Search results for "Relativitat"

showing 10 items of 20 documents

Method to obtain shear-free two-fluid solutions of Einstein's equations.

1989

We use the Einstein equations, stated as an initial-value problem (3+1 formalism), to present a method for obtaining a class of solutions which may be interpreted as the gravitational field produced by a mixture of two perfect fluids. The four-velocity of one of the components is assumed to be a shear-free, irrotational, and geodesic vector field. The solutions are given up to a set of a hyperbolic quasilinear system.

PhysicsGravitacióGeodesicPerfect fluidConservative vector fieldRelativitat (Física)symbols.namesakeGravitational fieldEinstein field equationssymbolsVector fieldEinsteinRicci curvatureMathematical physicsPhysical review. D, Particles and fields
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Stability of the intrinsic energy vanishing in the Schwarzschild metric under a slow rotation

2014

The linearized Kerr metric is considered and put in some Gauss coordinates which are further {\em intrinsic} ones. The linear and angular 4-momenta of this metric are calculated in these coordinates and the resulting value is just zero. Thus, the global vanishing previously found for the Schwarzschild metric remains linearly stable under slow rotational perturbations of this metric.

PhysicsGravitacióPhysics and Astronomy (miscellaneous)GaussKerr metricZero (complex analysis)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Stability (probability)General Relativity and Quantum CosmologySlow rotationRelativitat general (Física)Metric (mathematics)Schwarzschild metricEnergy (signal processing)Mathematical physicsGeneral Relativity and Gravitation
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On the uniqueness of the space-time energy in General Relativity. The illuminating case of the Schwarzschild metric

2013

The case of asymptotic Minkowskian space-times is considered. A special class of asymptotic rectilinear coordinates at the spatial infinity, related to a specific system of free falling observers, is chosen. This choice is applied in particular to the Schwarzschild metric, obtaining a vanishing energy for this space-time. This result is compared with the result of some known theorems on the uniqueness of the energy of any asymptotic Minkowskian space, showing that there is no contradiction between both results, the differences becoming from the use of coordinates with different operational meanings. The suitability of Gauss coordinates when defining an {\em intrinsic} energy is considered a…

PhysicsGravitacióPhysics and Astronomy (miscellaneous)General relativitySpace timemedia_common.quotation_subjectGaussFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)InfinitySpace (mathematics)General Relativity and Quantum CosmologyRelativitat general (Física)Schwarzschild metricUniquenessEnergy (signal processing)media_commonMathematical physics
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Two-point functions with an invariant Planck scale and thermal effects

2008

Nonlinear deformations of relativistic symmetries at the Planck scale are usually addressed in terms of modified dispersion relations. We explore here an alternative route by directly deforming the two-point functions of an underlying field theory. The proposed deformations depend on a length parameter (Planck length) and preserve the basic symmetries of the corresponding theory. We also study the physical consequences implied by these modifications at the Planck scale by analyzing the response function of an accelerated detector in Minkowski space, an inertial one in de Sitter space, and also in a black hole spacetime.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsPlanck energy010308 nuclear & particles physicsDe Sitter spacePlanck massPlanck momentumFOS: Physical sciences01 natural sciencessymbols.namesakeGeneral Relativity and Quantum CosmologyClassical mechanicsPlanck forceHigh Energy Physics - Theory (hep-th)Relativitat general (Física)0103 physical sciencessymbolsEspai i temps010306 general physicsPlanck unitsVirtual black holePlanck length
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Creatable universes

2007

We consider the question of properly defining energy and momenta for non asymptotic Minkowskian spaces in general relativity. Only spaces of this type, whose energy, linear 3-momentum, and intrinsic angular momentum vanish, would be candidates for creatable universes, that is, for universes which could have arisen from a vacuum quantum fluctuation. Given a universe, we completely characterize the family of coordinate systems for which one could sensibly say that this universe is a creatable universe.

PhysicsNuclear and High Energy PhysicsAngular momentumCosmologiaGeneral relativitymedia_common.quotation_subjectCoordinate systemAstrophysics (astro-ph)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Type (model theory)AstrophysicsUniverseGeneral Relativity and Quantum CosmologyTheoretical physicsRelativitat general (Física)Quantum fluctuationmedia_common
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Intrinsic energy of Lema\^itre-Tolman-Bondi models and cosmological implications

2013

Recently, some Lema{\^{\i}}tre-Tolman-Bondi metrics have been considered as models alternative to the dark energy within the Friedmann-Lema{\^{\i}}tre-Robertson-Walker universes. The vanishing of the intrinsic energy of these metrics is examined since such a vanishing, in the present case and in general, could be interpreted as a necessary condition to consider the possibility of the quantum creation of a metric. More specifically, this vanishing is examined in the particular case where the Lema{\^{\i}}tre-Tolman-Bondi metrics behave asymptotically like a Friedmann-Lema{\^{\i}}tre-Robertson-Walker universe. Finally, we deal with a particular model ruled out after being confronted with cosmi…

PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmologiamedia_common.quotation_subjectFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsUniversePhysics::History of PhysicsGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum CosmologyRelativitat general (Física)Metric (mathematics)Dark energyValue (mathematics)QuantumEnergy (signal processing)media_commonAstrophysics - Cosmology and Nongalactic Astrophysics
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Students' Understanding of the Special Theory of Relativity and Design for a Guided Visit to a Science Museum

2009

International audience; This paper describes the design of teaching materials that are used as learning tools in school visits to a science museum. An exhibition on the A century of the Special Theory of Relativity, in the Kutxaespacio Science Museum, in San Sebastian (Spain), was used to design a visit for first year engineering students at the university and assess the learning which was achieved. The first part of the paper presents the teaching sequence which was designed to build a bridge between formal teaching and the exhibition visit. The second part analyses the potential of the exhibition and the aforementioned teaching sequence to influence the students' knowledge of three aspect…

Science instructionMuseus de ciències4. EducationTeaching method05 social sciencesStudents understanding050301 educationRelativitat (Física)01 natural sciencesCiència EnsenyamentEducationExhibitionddc:370Engineering education0103 physical sciencesPedagogyMathematics educationComputingMilieux_COMPUTERSANDEDUCATIONCurriculum Teaching DidacticsSociologySocial Sciences & HumanitiesUnterricht Didaktik010306 general physicsBildung und Erziehung0503 education
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Two-Perfect Fluid Interpretation of an Energy Tensor

1990

The paper contains the necessary and sufficient conditions for a given energy tensor to be interpreted as a sum of two perfect fluids. Given a tensor of this class, the decomposition in two perfect fluids (which is determined up to a couple of real functions) is obtained.

Weyl tensorPhysicsTensor contractionFluidsPhysics and Astronomy (miscellaneous)Geometria diferencialMathematical analysisTensor fieldPhysics::Fluid Dynamicssymbols.namesakeExact solutions in general relativityRelativitat general (Física)symbolsSymmetric tensorStress–energy tensorTensorTensor density
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Els viatges de la física: perseguint ombres, mesurant meridians

2013

A partir del segle XVII l’estudi acurat i resolució de diversos problemes de la física, principalment relacionats amb l’astronomia i la forma de la Terra, però no sols, ha passat per realitzar mesures a diferents llocs i, per tant, per l’organització de viatges científics amb aquests objectius específics. Presentarem alguns d’aquests problemes i les solucions adoptades a l’època.

eclipse; Meridian; weather; relativity; travelhistoria de la cienciaeclipse; meridiano; meteorología; relatividad; viajeMultidisciplinaryhistòria de la ciènciarelativityMeteorologyeclipseviatgerelativitatrelatividadmeridiàMeridianmeteorologíameteorologiaHistory and Philosophy of Sciencehistory of scienceweathermeridianoeclipsieclipsi; meridià; meteorologia; relativitat; viatgeHumanitiestravelviaje
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Mecànica II

2020

El document forma part dels materials docents programats mitjançant l'ajut del Servei de Política Lingüística de la Universitat de València Apunts de l'assignatura de Mecànica II, amb tres temaris principals: Formulació Lagrangiana (part 1), Formulació Hamiltoniana (part 2) i Relativitat Especial (part 3). Notes of the course 'Mecànica II', with three main topics: Lagrangian formulation (part 1), Hamiltonian formulation (part 2) and Special Relativity (part 3).

lagrangiàmecànica newtonianaUNESCO::FÍSICAhamiltoniàrelativitat especial
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