Search results for "General relativity"

showing 10 items of 1057 documents

Type I vacuum solutions with aligned Papapetrou fields: an intrinsic characterization

2003

We show that Petrov type I vacuum solutions admitting a Killing vector whose Papapetrou field is aligned with a principal bivector of the Weyl tensor are the Kasner and Taub metrics, their counterpart with timelike orbits and their associated windmill-like solutions, as well as the Petrov homogeneous vacuum solution. We recover all these metrics by using an integration method based on an invariant classification which allows us to characterize every solution. In this way we obtain an intrinsic and explicit algorithm to identify them.

PhysicsWeyl tensorFOS: Physical sciencesStatistical and Nonlinear PhysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyKilling vector fieldsymbols.namesakeGeneral Relativity and Quantum CosmologyHomogeneoussymbolsInvariant (mathematics)BivectorMathematical PhysicsMathematical physics
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Covariant determination of the Weyl tensor geometry

2001

We give a covariant and deductive algorithm to determine, for every Petrov type, the geometric elements associated with the Weyl tensor: principal and other characteristic 2-forms, Debever null directions and canonical frames. We show the usefulness of these results by applying them in giving the explicit characterization of two families of metrics: static type I spacetimes and type III metrics with a hypersurface-orthogonal Killing vector. PACS numbers: 0240M, 0420C

PhysicsWeyl tensorGeneral Relativity and Quantum CosmologyKilling vector fieldPure mathematicssymbols.namesakePhysics and Astronomy (miscellaneous)Null (mathematics)symbolsCovariant transformationType (model theory)Characterization (mathematics)Classical and Quantum Gravity
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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
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On the invariant symmetries of the D-metrics

2007

We analyze the symmetries and other invariant qualities of the $\mathcal{D}$-metrics (type D aligned Einstein Maxwell solutions with cosmological constant whose Debever null principal directions determine shear-free geodesic null congruences). We recover some properties and deduce new ones about their isometry group and about their quadratic first integrals of the geodesic equation, and we analyze when these invariant symmetries characterize the family of metrics. We show that the subfamily of the Kerr-NUT solutions are those admitting a Papapetrou field aligned with the Weyl tensor.

PhysicsWeyl tensorGeodesicNull (mathematics)Statistical and Nonlinear PhysicsCosmological constantType (model theory)General Relativity and Quantum Cosmologysymbols.namesakeHomogeneous spacesymbolsInvariant (mathematics)Isometry groupMathematical PhysicsMathematical physicsJournal of Mathematical Physics
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Gravito-magnetic vacuum spacetimes: kinematic restrictions

2003

We show that there are no vacuum solutions with a purely magnetic Weyl tensor with respect to an observer submitted to kinematic restrictions involving first order differential scalars. This result generalizes previous ones for the vorticity-free and shear-free cases. We use a covariant approach which makes evident that only the Bianchi identities are used and, consequently, the results are also valid for non vacuum solutions with vanishing Cotton tensor.

PhysicsWeyl tensorPhysics and Astronomy (miscellaneous)Cotton tensorFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)KinematicsFirst orderObserver (physics)General Relativity and Quantum Cosmologysymbols.namesakeGeneral Relativity and Quantum CosmologysymbolsCovariant transformationDifferential (mathematics)Mathematical physics
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Obtaining the Weyl tensor from the Bel-Robinson tensor

2010

The algebraic study of the Bel-Robinson tensor proposed and initiated in a previous work (Gen. Relativ. Gravit. {\bf 41}, see ref [11]) is achieved. The canonical form of the different algebraic types is obtained in terms of Bel-Robinson eigen-tensors. An algorithmic determination of the Weyl tensor from the Bel-Robinson tensor is presented.

PhysicsWeyl tensorPhysics and Astronomy (miscellaneous)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmologysymbols.namesakeGeneral Relativity and Quantum CosmologyTensor (intrinsic definition)symbolsAlgebraic data typeCanonical formAlgebraic numberMathematics::Representation TheoryMathematical physics
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The runaway instability of thick discs around black holes. II. Non constant angular momentum discs

2003

We present results from a comprehensive number of relativistic, time-dependent, axisymmetric simulations of the runaway instability of non-constant angular momentum thick discs around black holes. This second paper extends earlier results where only constant angular momentum discs were considered. All relevant aspects of the theory of stationary thick discs around rotating black holes, necessary to build the initial state in our simulations, are presented in great detail. The angular momentum of the discs is assumed to increase outwards with the radial distance according to a power law. The main simplifying assumptions of our approach are not to include magnetic fields and self-gravity in t…

PhysicsWhite holeAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsGeneral Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyRotating black holeBinary black holeSpace and Planetary ScienceExtremal black holeStellar black holeAstrophysics::Earth and Planetary AstrophysicsSchwarzschild radiusHawking radiation
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On the convexity of relativistic ideal magnetohydrodynamics

2015

We analyze the influence of the magnetic field in the convexity properties of the relativistic magnetohydrodynamics system of equations. To this purpose we use the approach of Lax, based on the analysis of the linearly degenerate/genuinely non-linear nature of the characteristic fields. Degenerate and non-degenerate states are discussed separately and the non-relativistic, unmagnetized limits are properly recovered. The characteristic fields corresponding to the material and Alfv\'en waves are linearly degenerate and, then, not affected by the convexity issue. The analysis of the characteristic fields associated with the magnetosonic waves reveals, however, a dependence of the convexity con…

Physics[PHYS]Physics [physics]Special relativityPhysics and Astronomy (miscellaneous)Equation of state (cosmology)Degenerate energy levelsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Special relativityGeneral Relativity and Quantum CosmologyConvexityMagnetic field83A05 76W05 35L60 35L65Nonlinear systemConvexityMagnetohydrodynamicsFlow (mathematics)Magnetohydrodynamics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]ComputingMilieux_MISCELLANEOUSMathematical physicsAstronomía y Astrofísica
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Switching synchronization in one-dimensional memristive networks: An exact solution.

2017

We study a switching synchronization phenomenon taking place in one-dimensional memristive networks when the memristors switch from the high- to low-resistance state. It is assumed that the distributions of threshold voltages and switching rates of memristors are arbitrary. Using the Laplace transform, a set of nonlinear equations describing the memristors dynamics is solved exactly, without any approximations. The time dependencies of memristances are found, and it is shown that the voltage falls across memristors are proportional to their threshold voltages. A compact expression for the network switching time is derived.

Physicsbusiness.product_categoryLaplace transformMemristorTopology01 natural sciencesSynchronization010305 fluids & plasmaslaw.inventionNonlinear systemComputer Science::Emerging TechnologiesExact solutions in general relativitylaw0103 physical sciencesNetwork switchState (computer science)010306 general physicsbusinessVoltagePhysical review. E
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The virial theorem and the dark matter problem in hybrid metric-Palatini gravity

2012

Hybrid metric-Palatini gravity is a recently proposed theory, consisting of the superposition of the metric Einstein-Hilbert Lagrangian with an f(R) term constructed a la Palatini. The theory predicts the existence of a long-range scalar field, which passes the Solar System observational constraints, even if the scalar field is very light, and modifies the cosmological and galactic dynamics. Thus, the theory opens new possibilities to approach, in the same theoretical framework, the problems of both dark energy and dark matter. In this work, we consider the generalized virial theorem in the scalar-tensor representation of the hybrid metric-Palatini gravity. More specifically, taking into ac…

Physicsdark matter theory010308 nuclear & particles physicsDark matterVelocity dispersionFOS: Physical sciencesAstronomy and AstrophysicsVirial massAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesPotential energyGeneral Relativity and Quantum CosmologyVirial theoremTheoretical physicsGeneral Relativity and Quantum CosmologyPhysics - General PhysicsGeneral Physics (physics.gen-ph)Gravitational field0103 physical sciencesDark energygalaxy clusters010303 astronomy & astrophysicsScalar fieldmodified gravity
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