Search results for "Anisotropy"

showing 10 items of 912 documents

Inhomogeneous-strain-induced magnetic vortex cluster in one-dimensional manganite wire

2020

Abstract Mixed-valance manganites with strong electron correlation exhibit strong potential for spintronics, where emergent magnetic behaviors, such as propagation of high-frequency spin waves and giant topological Hall Effects can be driven by their mesoscale spin textures. Here, we create magnetic vortex clusters with flux closure spin configurations in single-crystal La0.67Sr0.33MnO3 wire. A distinctive transformation from out-of-plane domains to a vortex state is directly visualized using magnetic force microscopy at 4 K in wires when the width is below 1.0 μm. The phase-field modeling indicates that the inhomogeneous strain, accompanying with shape anisotropy, plays a key role for stab…

PhysicsMultidisciplinaryCondensed matter physicsSpintronicsSpin structure010502 geochemistry & geophysicsManganite01 natural sciencesVortex stateSpin waveCondensed Matter::Strongly Correlated ElectronsMagnetic force microscopeAnisotropy0105 earth and related environmental sciencesSpin-½Science Bulletin
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Random quasi-phase-matched second-harmonic generation in periodically poled lithium tantalate

2010

We observe second harmonic generation via random quasi-phase-matching in a 2.0 micron periodically poled, 1-cm-long, z-cut lithium tantalate. Away from resonance, the harmonic output profiles exhibit a characteristic pattern stemming from a stochastic domain distribution and a quadratic growth with the fundamental excitation, as well as a broadband spectral response. The results are in good agreement with a simple model and numerical simulations in the undepleted regime, assuming an anisotropic spread of the random nonlinear component. (C) 2010 Optical Society of America

PhysicsNonlinear opticNonlinear optics; Harmonic generation and mixingPhase (waves)FOS: Physical sciencesResonanceSecond-harmonic generationPhysics::OpticsHarmonic generation and mixing01 natural sciencesAtomic and Molecular Physics and Optics010309 opticsNonlinear systemchemistry.chemical_compoundchemistry0103 physical sciencesLithium tantalateHarmonicAtomic physics010306 general physicsAnisotropyExcitationOptics (physics.optics)Physics - Optics
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Anisotropic Heisenberg chain with composite spin

1986

A family of one-dimensional magnetic Hamiltonians is introduced, where at each site there are $n$ spin-$S$ operators. It is shown that, for special couplings between spins and for $S=\frac{1}{2}$, the model contains the complete spectrum of the Heisenberg chain with spins \textonehalf{}, 1, frac32;, etc., and the ground state is that of the corresponding Heisenberg chain. By the varying of a single parameter the model allows continuous transitions between chains with different spin. We map the spin-($S+S$) model onto the nonlinear $\ensuremath{\sigma}$ model and discuss the possibility of a finite gap in the spin-(\textonehalf{}+\textonehalf{}) model.

PhysicsNonlinear systemChain (algebraic topology)SpinsQuantum mechanicsSpectrum (functional analysis)SigmaCondensed Matter::Strongly Correlated ElectronsSpin (physics)Ground stateAnisotropyPhysical Review B
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Nonlinear inverse bremsstrahlung and highly anisotropic electron distributions

1996

A procedure is proposed to deal with the approximate solution of the kinetic equation for the velocity distribution function of electrons in a fully ionized plasma in the presence of strong, high frequency radiation. The Legendre polynomial expansion is applied after the kinetic equation has been written in an oscillating frame, where some directions are appropriately scaled, with the aim of making approximately isotropic, on the average, distributions that are otherwise anisotropic. The equations are derived for the isotropic part of the electron distribution in the scaled frame and for the scaling factor. The procedure is meant to display its potential in cases where the electron distribu…

PhysicsNonlinear systemClassical mechanicsDistribution functionField (physics)IsotropyBremsstrahlungElectronAnisotropyLegendre polynomialsComputational physicsPhysical Review E
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Influence of domain wall anisotropy on the current-induced hysteresis loop shift for quantification of the Dzyaloshinskii-Moriya interaction

2021

Using several material systems with various magnitudes of the interfacial Dzyaloshinskii-Moriya interaction (DMI), we elucidate a critical influence of domain wall (DW) anisotropy on the current-induced hysteresis loop shift scheme widely employed to determine the magnitude of the Dzyaloshinskii-Moriya effective field (${H}_{\mathrm{DMI}}$). Taking into account the DW anisotropy in the analysis of the hysteresis loop shift, which has not been included in the original model [Phys. Rev. B 93, 144409 (2016)], we show that it provides quantitative agreement of ${H}_{\mathrm{DMI}}$ with that determined from an asymmetric bubble expansion technique for small DMI material systems. For large DMI sy…

PhysicsNonlinear systemDomain wall (magnetism)Current (mathematics)SpintronicsField (physics)Condensed matter physicsMaterial systemAnisotropyMagnetic fieldPhysical Review B
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Solitary excitations in one-dimensional magnets

1991

Abstract The present status of theoretical and experimental investigations of solitary excitations in one-dimensional magnetic systems is reviewed. A survey of exact solutions to the nonlinear equations of motion for pertinent classical chain systems (sine-Gordon chain and ferromagnetic Heisenberg chains with various anisotropies) is given. Particular emphasis is devoted to the role of solitons in the thermodynamics of such systems. Models corresponding to real quasi-one-dimensional magnets are broadly discussed to demonstrate the properties of their solitary excitations. The experimental significance of such nonlinear excitations in the static and dynamic quantities of such systems is disc…

PhysicsNonlinear systemTransverse planeFerromagnetismChain (algebraic topology)Quantum mechanicsMagnetAntiferromagnetismCondensed Matter PhysicsAnisotropyQuantumAdvances in Physics
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Linear and non-linear flow mode in Pb–Pb collisions at sNN=2.76 TeV

2017

The second and the third order anisotropic flow, V2 and V3, are mostly determined by the corresponding initial spatial anisotropy coefficients, e2 and e3, in the initial density distribution. In addition to their dependence on the same order initial anisotropy coefficient, higher order anisotropic flow, Vn (n > 3), can also have a significant contribution from lower order initial anisotropy coefficients, which leads to mode-coupling effects. In this Letter we investigate the linear and non-linear modes in higher order anisotropic flow Vn for n = 4, 5, 6 with the ALICE detector at the Large Hadron Collider. The measurements are done for particles in the pseudorapidity range |η| < 0.8 and the…

PhysicsNuclear and High Energy Physics010308 nuclear & particles physicsHadron01 natural sciencesNuclear physicsThird orderViscosityFlow (mathematics)Pseudorapidity0103 physical sciencesRapidityBoundary value problem010306 general physicsAnisotropyPhysics Letters B
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CMB anisotropies: cosmic confusion and polarization

2001

Abstract Some physical effects producing Cosmic Microwave Background (CMB) anisotropies are briefly described. The CMB angular power spectrum is calculated -in appropriate cases- with the essential aim of estimating and comparing the effects produced by reionization and gravitational waves; thus a problem of Cosmic Confusion is pointed out. Accurate measurements of the CMB polarization could solve this problem in future. Some comments about the PLANCK mission —ESA project for anisotropy detection— are given.

PhysicsNuclear and High Energy PhysicsCOSMIC cancer databaseGravitational waveCosmic microwave backgroundAstrophysics::Instrumentation and Methods for AstrophysicsAstronomySpectral densityAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsPolarization (waves)Atomic and Molecular Physics and Opticssymbols.namesakesymbolsPlanckAnisotropyReionizationNuclear Physics B - Proceedings Supplements
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Relativistic second-order perturbations of the Einstein-de Sitter universe

1998

We consider the evolution of relativistic perturbations in the Einstein-de Sitter cosmological model, including second-order effects. The perturbations are considered in two different settings: the widely used synchronous gauge and the Poisson (generalized longitudinal) one. Since, in general, perturbations are gauge dependent, we start by considering gauge transformations at second order. Next, we give the evolution of perturbations in the synchronous gauge, taking into account both scalar and tensor modes in the initial conditions. Using the second-order gauge transformation previously defined, we are then able to transform these perturbations to the Poisson gauge. The most important feat…

PhysicsNuclear and High Energy PhysicsEinstein–de Sitter universeGravitational waveAstrophysics (astro-ph)Cosmic microwave backgroundFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological modelPoisson distributionAstrophysicsGeneral Relativity and Quantum CosmologyFormalism (philosophy of mathematics)symbols.namesakeClassical mechanicssymbolsGauge theoryAnisotropyMathematical physics
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Corrigendum to “Systematics of azimuthal anisotropy harmonics in proton–nucleus collisions at the LHC from the Color Glass Condensate” [Phys. Lett. B…

2019

PhysicsNuclear and High Energy PhysicsLarge Hadron ColliderProton010308 nuclear & particles physics01 natural sciencesColor-glass condensateAzimuthNuclear physicsmedicine.anatomical_structureHarmonics0103 physical sciencesmedicine010306 general physicsAnisotropyNucleusPhysics Letters
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