Search results for "Tensor"

showing 10 items of 550 documents

Rigid motions relative to an observer:L-rigidity

1996

A new definition of rigidity,L-rigidity, in general relativity is proposed. This concept is a special class of pseudorigid motions and therefore it depends on the chosen curveL. It is shown that, for slow-rotation steady motions in Minkowski space, weak rigidity andL-rigidity are equivalent. The methods of the PPN approximation are considered. In this formalism, the equations that characterizeL-rigidity are expressed. As a consequence, the baryon mass density is constant in first order, the stress tensor is constant in the comoving system, the Newtonian potential is constant along the lineL, and the gravitational field is constant along the lineL in the comoving system.

PhysicsGeneral Relativity and Quantum CosmologyMathematics of general relativityRigidity (electromagnetism)Classical mechanicsNewtonian potentialPhysics and Astronomy (miscellaneous)Gravitational fieldGeneral relativityCauchy stress tensorGeneral MathematicsMinkowski spaceIntroduction to the mathematics of general relativityInternational Journal of Theoretical Physics
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An intrinsic characterization of the Schwarzschild metric

1998

An intrinsic algorithm that exclusively involves conditions on the metric tensor and its differential concomitants is presented to identify every type-D static vacuum solution. In particular, the necessary and sufficient explicit and intrinsic conditions are given for a Lorentzian metric to be the Schwarzschild solution.

PhysicsGeneral Relativity and Quantum CosmologyPhysics and Astronomy (miscellaneous)Schwarzschild coordinatesMetric signatureSchwarzschild geodesicsKerr metricSchwarzschild metricDeriving the Schwarzschild solutionMetric tensor (general relativity)Mathematical physicsIntrinsic metricClassical and Quantum Gravity
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On the geometry of Killing and conformal tensors

2006

The second order Killing and conformal tensors are analyzed in terms of their spectral decomposition, and some properties of the eigenvalues and the eigenspaces are shown. When the tensor is of type I with only two different eigenvalues, the condition to be a Killing or a conformal tensor is characterized in terms of its underlying almost-product structure. A canonical expression for the metrics admitting these kinds of symmetries is also presented. The space-time cases 1+3 and 2+2 are analyzed in more detail. Starting from this approach to Killing and conformal tensors a geometric interpretation of some results on quadratic first integrals of the geodesic equation in vacuum Petrov-Bel type…

PhysicsGeodesicGeneralizationFOS: Physical sciencesStatistical and Nonlinear PhysicsConformal mapGeneral Relativity and Quantum Cosmology (gr-qc)Type (model theory)General Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyQuadratic equationHomogeneous spaceTensorMathematical PhysicsEigenvalues and eigenvectorsMathematical physicsJournal of Mathematical Physics
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A new multidimensional, energy-dependent two-moment transport code for neutrino-hydrodynamics

2015

We present the new code ALCAR developed to model multidimensional, multi energy-group neutrino transport in the context of supernovae and neutron-star mergers. The algorithm solves the evolution equations of the 0th- and 1st-order angular moments of the specific intensity, supplemented by an algebraic relation for the 2nd-moment tensor to close the system. The scheme takes into account frame-dependent effects of order O(v/c) as well as the most important types of neutrino interactions. The transport scheme is significantly more efficient than a multidimensional solver of the Boltzmann equation, while it is more accurate and consistent than the flux-limited diffusion method. The finite-volum…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)DiscretizationFOS: Physical sciencesAstronomy and AstrophysicsContext (language use)SolverBoltzmann equationAlgebraic closureMoment (mathematics)Space and Planetary ScienceApplied mathematicsTensorNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Role of gravity in the pair creation induced by electric fields

2018

We analyze the pair production induced by homogenous, time-dependent electric fields in an expanding space-time background. We point out that, in obtaining the semiclassical Maxwell equations, two distinct notions of adiabatic renormalization are possible. In Minkowski space the two recipes turn out to be equivalent. However, in the presence of gravity only the recipe requiring an adiabatic hierarchy between the gravitational and the gauge field is consistent with the conservation of the energy-momentum tensor.

PhysicsHigh Energy Physics - Theory010308 nuclear & particles physicsSemiclassical physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyRenormalizationGravitationsymbols.namesakeClassical mechanicsMaxwell's equationsHigh Energy Physics - Theory (hep-th)0103 physical sciencesMinkowski spacesymbolsTensorGauge theory010306 general physicsAdiabatic process
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A new functional flow equation for Einstein-Cartan quantum gravity

2015

We construct a special-purpose functional flow equation which facilitates non-perturbative renormalization group (RG) studies on theory spaces involving a large number of independent field components that are prohibitively complicated using standard methods. Its main motivation are quantum gravity theories in which the gravitational degrees of freedom are carried by a complex system of tensor fields, a prime example being Einstein-Cartan theory, possibly coupled to matter. We describe a sequence of approximation steps leading from the functional RG equation of the Effective Average Action to the new flow equation which, as a consequence, is no longer fully exact on the untruncated theory sp…

PhysicsHigh Energy Physics - TheoryField (physics)Immirzi parameterAsymptotic safety in quantum gravityGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Action (physics)General Relativity and Quantum CosmologyTensor fieldFlow (mathematics)High Energy Physics - Theory (hep-th)Quantum gravityTensorMathematical physics
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Adiabatic regularization for spin-1/2 fields

2013

We extend the adiabatic regularization method to spin-1/2 fields. The ansatz for the adiabatic expansion for fermionic modes differs significantly from the WKB-type template that works for scalar modes. We give explicit expressions for the first adiabatic orders and analyze particle creation in de Sitter spacetime. As for scalar fields, the adiabatic method can be distinguished by its capability to overcome the UV divergences of the particle number operator. We also test the consistency of the extended method by working out the conformal and axial anomalies for a Dirac field in a Friedmann-Lemaitre-Robertson-Walker spacetime, in exact agreement with those obtained from other renormalization…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Quantum field theory in curved spacetimeParticle creationField (physics)De Sitter spaceScalar (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyRenormalizationTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Regularization (physics)Stress–energy tensorFísica nuclearEnergy-momentum tensorAdiabatic processAstrophysics - Cosmology and Nongalactic Astrophysics
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D=4 supergravity dynamically coupled to superstring in a superfield Lagrangian approach

2003

We elaborate a full superfield description of the interacting system of dynamical D=4, N=1 supergravity and dynamical superstring. As far as minimal formulation of the simple supergravity is used, such a system should contain as well the tensor (real linear) multiplet which describes the dilaton and the two-superform gauge field whose pull-back provides the Wess-Zumino term for the superstring. The superfield action is given by the sum of the Wess-Zumino action for D=4, N=1 superfield supergravity, the superfield action for the tensor multiplet in curved superspace and the Green-Schwarz superstring action. The latter includes the coupling to the tensor multiplet both in the Nambu-Goto and i…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsSupergravityHigh Energy Physics::PhenomenologySuperstring theoryFOS: Physical sciencesSupersymmetrySuperspaceString (physics)General Relativity and Quantum CosmologyHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Gauge theoryTensorMultipletMathematical physics
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Kaluza-Klein origin for the superstring tension

1992

The natural configuration space of a string in a background antisymmetric tensor potential is not loop space, but a principal U(1) bundle over loop space. This allows a Kaluza-Klein--like interpretation of the string tension as momentum along the U(1) fiber, and a similar interpretation is possible for a {ital p}-dimensional object. The higher-dimensional'' action incorporating this momentum as a dynamical variable is given for a {ital p}-dimensional supersymmetric extended object, in a general supergravity background. Its relevance, for a flat background, to classical anomalies'' in the supersymmetry algebra is explained.

PhysicsHigh Energy Physics::TheoryClassical mechanicsAntisymmetric tensorSupergravityLoop spaceKaluza–Klein theorySuperstring theorySupersymmetryString (physics)Supersymmetry algebraMathematical physicsPhysical Review D
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Testing vector-tensor gravity with current cosmological observations

2015

A certain vector-tensor theory of gravitation (VT) has been recently applied to cosmology (Phys. Rev. D, 89, 2014, 044035). It leads to encouraging results. The zero order energy density of the vector field accounts for the cosmological constant. It has been recently proved that the VT vector field cannot play the role of the electromagnetic field. The evolution of the scalar perturbations is different in VT and general relativity. Tensor fluctuations evolve in the same way in both theories. Here, the VT evolution equations of the scalar modes are appropriately written, and the initial conditions at high redshift - for numerical integration- are given. The codes COSMOMC and CAMB are modifie…

PhysicsHistoryGeneral relativityScalar (mathematics)Cosmological constantCosmologyComputer Science ApplicationsEducationGravitationsymbols.namesakeTheoretical physicssymbolsVector fieldTensorPlanckJournal of Physics: Conference Series
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