Search results for "WTO"

showing 10 items of 163 documents

The Vlasov Limit for a System of Particles which Interact with a Wave Field

2008

In two recent publications [Commun. PDE, vol.22, p.307--335 (1997), Commun. Math. Phys., vol.203, p.1--19 (1999)], A. Komech, M. Kunze and H. Spohn studied the joint dynamics of a classical point particle and a wave type generalization of the Newtonian gravity potential, coupled in a regularized way. In the present paper the many-body dynamics of this model is studied. The Vlasov continuum limit is obtained in form equivalent to a weak law of large numbers. We also establish a central limit theorem for the fluctuations around this limit.

PhysicsContinuum (measurement)Point particle010102 general mathematicsStatistical and Nonlinear Physics16. Peace & justice01 natural sciencesvlasov limitLaw of large numbers[NLIN.NLIN-CD]Nonlinear Sciences [physics]/Chaotic Dynamics [nlin.CD]0103 physical sciencesNewtonian fluid010307 mathematical physics0101 mathematicsComputingMilieux_MISCELLANEOUSMathematical PhysicsMathematical physicsCentral limit theoremCommunications in Mathematical Physics
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Step-Edge Induced Anisotropic Domain-Wall Propagation

1999

We report the observation of anisotropic domain-wall propagation in ultrathin magnetic films with perpendicular anisotropy. A controlled density of step edges was introduced which allowed us to quantify its influence on the domain-wall pinning. For a sawtooth arrangement of the step edges the corresponding wall movement resulted in triangular shaped domains. All aspects of this anisotropic domain-wall evolution could be reproduced by a simulation based on a modified Ginzburg-Landau-type soft-spin model.

PhysicsDomain wall (magnetism)Condensed matter physicsCondensed Matter::SuperconductivityGeneral Physics and AstronomyStep edgesPerpendicular anisotropyMagnetic filmsSawtooth waveEdge (geometry)AnisotropySimulation basedPhysical Review Letters
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Hydrodynamical forces acting on particles in a two-dimensional flow near a solid wall

2000

The hydrodynamical forces acting on a single particle and on a random rigid array of particles suspended in a two-dimensional shear flow of Newtonian fluid near a rigid wall were studied numerically in the flow regime where the relevant Reynolds numbers are of the order of unity. The simulations were done with conventional finite volume method for single-particle cases and with lattice-Boltzmann method for many-particle cases. A set of comparison cases was solved with both methods in order to check the accuracy of the lattice-Boltzmann method. For the single-particle case analytic formulae for the longitudinal drag force and for the transverse lift force were found. A modification to Darcy'…

PhysicsFinite volume methodGeneral Physics and AstronomyReynolds numberMechanicsPhysics::Fluid Dynamicssymbols.namesakeClassical mechanicsFlow (mathematics)Hardware and ArchitectureDragsymbolsNewtonian fluidParticleTwo-dimensional flowShear flow
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Diffusion in Flashing Periodic Potentials

2005

The one-dimensional overdamped Brownian motion in a symmetric periodic potential modulated by external time-reversible noise is analyzed. The calculation of the effective diffusion coefficient is reduced to the mean first passage time problem. We derive general equations to calculate the effective diffusion coefficient of Brownian particles moving in arbitrary supersymmetric potential modulated: (i) by external white Gaussian noise and (ii) by Markovian dichotomous noise. For both cases the exact expressions for the effective diffusion coefficient are derived. We obtain acceleration of diffusion in comparison with the free diffusion case for fast fluctuating potentials with arbitrary profil…

PhysicsFluctuating Rectangular Periodic PotentialStatistical Mechanics (cond-mat.stat-mech)Mathematical analysisFOS: Physical sciencesSawtooth waveCondensed Matter - Soft Condensed MatterCondensed Matter PhysicsNoise (electronics)Electronic Optical and Magnetic Materialssymbols.namesakeAccelerationAdditive white Gaussian noisesymbolsSoft Condensed Matter (cond-mat.soft)Effective diffusion coefficientDiffusion (business)First-hitting-time modelBrownian motionCondensed Matter - Statistical Mechanics
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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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Post-Newtonian constraints onf(R)cosmologies in metric and Palatini formalism

2005

We compute the complete post-Newtonian limit of both the metric and Palatini formulations of $f(R)$ gravities using a scalar-tensor representation. By comparing the predictions of these theories with laboratory and solar system experiments, we find a set of inequalities that any lagrangian $f(R)$ must satisfy. The constraints imposed by those inequalities allow us to find explicit bounds to the possible nonlinear terms of the lagrangian. We conclude that in both formalisms the lagrangian $f(R)$ must be almost linear in $R$ and that corrections that grow at low curvatures are incompatible with observations. This result shows that modifications of gravity at very low cosmic densities cannot b…

PhysicsGravitationNuclear and High Energy Physicssymbols.namesakeNonlinear systemCOSMIC cancer databaseObservational cosmologysymbolsNewtonian fluidRotation formalisms in three dimensionsLagrangianCosmologyMathematical physicsPhysical Review D
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(2+1)-dimensional Einstein-Kepler problem in the centre-of-mass frame

1999

We formulate and analyze the Hamiltonian dynamics of a pair of massive spinless point particles in (2+1)-dimensional Einstein gravity by anchoring the system to a conical infinity, isometric to the infinity generated by a single massive but possibly spinning particle. The reduced phase space \Gamma_{red} has dimension four and topology R^3 x S^1. \Gamma_{red} is analogous to the phase space of a Newtonian two-body system in the centre-of-mass frame, and we find on \Gamma_{red} a canonical chart that makes this analogue explicit and reduces to the Newtonian chart in the appropriate limit. Prospects for quantization are commented on.

PhysicsHamiltonian mechanicsPhysics and Astronomy (miscellaneous)One-dimensional spaceFOS: Physical sciencesConical surfaceGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyQuantization (physics)symbols.namesakeKepler problemPhase spacesymbolsNewtonian fluidEinsteinMathematical physics
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Running Newton Constant, Improved Gravitational Actions, and Galaxy Rotation Curves

2004

A renormalization group (RG) improvement of the Einstein-Hilbert action is performed which promotes Newton's constant and the cosmological constant to scalar functions on spacetime. They arise from solutions of an exact RG equation by means of a ``cutoff identification'' which associates RG scales to the points of spacetime. The resulting modified Einstein equations for spherically symmetric, static spacetimes are derived and analyzed in detail. The modifications of the Newtonian limit due to the RG evolution are obtained for the general case. As an application, the viability of a scenario is investigated where strong quantum effects in the infrared cause Newton's constant to grow at large …

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsAstrophysics (astro-ph)Dark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantNewtonian limitAstrophysicsGeneral Relativity and Quantum CosmologyGravitationsymbols.namesakeGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Einstein field equationssymbolsSchwarzschild metricWeyl transformationGalaxy rotation curveMathematical physics
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A Fractional Approach to Non-Newtonian Blood Rheology in Capillary Vessels

2019

In small arterial vessels, fluid mechanics involving linear viscous fluid does not reproduce experimental results that correspond to non-parabolic profiles of velocity across the vessel diameter. In this paper, an alternative approach is pursued introducing long-range interactions that describe the interactions of non-adjacent fluid volume elements due to the presence of red blood cells and other dispersed cells in plasma. These non-local forces are defined as linearly dependent on the product of the volumes of the considered elements and on their relative velocity. Moreover, as the distance between two volume elements increases, the non-local forces decay with a material distance-decaying …

PhysicsNon-local modelRelative velocityNon-local fluidFluid mechanicsBlood flowFunction (mathematics)MechanicsViscous liquidFractional calculuNon-Newtonian fluidPhysics::Fluid DynamicsVolume (thermodynamics)RheologyMesoscale approachSolid mechanicsJournal of Peridynamics and Nonlocal Modeling
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Structure and dynamics of sawteeth crashes in ASDEX Upgrade

2010

The crash phase of the sawteeth in ASDEX Upgrade tokamak [Herrmann et al., Fusion Sci. Technol. 44(3), 569 (2003)] is investigated in detail in this paper by means of soft x-ray (SXR) and electron cyclotron emission (ECE) diagnostics. Analysis of precursor and postcursor (1,1) modes shows that the crash does not affect the position of the resonant surface q=1. Our experimental results suggest that sawtooth crash models should contain two ingredients to be consistent with experimental observations: (1) the (1,1) mode structure should survive the crash and (2) the flux changes should be small to preserve the position of the q=1 surface close to its original location. Detailed structure of the…

PhysicsNuclear physicsTokamakASDEX UpgradelawCyclotronPhase (waves)Magnetic reconnectionPlasma diagnosticsSawtooth waveCondensed Matter PhysicsInstabilitylaw.inventionPhysics of Plasmas
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