Search results for "Relativistic mechanics"

showing 7 items of 7 documents

Geometric Aspects of Mechanics

2010

In many respects, mechanics carries geometrical structures. This could be felt very clearly at various places in the first four chapters. The most important examples are the structures of the space–time continua that support the dynamics of nonrelativistic and relativistic mechanics, respectively. The formulation of Lagrangian mechanics over the space of generalized coordinates and their time derivatives, as well as of Hamilton–Jacobi canonical mechanics over the phase space, reveals strong geometrical features of these manifolds.

PhysicsPoisson bracketsymbols.namesakeGeneralized coordinatesGeometric mechanicsLagrangian mechanicsPhase spaceTangent spacesymbolsRelativistic mechanicsMechanicsAnalytical dynamics
researchProduct

Shock capturing methods in 1D numerical relativity

2008

A numerical code is presented which uses modern shock capturing methods to evolve spherically symmetric perfect fluid space-times. Harmonic slicing is used to ensure singularity avoidance, which is crucial in strong field situations. Some tests are presented, including an application to the stellar collapse problem.

PhysicsGravitational time dilationNumerical relativityClassical mechanicsTheory of relativityShock capturing methodRelativistic mechanicsPerfect fluidMechanicsIntroduction to the mathematics of general relativityTheoretical motivation for general relativityComputingMethodologies_COMPUTERGRAPHICS
researchProduct

Local Lorentz invariance tests for photons and hadrons at the Gamma Factory

2021

High-precision tests of local Lorentz invariance, via monitoring of the sidereal time variation of the photon energies emitted by ultrarelativistic heavy-ion beams and of the beam momentum, are proposed. This paper includes descriptions of the physics ideas and the concept for the detector. The experiment results will allow high-precision tests of LLI via anisotropy of the maximum attainable speed of a photon and an ion. The projected accuracy for the asymmetries interpreted in the framework of the anisotropic relativistic mechanics corresponds to the limit on sidereal time variation of the one-way maximum attainable speed at the levels between $10^{-14}$ and $10^{-17}$.

PhysicsPhotonHadronGeneral Physics and AstronomyFOS: Physical sciences02 engineering and technologyGeneral Relativity and Quantum Cosmology (gr-qc)Lorentz covarianceSpecial relativity021001 nanoscience & nanotechnology7. Clean energy01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics - Experiment3. Good healthMomentumHigh Energy Physics - Experiment (hep-ex)Sidereal timeQuantum electrodynamics0103 physical sciencesRelativistic mechanics010306 general physics0210 nano-technologyAnisotropy
researchProduct

Newtonian and relativistic emission coordinates

2009

Emission coordinates are those generated by positioning systems. Positioning systems are physical systems constituted by four emitters broadcasting their respective times by means of sound or light signals. We analyze the incidence of the space-time causal structure on the construction of emission coordinates. The Newtonian case of four emitters at rest is analyzed and contrasted with the corresponding situation in special relativity.

PhysicsNuclear and High Energy Physicssymbols.namesakeTheory of relativityClassical mechanicsLagrangian mechanicssymbolsRelativistic mechanicsRelativistic aberrationSpecial relativityAction-angle coordinatesIntroduction to the mathematics of general relativityTests of special relativityPhysical Review D
researchProduct

Two-dimensional approach to relativistic positioning systems

2006

A relativistic positioning system is a physical realization of a coordinate system consisting in four clocks in arbitrary motion broadcasting their proper times. The basic elements of the relativistic positioning systems are presented in the two-dimensional case. This simplified approach allows to explain and to analyze the properties and interest of these new systems. The positioning system defined by geodesic emitters in flat metric is developed in detail. The information that the data generated by a relativistic positioning system give on the space-time metric interval is analyzed, and the interest of these results in gravimetry is pointed out.

PhysicsNuclear and High Energy PhysicsPositioning systemGeodesicCoordinate systemFOS: Physical sciencesEnergy–momentum relationGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyRelativistic particleClassical mechanicsMetric (mathematics)Relativistic mechanics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Realization (systems)
researchProduct

Comparison of different boost transformations for the calculation of form factors in relativistic quantum mechanics

2002

The effect of different boost expressions, pertinent to the instant, front and point forms of relativistic quantum mechanics, is considered for the calculation of the ground-state form factor of a two-body system in simple scalar models. Results with a Galilean boost as well as an explicitly covariant calculation based on the Bethe-Salpeter approach are given for comparison. It is found that the present so-called point-form calculations of form factors strongly deviate from all the other ones. This suggests that the formalism which underlies them requires further elaboration. A proposition in this sense is made.

PhysicsParticle physics010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]FOS: Physical sciencesRelativistic quantum mechanics01 natural sciencesGalileanHigh Energy Physics - PhenomenologyFormalism (philosophy of mathematics)Classical mechanicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesRelativistic mechanicsCovariant transformation[PHYS.HTHE] Physics [physics]/High Energy Physics - Theory [hep-th]010306 general physics
researchProduct

General Relativistic Dynamics of Irrotational Dust: Cosmological Implications

1994

The non--linear dynamics of cosmological perturbations of an irrotational collisionless fluid is analyzed within General Relativity. Relativistic and Newtonian solutions are compared, stressing the different role of boundary conditions in the two theories. Cosmological implications of relativistic effects, already present at second order in perturbation theory, are studied and the dynamical role of the magnetic part of the Weyl tensor is elucidated.

PhysicsWeyl tensorGeneral relativityAstrophysics (astro-ph)Relativistic dynamicsFOS: Physical sciencesGeneral Physics and AstronomyEnergy–momentum relationAstrophysicsCenter of mass (relativistic)symbols.namesakeGeneral Relativity and Quantum CosmologyClassical mechanicssymbolsRelativistic mechanicsRelativistic quantum chemistryRelativistic speed
researchProduct