Search results for "classical mechanics"

showing 10 items of 1211 documents

Dynamics of thick discs around Schwarzschild-de Sitter black holes

2003

We consider the effects of a cosmological constant on the dynamics of constant angular momentum discs orbiting Schwarzschild-de Sitter black holes. The motivation behind this study is to investigate whether the presence of a radial force contrasting the black hole's gravitational attraction can influence the occurrence of the runaway instability, a robust feature of the dynamics of constant angular momentum tori in Schwarzschild and Kerr spacetimes. In addition to the inner cusp near the black hole horizon through which matter can accrete onto the black hole, in fact, a positive cosmological constant introduces also an outer cusp through which matter can leave the torus without accreting on…

Angular momentumAstrophysics::High Energy Astrophysical PhenomenaAccretion discs ; Black holes ; Relativity ; Hydrodynamics ; Cosmological constantFOS: Physical sciencesCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)UNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsInstabilityGeneral Relativity and Quantum CosmologyRelativityGravitationGeneral Relativity and Quantum CosmologyDe Sitter universeCosmological constantPhysicsBlack holesHorizonAstrophysics (astro-ph)Astronomy and AstrophysicsTorus:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Classical mechanicsSpace and Planetary ScienceHydrodynamicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaSchwarzschild radiusAccretion discs:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Relativistic simulations of rotational core collapse : I. Methods, initial models, and code tests

2002

We describe an axisymmetric general relativistic code for rotational core collapse. The code evolves the coupled system of metric and fluid equations using the ADM 3+1 formalism and a conformally flat metric approximation of the Einstein equations. The relativistic hydrodynamics equations are formulated as a first-order flux-conservative hyperbolic system and are integrated using high-resolution shock-capturing schemes based on Riemann solvers. We assess the quality of the conformally flat metric approximation for relativistic core collapse and present a comprehensive set of tests which the code successfully passed. The tests include relativistic shock tubes, the preservation of the rotatio…

Angular momentumAstrophysics::High Energy Astrophysical PhenomenaRotational symmetryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsNumerical methodAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAGeneral Relativity and Quantum CosmologyGravitational wavesGravitationRelativitysymbols.namesakeWaveformPhysicsAstrophysics (astro-ph)Astronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Hyperbolic systemsNeutron starRiemann hypothesisClassical mechanicsSpace and Planetary ScienceGravitational waves ; Hydrodynamics ; Numerical method ; RelativitysymbolsHydrodynamicsFluid equationUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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The planar two-body problem for spheroids and disks

2021

We outline a new method suggested by Conway (2016) for solving the two-body problem for solid bodies of spheroidal or ellipsoidal shape. The method is based on integrating the gravitational potential of one body over the surface of the other body. When the gravitational potential can be analytically expressed (as for spheroids or ellipsoids), the gravitational force and mutual gravitational potential can be formulated as a surface integral instead of a volume integral, and solved numerically. If the two bodies are infinitely thin disks, the surface integral has an analytical solution. The method is exact as the force and mutual potential appear in closed-form expressions, and does not invol…

Angular momentumInertial frame of reference010504 meteorology & atmospheric sciencesFOS: Physical sciencesTwo-body problem01 natural sciencesVolume integralGravitational potential0103 physical sciences010303 astronomy & astrophysicsMathematical Physics0105 earth and related environmental sciencesEarth and Planetary Astrophysics (astro-ph.EP)PhysicsVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430Applied MathematicsSurface integralEquations of motionAstronomy and AstrophysicsComputational Physics (physics.comp-ph)EllipsoidComputational MathematicsClassical mechanicsSpace and Planetary ScienceModeling and SimulationPhysics - Computational PhysicsAstrophysics - Earth and Planetary AstrophysicsCelestial Mechanics and Dynamical Astronomy
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Thouless-Valatin Rotational Moment of Inertia from the Linear Response Theory

2017

Spontaneous breaking of continuous symmetries of a nuclear many-body system results in appearance of zero-energy restoration modes. Such modes introduce a non-physical contributions to the physical excitations called spurious Nambu-Goldstone modes. Since they represent a special case of collective motion, they are sources of important information about the Thouless-Valatin inertia. The main purpose of this work is to study the Thouless-Valatin rotational moment of inertia as extracted from the Nambu-Goldstone restoration mode that results from the zero-frequency response to the total angular momentum operator. We examine the role and effects of the pairing correlations on the rotational cha…

Angular momentumNuclear Theorymedia_common.quotation_subjectNuclear TheoryFOS: Physical sciencesRotary inertiaInertia114 Physical sciences01 natural sciencesbinding energy and massesMoment of inertia factorNuclear Theory (nucl-th)symbols.namesake0103 physical sciences010306 general physicsRotational partition functionEuler's equationsEQUATIONSmedia_commonPhysicsta114nuclear density functional theory010308 nuclear & particles physicstiheysfunktionaaliteoriacollective modelsMoment of inertianuclear structure and decayssuprajuoksevuusRotational energyClassical mechanicssuperfluiditysymbolsydinfysiikka
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Angular Pseudomomentum Theory for the Generalized Nonlinear Schr\"{o}dinger Equation in Discrete Rotational Symmetry Media

2009

We develop a complete mathematical theory for the symmetrical solutions of the generalized nonlinear Schr\"odinger equation based on the new concept of angular pseudomomentum. We consider the symmetric solitons of a generalized nonlinear Schr\"odinger equation with a nonlinearity depending on the modulus of the field. We provide a rigorous proof of a set of mathematical results justifying that these solitons can be classified according to the irreducible representations of a discrete group. Then we extend this theory to non-stationary solutions and study the relationship between angular momentum and pseudomomentum. We illustrate these theoretical results with numerical examples. Finally, we…

Angular momentumRotational symmetryFOS: Physical sciencesMultidimensional discrete solitonsPattern Formation and Solitons (nlin.PS)01 natural sciences010305 fluids & plasmasSchrödinger equationsymbols.namesake0103 physical sciences010306 general physicsNonlinear Schrodinger equationNonlinear Sciences::Pattern Formation and SolitonsNonlinear Schrödinger equationMathematicsAngular pseudomomentumMathematical analysisFísicaStatistical and Nonlinear PhysicsCondensed Matter PhysicsNonlinear Sciences - Pattern Formation and SolitonsMathematical theoryCondensed Matter - Other Condensed MatterNonlinear systemClassical mechanicsIrreducible representationsymbolsDiscrete symmetry mediaSolitonMATEMATICA APLICADAOther Condensed Matter (cond-mat.other)
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A second strain gradient elasticity theory with second velocity gradient inertia – Part II: Dynamic behavior

2013

Abstract This paper is the sequel of a companion Part I paper devoted to the constitutive equations and to the quasi-static behavior of a second strain gradient material model with second velocity gradient inertia. In the present Part II paper, a multi-cell homogenization procedure (developed in the Part I paper) is applied to a nonhomogeneous body modelled as a simple material cell system, in conjunction with the principle of virtual work (PVW) for inertial actions (i.e. momenta and inertia forces), which at the macro-scale level takes on the typical format as for a second velocity gradient inertia material model. The latter (macro-scale) PVW is used to determine the equilibrium equations …

Angular momentummedia_common.quotation_subjectRotary inertiaPolhodeContinuum thermodynamicsInertiaMoment of inertia factorsymbols.namesakeMaterials Science(all)Modelling and SimulationGeneral Materials ScienceEuler's equationsmedia_commonMathematicsWave propagationApplied MathematicsMechanical EngineeringMathematical analysisMoment of inertiaCondensed Matter PhysicsRigid body dynamicsDynamicsGradient elasticityClassical mechanicsHigher order inertiaMechanics of MaterialsModeling and SimulationsymbolsInternational Journal of Solids and Structures
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A gradient elasticity theory for second-grade materials and higher order inertia

2012

Abstract Second-grade elastic materials featured by a free energy depending on the strain and the strain gradient, and a kinetic energy depending on the velocity and the velocity gradient, are addressed. An inertial energy balance principle and a virtual work principle for inertial actions are envisioned to enrich the set of traditional theoretical tools of thermodynamics and continuum mechanics. The state variables include the body momentum and the surface momentum, related to the velocity in a nonstandard way, as well as the concomitant mass-accelerations and inertial forces, which do intervene into the motion equations and into the force boundary conditions. The boundary traction is the …

Angular momentummedia_common.quotation_subjectTraction (engineering)Continuum thermodynamicsInertiaMaterials Science(all)Modelling and SimulationWave dispersionGeneral Materials ScienceVirtual workBoundary value problemmedia_commonMathematicsContinuum mechanicsForce densityMechanical EngineeringApplied MathematicsMathematical analysisEquations of motionCondensed Matter PhysicsDynamicsGradient elasticityClassical mechanicsHigher order inertiaMechanics of MaterialsModeling and SimulationInternational Journal of Solids and Structures
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Ejection and collision orbits of the spatial restricted three-body problem

1985

We begin by describing the global flow of the spatial two body rotating problem, μ=0. The remainder of the work is devoted to study the ejection and collision orbits when μ>-0. We make use of the ‘blow up’ techniques to show that for any fixed value of the Jacobian constant the set of these orbits is diffeomorphic to S2×R. Also we find some particular collision-ejection orbits.

Applied MathematicsAstronomy and AstrophysicsTwo-body problemThree-body problemCollisionCelestial mechanicsComputational Mathematicssymbols.namesakeClassical mechanicsSpace and Planetary ScienceModeling and SimulationAutomotive EngineeringJacobian matrix and determinantsymbolsOrbit (dynamics)Astrophysics::Earth and Planetary AstrophysicsRemainderConstant (mathematics)Mathematical PhysicsMathematicsCelestial Mechanics
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A class of shear deformable isotropic elastic plates with parametrically variable warping shapes

2017

A homogeneous shear deformable isotropic elastic plate model is addressed in which the normal transverse fibers are allowed to rotate and to warp in a physically consistent manner specified by a fixed value of a real non-negative warping parameter ω. On letting ω vary continuously (at fixed load and boundary conditions), a continuous family of shear deformable plates Pω is generated, which spans from the Kirchhoff plate at the lower limit ω=0, to the Mindlin plate at the upper limit ω=∞; for ω=2, Pω identifies with the third-order Reddy plate. The boundary-value problem for the generic plate Pω is addressed in the case of quasi-static loads, for which a principle of minimum total potential …

Applied MathematicsIsotropyComputational Mechanics02 engineering and technologyBending of plates021001 nanoscience & nanotechnologysymbols.namesake020303 mechanical engineering & transportsClassical mechanics0203 mechanical engineeringHarmonic functionHelmholtz free energyPlate theoryBiharmonic equationsymbolsBoundary value problemImage warping0210 nano-technologyMathematicsZAMM - Journal of Applied Mathematics and Mechanics / Zeitschrift für Angewandte Mathematik und Mechanik
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Figures of equilibrium in close binary systems

1992

The equilibrium configurations of close binary systems are analyzed. The autogravitational, centrifugal and tidal potentials are expanded in Clairaut's coordinates. From the set of the total potential angular terms an integral equations system is derived. The reduction of them to ordinary differential equations and the determination of the boundary conditions allow a formulation of the problem in terms of a single variable.

Applied MathematicsMathematical analysisfigure of celestial bodiesspherical harmonicsBinary numberSpherical harmonicsAstronomy and AstrophysicsIntegral equationCelestial mechanicsComputational MathematicsClassical mechanicsSpace and Planetary ScienceModeling and SimulationOrdinary differential equationPoisson equationsclose binary starsBoundary value problemPoisson's equationReduction (mathematics)Mathematical PhysicsMathematicsCelestial Mechanics and Dynamical Astronomy
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