Search results for "Tensor"

showing 10 items of 550 documents

Computing bulk and shear viscosities from simulations of fluids with dissipative and stochastic interactions

2016

Exact values for bulk and shear viscosity are important to characterize a fluid and they are a necessary input for a continuum description. Here we present two novel methods to compute bulk viscosities by non-equilibrium molecular dynamics (NEMD) simulations of steady-state systems with periodic boundary conditions -- one based on frequent particle displacements and one based on the application of external bulk forces with an inhomogeneous force profile. In equilibrium simulations, viscosities can be determined from the stress tensor fluctuations via Green-Kubo relations; however, the correct incorporation of random and dissipative forces is not obvious. We discuss different expressions pro…

PhysicsCauchy stress tensorForce profileShear viscosityDissipative particle dynamicsGeneral Physics and AstronomyFOS: Physical sciences02 engineering and technologyMechanicsCondensed Matter - Soft Condensed Matter021001 nanoscience & nanotechnology01 natural sciencesMolecular dynamicsShear (geology)0103 physical sciencesDissipative systemPeriodic boundary conditionsSoft Condensed Matter (cond-mat.soft)Physical and Theoretical Chemistry010306 general physics0210 nano-technology
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Balance equation of generalised sub-grid scale (SGS) turbulent kinetic energy in a new tensorial dynamic mixed SGS model

2000

A new dynamic model is proposed in which the eddy viscosity is defined as a symmetric second rank tensor, proportional to the product of a turbulent length scale with an ellipsoid of turbulent velocity scales. The employed definition of the eddy viscosity allows to remove the local balance assumption of the SGS turbulent kinetic energy formulated in all the dynamic Smagorinsky-type SGS models. Furthermore, because of the tensorial structure of the eddy viscosity the alignment assumption between the principal axes of the SGS turbulent stress tensor and the resolved strain-rate tensor is equally removed, an assumption which is employed in the scalar eddy viscosity SGS models. The proposed mod…

PhysicsCauchy stress tensorTurbulenceScalar (physics)Turbulence modelingGeneral Physics and AstronomyMaxwell stress tensorMechanicsPhysics::Fluid DynamicsMechanics of MaterialsTurbulence kinetic energyGeneral Materials ScienceStatistical physicsTensorLarge eddy simulation
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Potential perturbation to Friedmann universes

1994

The energy-momentum tensor of perturbed Friedmann universes in the longitudinal gauge (depending on only one gravitational potential) is obtained in order to clarify the physical meaning of two important cases: (1) conformally static perturbations (when the potential is independent of time), and (2) nonstatic perturbations in the case where the potential allows a particular separation of time and space coordinates. The statement according to which the longitudinal gauge allows a description of high-density-contrast regions is analyzed. In the conformally static case we suggest interpreting the energy-momentum tensor as representing a set of particles in gravitational interaction, suitable f…

PhysicsClassical mechanicsCosmologiaStress–energy tensorPerturbation (astronomy)Relativitat (Física)Mathematical physics
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Spin accumulation from nonequilibrium first principles methods

2021

For the technologically relevant spin Hall effect, most theoretical approaches rely on the evaluation of the spin-conductivity tensor. In contrast, for most experimental configurations the generation of spin accumulation at interfaces and surfaces is the relevant quantity. Here, we directly calculate the accumulation of spins due to the spin Hall effect at the surface of a thin metallic layer, making quantitative predictions for different materials. Two distinct limits are considered, both relying on a fully relativistic Korringa-Kohn-Rostoker density functional theory method. In the semiclassical approach, we use the Boltzmann transport formalism and compare it directly with a fully quantu…

PhysicsCondensed Matter - Materials ScienceCondensed matter physicsSpinsMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciencesNon-equilibrium thermodynamicsSemiclassical physicscond-mat.mtrl-sciKeldysh formalismCondensed Matter - Other Condensed Mattercond-mat.otherSpin Hall effectDensity functional theoryTensorOther Condensed Matter (cond-mat.other)Spin-½Physical Review B
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New Boundary-Driven Twist States in Systems with Broken Spatial Inversion Symmetry

2017

A full description of a magnetic sample includes a correct treatment of the boundary conditions (BCs). This is in particular important in thin film systems, where even bulk properties might be modified by the properties of the boundary of the sample. We study generic ferromagnets with broken spatial inversion symmetry and derive the general micromagnetic BCs of a system with Dzyaloshinskii-Moriya interaction (DMI). We demonstrate that the BCs require the full tensorial structure of the third-rank DMI tensor and not just the antisymmetric part, which is usually taken into account. Specifically, we study systems with $C_{\infty v}$ symmetry and explore the consequences of the DMI. Interesting…

PhysicsCondensed Matter - Mesoscale and Nanoscale PhysicsMagnetoresistanceField (physics)Condensed matter physicsAntisymmetric relationFOS: Physical sciencesGeneral Physics and AstronomyBoundary (topology)02 engineering and technologyPhysik (inkl. Astronomie)021001 nanoscience & nanotechnology01 natural sciencesSymmetry (physics)Mesoscale and Nanoscale Physics (cond-mat.mes-hall)0103 physical sciencesTensorBoundary value problemTwist010306 general physics0210 nano-technologyPhysical Review Letters
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Interaction of two-level systems in amorphous materials with arbitrary phonon fields

2006

To describe the interaction of the two level systems (TLSs) of an amorphous solid with arbitrary strain fields, we introduce a generalization of the standard interaction Hamiltonian. In this new model, the interaction strength depends on the orientation of the TLS with respect to the strain field through a $6\times 6$ symmetric tensor of deformation potential parameters, $[R]$. Taking into account the isotropy of the amorphous solid, we deduce that $[R]$ has only two independent parameters. We show how these two parameters can be calculated from experimental data and we prove that for any amorphous bulk material the average coupling of TLSs with longitudinal phonons is always stronger than …

PhysicsCondensed matter physicsPhononIsotropyFOS: Physical sciencesInteraction strengthDisordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksCondensed Matter PhysicsQuasi particlesElectronic Optical and Magnetic MaterialsAmorphous solidCondensed Matter::Materials Sciencesymbols.namesakeQuantum mechanicssymbolsSymmetric tensorHamiltonian (quantum mechanics)Physical Review B
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form factor at order of chiral perturbation theory

2001

Abstract This paper describes the calculation of the electromagnetic form factor of the K 0 meson at order p 6 of chiral perturbation theory which is the next-to-leading order correction to the well-known p 4 result achieved by Gasser and Leutwyler. On the one hand, at order p 6 the chiral expansion contains 1- and 2-loop diagrams which are discussed in detail. Especially, a numerical procedure for calculating the irreducible 2-loop graphs of the sunset topology is presented. On the other hand, the chiral Lagrangian L (6) produces a direct coupling of the K 0 current with the electromagnetic field tensor. Due to this coupling one of the unknown parameters of L (6) occurs in the contribution…

PhysicsCouplingNuclear and High Energy PhysicsChiral perturbation theoryMesonCharge radiusHigh Energy Physics::LatticeForm factor (quantum field theory)Order (group theory)Direct couplingMathematical physicsElectromagnetic tensorNuclear Physics B
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Stationary models of magnetized viscous tori around a Schwarzschild black hole

2020

We present stationary solutions of magnetized, viscous thick accretion disks around a Schwarzschild black hole. We assume that the tori are not self-gravitating, are endowed with a toroidal magnetic field, and obey a constant angular momentum law. Our study focuses on the role of the black hole curvature in the shear viscosity tensor and in their potential combined effect on the stationary solutions. Those are built in the framework of a causality-preserving, second-order gradient expansion scheme of relativistic hydrodynamics in the Eckart frame description which gives rise to hyperbolic equations of motion. The stationary models are constructed by numerically solving the general relativis…

PhysicsCusp (singularity)Angular momentum010308 nuclear & particles physicsHorizonFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Curvature01 natural sciencesInstabilityGeneral Relativity and Quantum Cosmology83C57 83C55Classical mechanicsInviscid flow0103 physical sciencesSchwarzschild metricTensor010306 general physics
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The Negele-Vautherin density matrix expansion applied to the Gogny force

2010

We use the Negele-Vautherin density matrix expansion to derive a quasi-local density functional for the description of systems of fermions interacting with short-ranged interactions composed of arbitrary finite-range central, spin-orbit, and tensor components. Terms that are absent in the original Negele-Vautherin approach owing to the angle averaging of the density matrix are fixed by employing a gauge invariance condition. We obtain the Kohn-Sham interaction energies in all spin-isospin channels, including the exchange terms, expressed as functions of the local densities and their derivatives up to second (next to leading) order. We illustrate the method by determining the coupling consta…

PhysicsDensity matrixCoupling constantNuclear and High Energy PhysicsNuclear Theory010308 nuclear & particles physicsBinding energyFOS: Physical sciencesFermion16. Peace & justice01 natural sciencesNuclear Theory (nucl-th)Classical mechanics21.10.DrCentral force21.60.Jz0103 physical sciences21.30.-xGauge theoryTensor010306 general physics
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Nuclear energy density optimization: Shell structure

2013

Nuclear density functional theory is the only microscopical theory that can be applied throughout the entire nuclear landscape. Its key ingredient is the energy density functional. In this work, we propose a new parameterization UNEDF2 of the Skyrme energy density functional. The functional optimization is carried out using the POUNDerS optimization algorithm within the framework of the Skyrme Hartree-Fock-Bogoliubov theory. Compared to the previous parameterization UNEDF1, restrictions on the tensor term of the energy density have been lifted, yielding a very general form of the energy density functional up to second order in derivatives of the one-body density matrix. In order to impose c…

PhysicsDensity matrixNuclear and High Energy PhysicsWork (thermodynamics)ta114Nuclear Theory[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]010308 nuclear & particles physicsOrbital-free density functional theoryBinding energyNuclear TheoryFOS: Physical sciences01 natural sciencesComputational physicsNuclear physicsNuclear Theory (nucl-th)0103 physical sciencesTensor010306 general physicsParametrizationOpen shellNuclear density
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