Search results for " Tensor"

showing 10 items of 210 documents

Existence of global weak solutions to the kinetic Peterlin model

2018

Abstract We consider a class of kinetic models for polymeric fluids motivated by the Peterlin dumbbell theories for dilute polymer solutions with a nonlinear spring law for an infinitely extensible spring. The polymer molecules are suspended in an incompressible viscous Newtonian fluid confined to a bounded domain in two or three space dimensions. The unsteady motion of the solvent is described by the incompressible Navier–Stokes equations with the elastic extra stress tensor appearing as a forcing term in the momentum equation. The elastic stress tensor is defined by Kramer’s expression through the probability density function that satisfies the corresponding Fokker–Planck equation. In thi…

PhysicsCauchy stress tensorApplied Mathematics010102 general mathematicsGeneral EngineeringGeneral MedicineSpace (mathematics)Kinetic energy01 natural sciencesPhysics::Fluid Dynamics010101 applied mathematicsComputational MathematicsNonlinear systemClassical mechanicsSpring (device)Bounded functionCompressibilityNewtonian fluid0101 mathematicsGeneral Economics Econometrics and FinanceAnalysisNonlinear Analysis: Real World Applications
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Low compressibility accretion disc formation in close binaries: the role of physical viscosity

2006

Aims. Physical viscosity naturally hampers gas dynamics (rarefaction or compression). Such a role should support accretion disc development inside the primary gravitation potential well in a close binary system, even for low compressibility modelling. Therefore, from the astrophysical point of view, highly viscous accretion discs could exist even in the low compressibility regime showing strong thermal differences to high compressibility ones Methods. We performed simulations of stationary Smooth Particle Hydrodynamics (SPH) low compressibility accretion disc models for the same close binary system. Artificial viscosity operates in all models. The absence of physical viscosity and a superso…

PhysicsCauchy stress tensorAstronomy and AstrophysicsAstrophysicsPhysics::Fluid DynamicsSmoothed-particle hydrodynamicsViscosityClassical mechanicsSpace and Planetary ScienceInviscid flowMass transferCompressibilityViscous stress tensorNavier–Stokes equationsAstrophysics::Galaxy AstrophysicsAstronomy & Astrophysics
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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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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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Partial wave decomposition of finite-range effective tensor interaction

2016

We perform a detailed analysis of the properties of the finite-range tensor term associated with the Gogny and M3Y effective interactions. In particular, by using a partial-wave decomposition of the equation of state of symmetric nuclear matter, we show how we can extract their tensor parameters directly from microscopic results based on bare nucleon-nucleon interactions. Furthermore, we show that the zero-range limit of both finite-range interactions has the form of the next-to-next-to-next-leading-order (N3LO) Skyrme pseudopotential, which thus constitutes a reliable approximation in the density range relevant for finite nuclei. Finally, we use Brueckner-Hartree-Fock results to fix the te…

PhysicsEquation of state[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear Theory010308 nuclear & particles physicsNuclear TheoryFOS: Physical sciencesNuclear matter01 natural sciencesPseudopotentialNuclear Theory (nucl-th)Range (mathematics)Classical mechanicsCartesian tensor0103 physical sciencesLimit (mathematics)Tensor010306 general physicsTensor density
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A programming guide for tensor networks with global SU(2) symmetry

2020

Abstract This paper is a manual with tips and tricks for programming tensor network algorithms with global S U ( 2 ) symmetry. We focus on practical details that are many times overlooked when it comes to implementing the basic building blocks of codes, such as useful data structures to store the tensors, practical ways of manipulating them, and adapting typical functions for symmetric tensors. Here we do not restrict ourselves to any specific tensor network method, but keep always in mind that the implementation should scale well for simulations of higher-dimensional systems using, e.g., Projected Entangled Pair States, where tensors with many indices may show up. To this end, the structur…

PhysicsFibonacci number010308 nuclear & particles physicsAlgebraic specificationGeneral Physics and AstronomyData structure01 natural sciencesTopological quantum computerAlgebraFusion tree0103 physical sciencesSymmetric tensorTensorSymmetry (geometry)010306 general physicsAnnals of Physics
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Rigid motions relative to an observer:L-rigidity

1996

A new definition of rigidity,L-rigidity, in general relativity is proposed. This concept is a special class of pseudorigid motions and therefore it depends on the chosen curveL. It is shown that, for slow-rotation steady motions in Minkowski space, weak rigidity andL-rigidity are equivalent. The methods of the PPN approximation are considered. In this formalism, the equations that characterizeL-rigidity are expressed. As a consequence, the baryon mass density is constant in first order, the stress tensor is constant in the comoving system, the Newtonian potential is constant along the lineL, and the gravitational field is constant along the lineL in the comoving system.

PhysicsGeneral Relativity and Quantum CosmologyMathematics of general relativityRigidity (electromagnetism)Classical mechanicsNewtonian potentialPhysics and Astronomy (miscellaneous)Gravitational fieldGeneral relativityCauchy stress tensorGeneral MathematicsMinkowski spaceIntroduction to the mathematics of general relativityInternational Journal of Theoretical Physics
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