Search results for "Classical mechanics"

showing 10 items of 1211 documents

Nonlocal elasticity and related variational principles

2001

Abstract The Eringen model of nonlocal elasticity is considered and its implications in solid mechanics studied. The model is refined by assuming an attenuation function depending on the `geodetical distance' between material particles, such that in the diffusion processes of the nonlocality effects certain obstacles as holes or cracks existing in the domain can be circumvented. A suitable thermodynamic framework with nonlocality is also envisaged as a firm basis of the model. The nonlocal elasticity boundary-value problem for infinitesimal displacements and quasi-static loads is addressed and the conditions for the solution uniqueness are established. Three variational principles, nonlocal…

Applied MathematicsMechanical EngineeringCondensed Matter PhysicsFinite element methodQuantum nonlocalityClassical mechanicsMechanics of MaterialsVariational principleModeling and SimulationSolid mechanicsGeneral Materials ScienceDirect stiffness methodUniquenessElasticity (economics)MathematicsStiffness matrixInternational Journal of Solids and Structures
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Energy dissipative characteristic schemes for the diffusive Oldroyd-B viscoelastic fluid

2015

Applied MathematicsMechanical EngineeringMathematical analysisComputational MechanicsViscoelastic fluid010103 numerical & computational mathematics01 natural sciencesComputer Science Applications010101 applied mathematicsClassical mechanicsMechanics of MaterialsDissipative system0101 mathematicsEnergy (signal processing)MathematicsInternational Journal for Numerical Methods in Fluids
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Comparison between probe stagnation point heat flux measurements and correlation formulas in SCIROCCO plasma wind tunnel tests

2012

A large part of the SCIROCCO Arc Heater Performance Map has been investigated. The heat flux measurements at the stagnation point of t he facility Calibratio Probe have been used to find an experimental fit. Such a formula ha s been compared with the predictions of the De Filippis-Serpico equation and the well known Fay-Riddell formula. Finally the experimental fit has been also compared with the Sa gner-Verant formula obtained at the ONERA F4 hypersonic plasma wind tunnel.

Arc (geometry)Hypersonic speedClassical mechanicsHeat fluxmeasurements scirocco plasma wind tunnel testsPhysics::Space PhysicsSettore ING-IND/06 - FluidodinamicaPlasmaMechanicsStagnation pointMathematicsWind tunnel
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On the global dissipative and multipeakon dissipative behavior of the two-component Camassa-Holm system

2014

Published version of an article in the journal: Abstract and Applied Analysis. Also available from the publisher at: http://dx.doi.org/10.1155/2014/348695 Open Access The global dissipative and multipeakon dissipative behavior of the two-component Camassa-Holm shallow water system after wave breaking was studied in this paper. The underlying approach is based on a skillfully defined characteristic and a set of newly introduced variables which transform the original system into a Lagrangian semilinear system. It is the transformation, together with the associated properties, that allows for the continuity of the solution beyond collision time to be established, leading to a uniquely global d…

Article SubjectSemigroupComponent (thermodynamics)lcsh:MathematicsApplied MathematicsBreaking waveDissipative operatorAnalysis; Applied Mathematicslcsh:QA1-939CollisionVDP::Mathematics and natural science: 400::Mathematics: 410::Analysis: 411Dissipative solitonClassical mechanicsTransformation (function)Dissipative systemAnalysisMathematics
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Integrable models and degenerate horizons in two-dimensional gravity

1999

We analyse an integrable model of two-dimensional gravity which can be reduced to a pair of Liouville fields in conformal gauge. Its general solution represents a pair of ``mirror'' black holes with the same temperature. The ground state is a degenerate constant dilaton configuration similar to the Nariai solution of the Schwarzschild-de Sitter case. The existence of $\phi=const.$ solutions and their relation with the solution given by the 2D Birkhoff's theorem is then investigated in a more general context. We also point out some interesting features of the semiclassical theory of our model and the similarity with the behaviour of AdS$_2$ black holes.

AstrofísicaHigh Energy Physics - TheoryPhysicsGravitacióNuclear and High Energy PhysicsIntegrable systemCanonical quantizationDegenerate energy levelsFOS: Physical sciencesSemiclassical physicsConformal mapContext (language use)General Relativity and Quantum CosmologyClassical mechanicsde Sitter–Schwarzschild metricHigh Energy Physics - Theory (hep-th)DilatonMathematical physicsPhysical Review D
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Diffeomorphisms, Noether charges, and the canonical formalism in two-dimensional dilaton gravity

1995

We carry out a parallel study of the covariant phase space and the conservation laws of local symmetries in two-dimensional dilaton gravity. Our analysis is based on the fact that the Lagrangian can be brought to a form that vanishes on-shell giving rise to a well-defined covariant potential for the symplectic current. We explicitly compute the symplectic structure and its potential and show that the requirement to be finite and independent of the Cauchy surface restricts the asymptotic symmetries.

AstrofísicaPhysicsGravitacióSymplectic representationsymbols.namesakeSymplectic vector spaceCauchy surfaceClassical mechanicssymbolsDilatonNoether's theoremSymplectomorphismMathematics::Symplectic GeometrySymplectic geometryMathematical physicsSymplectic manifoldPhysical Review D
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Gravitational wave content and stability of uniformly, rotating, triaxial neutron stars in general relativity

2017

Targets for ground-based gravitational wave interferometers include continuous, quasiperiodic sources of gravitational radiation, such as isolated, spinning neutron stars. In this work we perform evolution simulations of uniformly rotating, triaxially deformed stars, the compressible analogues in general relativity of incompressible, Newtonian Jacobi ellipsoids. We investigate their stability and gravitational wave emission. We employ five models, both normal and supramassive, and track their evolution with different grid setups and resolutions, as well as with two different evolution codes. We find that all models are dynamically stable and produce a strain that is approximately one-tenth …

AstrofísicaPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGravitational waveGeneral relativityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Compact star01 natural sciencesGeneral Relativity and Quantum CosmologyArticleGravitational energyNumerical relativityClassical mechanicsTests of general relativity0103 physical sciencesAstronomiaTwo-body problem in general relativityAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsGravitational redshift
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Constraint preserving boundary conditions for the Z4c formulation of general relativity

2010

We discuss high order absorbing constraint preserving boundary conditions for the Z4c formulation of general relativity coupled to the moving puncture family of gauges. We are primarily concerned with the constraint preservation and absorption properties of these conditions. In the frozen coefficient approximation, with an appropriate first order pseudo-differential reduction, we show that the constraint subsystem is boundary stable on a four dimensional compact manifold. We analyze the remainder of the initial boundary value problem for a spherical reduction of the Z4c formulation with a particular choice of the puncture gauge. Numerical evidence for the efficacy of the conditions is prese…

AstrofísicaPhysicsNuclear and High Energy PhysicsGeneral relativityMathematical analysisBoundary (topology)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologySymmetry (physics)Constraint (information theory)Numerical relativityTheory of relativityClassical mechanicsAstronomiaCircular symmetryBoundary value problem
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Regularization of spherical and axisymmetric evolution codes in numerical relativity

2007

Several interesting astrophysical phenomena are symmetric with respect to the rotation axis, like the head-on collision of compact bodies, the collapse and/or accretion of fields with a large variety of geometries, or some forms of gravitational waves. Most current numerical relativity codes, however, can not take advantage of these symmetries due to the fact that singularities in the adapted coordinates, either at the origin or at the axis of symmetry, rapidly cause the simulation to crash. Because of this regularity problem it has become common practice to use full-blown Cartesian three-dimensional codes to simulate axi-symmetric systems. In this work we follow a recent idea idea of Rinne…

AstrofísicaPhysicsPhysics and Astronomy (miscellaneous)Gravitational waveRotational symmetryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmologylaw.inventionNumerical relativityClassical mechanicsDifferential geometrylawRegularization (physics)Homogeneous spaceAstronomiaCartesian coordinate systemGravitational singularityGeneral Relativity and Gravitation
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The barotropic model

2003

AtmospherePhysicsGeopotentialClassical mechanicsVorticity equationBarotropic fluidDynamics (mechanics)Balance equationAtmospheric modelOrr–Sommerfeld equationAtmospheric sciences
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