Search results for " Tensor"

showing 10 items of 210 documents

Description and evolution of anisotropy in superfluid vortex tangles with counterflow and rotation

2006

We examine several vectorial and tensorial descriptions of the geometry of turbulent vortex tangles. We study the anisotropy in rotating counterflow experiments, in which the geometry of the tangle is especially interesting because of the opposite effects of rotation, which orients the vortices, and counterflow, which randomizes them. We propose to describe the anisotropy and the polarization of the vortex tangle through a tensor, which contains the first and second moments of the distribution of the unit vector ${\mathbf{s}}^{\ensuremath{'}}$ locally tangent to the vortex lines. We use an analogy with paramagnetism to estimate the anisotropy, the average polarization, the polarization fluc…

PhysicsQuantum fluidTangentAngular velocityCondensed Matter PhysicsMathematics::Geometric TopologyElectronic Optical and Magnetic MaterialsTangleVortexSuperfluidityexamine several vectorial and tensorialClassical mechanicsUnit vectorQuantum mechanicsAnisotropySettore MAT/07 - Fisica Matematica
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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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Type D vacuum solutions: a new intrinsic approach

2013

We present a new approach to the intrinsic properties of the type D vacuum solutions based on the invariant symmetries that these spacetimes admit. By using tensorial formalism and without explicitly integrating the field equations, we offer a new proof that the upper bound of covariant derivatives of the Riemann tensor required for a Cartan-Karlhede classification is two. Moreover we show that, except for the Ehlers-Kundt's C-metrics, the Riemann derivatives depend on the first order ones, and for the C-metrics they depend on the first order derivatives and on a second order constant invariant. In our analysis the existence of an invariant complex Killing vector plays a central role. It al…

PhysicsRiemann curvature tensorPure mathematicsPhysics and Astronomy (miscellaneous)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)Upper and lower boundsGeneral Relativity and Quantum Cosmologysymbols.namesakeRiemann hypothesisKilling vector fieldGeneral Relativity and Quantum CosmologyHomogeneous spacesymbolsCovariant transformationField equation
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An intrinsic characterization of the Kerr metric

2009

We give the necessary and sufficient (local) conditions for a metric tensor to be the Kerr solution. These conditions exclusively involve explicit concomitants of the Riemann tensor.

PhysicsRiemann curvature tensorsymbols.namesakePhysics and Astronomy (miscellaneous)Kerr metricsymbolsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Characterization (mathematics)Metric tensor (general relativity)General Relativity and Quantum CosmologyMathematical physics
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Measurement of K-e3(0) form factors

2004

The semi-leptonic decay of the neutral K meson $K^{0}_{L} \to \pi^{\pm}e^{\mp}\nu (K_{e3})$, was used to study the strangeness-changing weak interaction of hadrons. A sample of 5.6 million reconstructed events recorded by the NA48 experiment was used to measure the Dalitz plot density. Admitting all possible Lorentz-covariant couplings, the form factors for vector $(f_{+}(q^{2}))$, scalar $(f_{S})$ and tensor $(f_{T})$ interactions were measured. The linear slope of the vector form factor $\lambda_{+} = 0.0284 \pm 0.0007 \pm 0.0013$ and values for the ratios $|f_{S}/f_{+}(0)|=0.015^{+0.007}_{-0.010} \pm 0.012$ and $|f_{T}/f_{+}(0)|=0.05^{+0.03}_{-0.04} \pm 0.03$ were obtained. The values fo…

PhysicsSemileptonic decayNuclear and High Energy PhysicsMesonScalar (mathematics)HadronSEMI-LEPTONIC DECAYS; RADIATIVE-CORRECTIONS; TENSOR INTERACTIONS; MONTE-CARLO; KAONSForm factor (quantum field theory)Zero (complex analysis)Dalitz plotTENSOR INTERACTIONSWeak interactionSEMI-LEPTONIC DECAYSNOMONTE-CARLORADIATIVE-CORRECTIONSKAONSAtomic physicsParticle Physics - Experiment
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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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Non-Linear Relativistic Evolution of Cosmological Perturbations in Irrotational Dust

2008

PhysicsWeyl tensorNonlinear systemsymbols.namesakeDeformation tensorCosmological modelssymbolsAstronomyConservative vector fieldMathematical physics
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