Search results for "Anisotropy"

showing 10 items of 912 documents

Gradient estimates for the perfect conductivity problem in anisotropic media

2018

Abstract We study the perfect conductivity problem when two perfectly conducting inclusions are closely located to each other in an anisotropic background medium. We establish optimal upper and lower gradient bounds for the solution in any dimension which characterize the singular behavior of the electric field as the distance between the inclusions goes to zero.

Finsler LaplacianApplied MathematicsGeneral Mathematics010102 general mathematicsMathematical analysisZero (complex analysis)Perfect conductorGradient blow-upConductivity01 natural sciences010101 applied mathematicsMathematics - Analysis of PDEsDimension (vector space)Settore MAT/05 - Analisi MatematicaElectric fieldSingular behaviorFOS: MathematicsMathematics (all)Primary: 35J25 35B44 35B50 Secondary: 35J62 78A48 58J600101 mathematicsPerfect conductorAnisotropyAnalysis of PDEs (math.AP)MathematicsJournal de Mathématiques Pures et Appliquées
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Dielectric Relaxation of a Polybutadiene Melt at a Crystalline Graphite Surface: Atomistic Molecular Dynamics Simulations

2014

Dielectric experiments are an indispensable tool to further our understanding of the relaxation behavior of polymers, not only in bulk samples but also in confined situations. A chemically realistic Molecular Dynamics simulation, in which all information about molecular motions is available, can shed light onto the questions of heterogeneity and anisotropy of the underlying molecular relaxation processes which lead to the ensemble averaged experimental dielectric signal. In this contribution, we present a careful analysis of the dielectric response of a weakly polar and confined polymer, 1,4-polybutadiene between graphite walls. The relaxation of the segmental dipole moments was obtained in…

Fluctuation-dissipation theoremMolecular dynamicsDipolesymbols.namesakeMaterials scienceComputational chemistryChemical physicsRelaxation (NMR)symbolsDielectricAnisotropyCole–Cole equationDebye
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Modeling of anisotropic grain growth in minerals

2001

The role of surface energy anisotropy during grain growth is investigated using both physical experiments on octachloropropane and numerical experiments using the Elle microstructural modelling system. In particular the effects of anisotropy on growth rates, grain shapes and lattice preferred orientations are analysed. Anisotropic growth in thin polycrystalline sheets of octachloropropane is found to systematically remove certain c-axis orientations from the sample, without obviously modifying the grain shapes. By comparison with equivalent numerical experiments, we can explain these observations with a simple boundary layer model that treats each side of each grain boundary as an independe…

Grain growthBoundary layerCondensed matter physicsFinite strain theoryGrain boundaryCrystalliteGrowth rateAnisotropyGeologySurface energy
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GFP-mut2 Proteins in Trehalose-Water Matrixes: Spatially Heterogeneous Protein-Water-Sugar Structures

2007

We report investigations on the properties of nanoenvironments around single-GFP-mut2 proteins in trehalose-water matrixes. Single-GFPmut2 molecules embedded in thin trehalose-water films were characterized in terms of their fluorescence brightness, bleaching dynamics, excited state lifetime, and fluorescence polarization. For each property, sets of approximately 100-150 single molecules have been investigated as a function of trehalose content and hydration. Three distinct and interconverting families of proteins have been found which differ widely in terms of bleaching dynamics, brightness, and fluorescence polarization, whose relative populations sizably depend on sample hydration. The r…

Green Fluorescent ProteinsBiophysicsAnalytical chemistryCarbohydratesMolecular ConformationPhase TransitionColloidchemistry.chemical_compoundMoleculeColloidsSupercoolingthrealosesingle molecule fluorescenceChemistryTrehaloseWaterSingle-molecule experimentFluorescenceTrehaloseSolutionsModels ChemicalChemical physicsCell BiophysicsGFPmut2Excited statelifetimesFluorescence anisotropy
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Searches for transverse momentum dependent flow vector fluctuations in Pb-Pb and p-Pb collisions at the LHC

2017

The measurement of azimuthal correlations of charged particles is presented for Pb-Pb collisions at $\sqrt{s_{\rm NN}}=$ 2.76 TeV and p-Pb collisions at $\sqrt{s_{\rm NN}}=$ 5.02 TeV with the ALICE detector at the CERN Large Hadron Collider. These correlations are measured for the second, third and fourth order flow vector in the pseudorapidity region $|��|<0.8$ as a function of centrality and transverse momentum $p_{\rm T}$ using two observables, to search for evidence of $p_{\rm T}$-dependent flow vector fluctuations. For Pb-Pb collisions at 2.76 TeV, the measurements indicate that $p_{\rm T}$-dependent fluctuations are only present for the second order flow vector. Similar results hav…

HEAVY-ION COLLISIONSnucl-extransverse momentum dependenceCOLLABORATIONangular correlation [charged particle]High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ALICEmodel: hydrodynamicstransport theory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear Experiment (nucl-ex)[ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear ExperimentNuclear ExperimentMonte CarloHeavy Ion Experiments; RELATIVISTIC NUCLEAR COLLISIONS; HEAVY-ION COLLISIONS; QUARK-GLUON; PLASMA; COLLECTIVE FLOW; COLLABORATIONPLASMAfluctuation [geometry]flow: anisotropygeometry: fluctuationQUARK-GLUONCERN LHC CollHeavy Ion Experiments; Nuclear and High Energy PhysicsflowRELATIVISTIC NUCLEAR COLLISIONSHeavy Ion ExperimentQuark-Gluon PlasmaParticle Physics - Experiment2760 GeV/nucleon5020 GeV/nucleonNuclear and High Energy PhysicsCERN LabCOLLECTIVE FLOWFOS: Physical sciencestransverse momentum[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]vector [fluctuation]Heavy Ion Experimentsscattering [heavy ion][ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]factorizationlcsh:Nuclear and particle physics. Atomic energy. Radioactivityddc:530hydrodynamics [model]Nuclear Physics - Experimentnumerical calculationsinitial stateleadHeavy Ion Experiments Nuclear and High Energy Physics.hep-exboundary conditionrapiditycorrelationviscositylcsh:QC770-798High Energy Physics::Experimentp nucleusentropy: densitycharged particle: angular correlationexperimental results
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A search for anisotropy in the arrival directions of ultra high energy cosmic rays recorded at the Pierre Auger Observatory

2012

Observations of cosmic ray arrival directions made with the Pierre Auger Observatory have previously provided evidence of anisotropy at the 99% CL using the correlation of ultra high energy cosmic rays (UHECRs) with objects drawn from the Véron-Cetty Véron catalog. In this paper we report on the use of three catalog independent methods to search for anisotropy. The 2pt–L, 2pt+ and 3pt methods, each giving a different measure of selfclustering in arrival directions, were tested on mock cosmic ray data sets to study the impacts of sample size and magnetic smearing on their results, accounting for both angular and energy resolutions. If the sources of UHECRs follow the same large scale structu…

HIRES STEREO[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomySMALL-SCALE ANISOTROPYAstrophysics01 natural sciencesAltas energíasCosmic Rays ShowerCosmologyUltra-high-energy cosmic rayAnisotropy010303 astronomy & astrophysicsmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[PHYS]Physics [physics]BL-LACERTAEAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryRadiación cósmicaFísica nuclearOBJECTSAstrophysics - High Energy Astrophysical Phenomenacosmic ray experiments; ultra high energy cosmic raysACTIVE GALACTIC NUCLEIActive galactic nucleusmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic raysearch for anisotropyultra high energy cosmic raysCosmic Ray[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciences010306 general physicsCiencias ExactasPierre Auger ObservatorySPECTRUMAstronomyFísicaAstronomy and AstrophysicsASTROFÍSICAUniverseGalaxyExperimental High Energy Physicsanisotrpycosmic ray experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyJournal of Cosmology and Astroparticle Physics
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Electronic characterisation of the oxidized state of the blue copper protein Rusticyanin by 1 H NMR: Is the axial methionine the dominant influence f…

2001

The oxidized state of rusticyanin, the blue copper protein with the highest redox potential in its class, has been investigated through (1)H nuclear magnetic resonance applied to its cobalt(II) derivative. The assignment of the protons belonging to the coordinated residues has been performed. Many other amino acids situated in the vicinity of the metal ion, including six hydrophobic residues (isoleucine140 and five phenylalanines) have also been identified. The orientation of the main axes of the magnetic susceptibility tensor for the cobalt(II)-rusticyanin as well as its axial, Deltachi(ax), and rhombic, Deltachi(rh), magnetic susceptibility anisotropy components have been determined. A co…

Half-reactionChemistryCopper proteinInorganic chemistrychemistry.chemical_elementCobaltLigandsBiochemistryMagnetic susceptibilityRedoxElectron TransportCrystallographyMethionineBacterial ProteinsAzurinMetalloproteinsRusticyaninProton NMRAnisotropyProtonsAzurinNuclear Magnetic Resonance BiomolecularOxidation-ReductionCobaltCopper
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Spatial distribution of X-ray emitting ejecta in Tychos SNR: indications of shocked Titanium

2015

Young supernova remnants show a characteristic ejecta-dominated X-ray emission that allows us to probe the products of the explosive nucleosynthesis processes and to ascertain important information about the physics of the supernova explosions. Hard X-ray observations have recently revealed the radioactive decay lines of 44Ti at ~67.9 keV and ~78.4 keV in the Tycho's SNR. We here analyze the set of XMM-Newton archive observations of the Tycho's SNR. We produce equivalent width maps of the Fe K and Ca XIX emission lines and find indications for a stratification of the abundances of these elements and significant anisotropies. We then perform a spatially resolved spectral analysis by identify…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSpectral lineISM: individual objects: Tycho's SNR ISM: supernova remnants X-rays: ISMSupernovaSpace and Planetary ScienceNucleosynthesisAstrophysics::Solar and Stellar AstrophysicsEmission spectrumAstrophysics - High Energy Astrophysical PhenomenaEjectaAnisotropyEquivalent widthRadioactive decayAstrophysics::Galaxy Astrophysics
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Simulations of an inhomogeneous stellar wind interacting with a pulsar wind in a binary system

2014

Binary systems containing a massive star and a non-accreting pulsar present strong interaction between the stellar and the pulsar winds. The properties of this interaction, which largely determine the non-thermal radiation in these systems, strongly depend on the structure of the stellar wind, which can be clumpy or strongly anisotropic, as in Be stars. We study numerically the influence of inhomogeneities in the stellar wind on the structure of the two-wind interaction region. We carried out for the first time axisymmetric, relativistic hydrodynamical simulations, with Lorentz factors of ~6 and accounting for the impact of instabilities, to study the impact in the two-wind interaction stru…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstrophysics::High Energy Astrophysical PhenomenaLorentz transformationStrong interactionRotational symmetryFOS: Physical sciencesBinary numberAstronomy and AstrophysicsContext (language use)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicssymbols.namesakePulsar13. Climate actionSpace and Planetary SciencePhysics::Space PhysicssymbolsAstrophysics::Solar and Stellar AstrophysicsDensity contrastAstrophysics - High Energy Astrophysical PhenomenaAnisotropyPhysics::Atmospheric and Oceanic PhysicsAstrophysics::Galaxy AstrophysicsAstronomy & Astrophysics
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Hydrodynamic simulations unravel the progenitor-supernova-remnant connection in SN 1987A

2019

(Abridged) We aim at linking the dynamical and radiative properties of the remnant of SN 1987A to the geometrical and physical characteristics of the parent aspherical SN explosion and to the internal structure of its progenitor star. We performed 3D hydrodynamic simulations which describe the long-term evolution of SN 1987A from the onset of the SN to the full-fledged remnant at the age of 50 years, accounting for the pre-SN structure of the progenitor star. The simulations include all physical processes relevant for the complex phases of SN evolution and for the interaction of the SNR with the highly inhomogeneous ambient environment around SN 1987A. From the simulations, we synthesize ob…

High Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysics010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRedshiftStarsSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary Science0103 physical sciencesRadiative transferAstrophysics::Solar and Stellar AstrophysicsEmission spectrumSupergiantAstrophysics - High Energy Astrophysical PhenomenaAnisotropyEjectaSupernova remnant010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics
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