks[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsAstronomy and AstrophysicGalaxygalaxies: SeyfertX-rays: galaxiesISM: jets and outflowsSpace and Planetary Science[SDU]Sciences of the Universe [physics]active [galaxies]Astrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]X-rays: individuals: (NGC 4593)
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Cosmological hydrodynamical simulations of galaxy clusters: X-ray scaling relations and their evolution

2018

We analyse cosmological hydrodynamical simulations of galaxy clusters to study the X-ray scaling relations between total masses and observable quantities such as X-ray luminosity, gas mass, X-ray temperature, and $Y_{X}$. Three sets of simulations are performed with an improved version of the smoothed particle hydrodynamics GADGET-3 code. These consider the following: non-radiative gas, star formation and stellar feedback, and the addition of feedback by active galactic nuclei (AGN). We select clusters with $M_{500} > 10^{14} M_{\odot} E(z)^{-1}$, mimicking the typical selection of Sunyaev-Zeldovich samples. This permits to have a mass range large enough to enable robust fitting of the r…

galaxies: clusters: intracluster mediumCosmology and Nongalactic Astrophysics (astro-ph.CO)Active galactic nucleusNUMERICAL [METHODS]Ciencias FísicasFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsnumerical galaxies: clusters: general galaxies: clusters: intracluster medium X-rays: galaxies: clusters [methods]01 natural sciencesmethods: numericalLuminosity//purl.org/becyt/ford/1 [https]GALAXIES: CLUSTERS [X-RAYS]Smoothed-particle hydrodynamics0103 physical sciences010303 astronomy & astrophysicsScalingAstrophysics::Galaxy AstrophysicsGalaxy clusterPhysicsmethods: numerical galaxies: clusters: general galaxies: clusters: intracluster medium X-rays: galaxies: clustersSettore FIS/05010308 nuclear & particles physicsStar formationAstronomy and AstrophysicsObservable//purl.org/becyt/ford/1.3 [https]RedshiftAstronomíamethods: numerical; galaxies: clusters: general; galaxies: clusters: intracluster medium; X-rays: galaxies: clusters; Astrophysics - Cosmology and Nongalactic Astrophysicsgalaxies: clusters: generalSpace and Planetary ScienceX-rays: galaxies: clustersCLUSTERS: INTRACLUSTER MEDIUM [GALAXIES]CLUSTERS: GENERAL [GALAXIES]CIENCIAS NATURALES Y EXACTASAstrophysics - Cosmology and Nongalactic AstrophysicsMonthly Notices of the Royal Astronomical Society
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Unveiling the environment and faint features of the isolated galaxy CIG 96 with deep optical and HI observations

2018

Context. Asymmetries in atomic hydrogen (HI) in galaxies are often caused by the interaction with close companions, making isolated galaxies an ideal framework to study secular evolution. The AMIGA project has demonstrated that isolated galaxies show the lowest level of asymmetry in their HI integrated profiles compared to even field galaxies, yet some present significant asymmetries. CIG 96 (NGC 864) is a representative case reaching a 16% level. Aims. Our aim is to investigate the HI asymmetries of the spiral galaxy CIG 96 and what processes have triggered the star-forming regions observed in the XUV pseudo-ring. Methods. We performed deep optical observations at CAHA1.23m, CAHA2.2m and V…

galaxies: spiralHIERARCHICAL SATELLITE ACCRETIONmedia_common.quotation_subjectFOS: Physical sciencesAstrophysicsI.01 natural sciences7. Clean energyAsymmetryAMIGA SAMPLElaw.inventionTelescopelaw0103 physical scienceskinematics and dynamics [galaxies]DARK-MATTER SUBSTRUCTURESurface brightness010303 astronomy & astrophysicsStellar evolutionComputingMilieux_MISCELLANEOUSevolution [galaxies]galaxies: kinematics and dynamicsLOPSIDED SPIRAL GALAXIESmedia_commonindividual: NGC 864 [galaxies]Physicsradio lines: galaxiesSpiral galaxy010308 nuclear & particles physicsgalaxies: individual: NGC864Astronomy and AstrophysicsDISK GALAXIESAstrophysics - Astrophysics of GalaxiesAccretion (astrophysics)Galaxygalaxies [radio lines]RINGSTIDAL STREAMspiral [galaxies][SDU]Sciences of the Universe [physics]Space and Planetary ScienceGASAstrophysics of Galaxies (astro-ph.GA)structure [galaxies]galaxies: structureDIGITAL SKY SURVEYCirrusGalaxies: Individual: NGC 864galaxies: evolutionAstronomy & astrophysics
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