Search results for "ideal"

showing 10 items of 440 documents

An intrinsic characterization of spherically symmetric spacetimes

2010

We give the necessary and sufficient (local) conditions for a metric tensor to be a non conformally flat spherically symmetric solution. These conditions exclusively involve explicit concomitants of the Riemann tensor. As a direct application we obtain the {\em ideal} labeling of the Schwarzschild, Reissner-Nordstr\"om and Lema\^itre-Tolman-Bondi solutions.

PhysicsRiemann curvature tensorIdeal (set theory)Physics and Astronomy (miscellaneous)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Characterization (mathematics)General Relativity and Quantum CosmologyPhysics::History of PhysicsGeneral Relativity and Quantum Cosmologysymbols.namesakesymbolsSymmetric solutionMetric tensor (general relativity)Schwarzschild radiusMathematical physicsClassical and Quantum Gravity
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A Precise Determination of the Number of Families With Light Neutrinos and of the Z Boson Partial Widths

1990

Title : The socialization at work in the federal universe, the determining element of the social regulation of the sports organization. Contribution to the social politics of the sport service of Nice city Abstract : This study postulates the existence of certain specific cultural determinism in the social regulation of the sports organization. It leans on a work of inquiry which concerns 148 agents of the municipal service of the sports of the Nice city. The investigation puts in evidence a causal report between the type of trajectory of professional insertion of the municipal agents and their level of support in the manager politics of the organization. The agents, whose bibliographic rou…

PhysicsService (business)Nuclear and High Energy PhysicsParticle physicsbusiness.industrySocializationPublic relationsIdeal (ethics)PoliticsWork (electrical)Element (criminal law)businessParticle Physics - ExperimentCultural determinismUniverse (mathematics)
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State functions of ideal gases

2004

PhysicsState functionGas lawsMechanicsIdeal gas
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Test of mode coupling theory for a supercooled liquid of diatomic molecules.I. Translational degrees of freedom

1997

A molecular dynamics simulation is performed for a supercooled liquid of rigid diatomic molecules. The time-dependent self and collective density correlators of the molecular centers of mass are determined and compared with the predictions of the ideal mode coupling theory (MCT) for simple liquids. This is done in real as well as in momentum space. One of the main results is the existence of a unique transition temperature T_c, where the dynamics crosses over from an ergodic to a quasi-nonergodic behavior. The value for T_c agrees with that found earlier for the orientational dynamics within the error bars. In the beta- regime of MCT the factorization of space- and time dependence is satisf…

PhysicsStatistical Mechanics (cond-mat.stat-mech)Order (ring theory)FOS: Physical sciencesPosition and momentum spaceDisordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksDiatomic moleculePower lawQuantum mechanicsExponentRelaxation (physics)Ideal (ring theory)Structure factorCondensed Matter - Statistical Mechanics
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Dissipative terms of thermal nature in the theory of an ideal monoatomic superfluid

1996

A dissipative model of helium II was built up in previous works, using a 13-field extended thermodynamic theory formulated by Liu and Muller. In this work a generalization of such model is presented, where an extended thermodynamics with 14 fields due to Kremer is used. It is shown that the fourteenth field is able to account for the experimental data concerning the second sound attenuation. Further, the proposed theory is able to explain the Osborne experiment. Finally, a comparison with the two-fluid model is performed, emphasizing the different ways in which the dissipative phenomena are explained by the two theories.

PhysicsSuperfluidityWork (thermodynamics)Monatomic gasField (physics)GeneralizationApplied MathematicsGeneral MathematicsSecond soundDissipative systemGeneral Physics and AstronomyIdeal (order theory)Statistical physicsZAMP Zeitschrift f�r angewandte Mathematik und Physik
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Building a numerical relativistic non-ideal magnetohydrodynamics code for astrophysical applications

2013

AbstractIncluding resistive effects in relativistic magnetized plasmas is a challenging task, that a number of authors have recently tackled employing different methods. From the numerical point of view, the difficulty in including non-ideal terms arises from the fact that, in the limit of very high plasma conductivity (i.e., close to the ideal MHD limit), the system of governing equations becomes stiff, and the standard explicit integrating methods produce instabilities that destroy the numerical solution. To deal with such a difficulty, we have extended the relativistic MHD code MR-GENESIS, to include a number of Implicit Explicit Runge-Kutta (IMEX-RK) numerical methods. To validate the i…

PhysicsTheoretical physicsCode (set theory)Theory of relativityIdeal (set theory)Space and Planetary ScienceNumerical analysisAstronomy and AstrophysicsMagnetohydrodynamicsComputational physicsAIP Conf. Proc., in press (2013)
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Relativistic perfect fluids in local thermal equilibrium

2017

Every evolution of a fluid is uniquely described by an energy tensor. But the converse is not true: an energy tensor may describe the evolution of different fluids. The problem of determining them is called here the {\em inverse problem}. This problem may admit unphysical or non-deterministic solutions. This paper is devoted to solve the inverse problem for perfect energy tensors in the class of perfect fluids evolving in local thermal equilibrium (l.t.e.). The starting point is a previous result (Coll and Ferrando in J Math Phys 30: 2918-2922, 1989) showing that thermodynamic fluids evolving in l.t.e. admit a purely hydrodynamic characterization. This characterization allows solving this i…

PhysicsThermal equilibriumClass (set theory)Physics and Astronomy (miscellaneous)010308 nuclear & particles physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Characterization (mathematics)Inverse problem01 natural sciencesGeneral Relativity and Quantum CosmologyIdeal gasClassical mechanicsDifferential geometry0103 physical sciencesConversePoint (geometry)010306 general physics
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Ideal Gas Stephani Universes

2003

The Stephani Universes that can be interpreted as an ideal gas evolving in local thermal equilibrium are determined, and the method to obtain the associated thermodynamic schemes is given

PhysicsThermal equilibriumTheoretical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Ideal gasComputer Science::DatabasesGeneral Relativity and Quantum Cosmology
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Geometric Origin of the Tennis Racket Effect

2020

The tennis racket effect is a geometric phenomenon which occurs in a free rotation of a three-dimensional rigid body. In a complex phase space, we show that this effect originates from a pole of a Riemann surface and can be viewed as a result of the Picard-Lefschetz formula. We prove that a perfect twist of the racket is achieved in the limit of an ideal asymmetric object. We give upper and lower bounds to the twist defect for any rigid body, which reveals the robustness of the effect. A similar approach describes the Dzhanibekov effect in which a wing nut, spinning around its central axis, suddenly makes a half-turn flip around a perpendicular axis and the Monster flip, an almost impossibl…

Physics[PHYS]Physics [physics]Riemann surfaceGeneral Physics and AstronomyClassical Physics (physics.class-ph)FOS: Physical sciencesMathematical Physics (math-ph)Physics - Classical PhysicsRigid body01 natural sciencesUpper and lower boundssymbols.namesakePerpendicular AxisClassical mechanics[MATH.MATH-MP]Mathematics [math]/Mathematical Physics [math-ph]Phase space0103 physical sciencesRacketsymbolsIdeal (ring theory)Twist010306 general physicscomputerMathematical Physicscomputer.programming_language
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Upwind Relativistic MHD Code for Astrophysical Applications

2003

We describe the status of devolpment of a 2.5D numerical code to solve the equations of ideal relativistic magnetohydrodynamics. The numerical code, based on high-resolution shock-capturing techniques, solves the equations written in conservation form and computes the numerical fluxes using a linearized Riemann solver. A special procedure is used to force the conservation of magnetic flux along the evolution.

Physicssymbols.namesakeIdeal (set theory)Accretion discAstrophysics::High Energy Astrophysical PhenomenasymbolsCode (cryptography)Numerical fluxApplied mathematicsMagnetohydrodynamicsConservation formRiemann solverMagnetic flux
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