Search results for "Relativity"

showing 10 items of 1213 documents

The Random-Phase Approximation

2007

In this chapter we extend the TDA particle-hole formalism of Chap. 9 to include correlations in the nuclear ground state. This sophisticated particle-hole formalism is called the random-phase approximation (RPA). In this description the simple Hartree-Fock particle-hole vacuum is replaced by a correlated ground state involving many-particle-many-hole excitations of the simple particle-hole vacuum. The resulting configuration mixing in excited states is more involved in the RPA than it is in the TDA. The ground-state correlations induce both particle-hole and hole-particle components in the RPA wave function.

PhysicsGeneral Relativity and Quantum CosmologyMuffin-tin approximationAstrophysics::High Energy Astrophysical PhenomenaQuantum mechanicsExcited stateNuclear TheoryBorn–Huang approximationDiscrete dipole approximation codesSpouge's approximationGround stateRandom phase approximationEikonal approximation
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Numerical relativistic hydrodynamics: Local characteristic approach.

1991

We extend some recent Ishock capturing methodsR designed to solve nonlinear hyperbolic systems of conservation laws and which avoid the use of artifical viscosity for treating strong discontinuities to a relativistic hydrodynamics system of equations. Some standard shock-tube problems and radial accretion onto a Schwarzschild black hole are used to calibrate our code.

PhysicsGeneral Relativity and Quantum CosmologyNonlinear systemConservation lawTheory of relativityClassical mechanicsAstrophysics::High Energy Astrophysical PhenomenaViscosity (programming)Schwarzschild metricFluid mechanicsClassification of discontinuitiesSystem of linear equationsPhysical review. D, Particles and fields
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New solutions of the hamiltonian and diffeomorphism constraints of quantum gravity from a highest weight loop representation

1991

Abstract We introduce a highest weight type representation of the Rovelli-Smolin algebra of loop observables for quantum gravity. In terms of this representation, new solutions of the hamiltonian and diffeomorphism constraints are given. Assuming the locality of the quantum hamiltonian constraint we show that any functional depending on the generalized link class of the disjoint union of arbitrary simple loops is a solution. Finally we argue that this is the general solution in the irreducible representation space.

PhysicsGeneral Relativity and Quantum CosmologyNuclear and High Energy PhysicsPure mathematicsHamiltonian constraintQuantum mechanicsIrreducible representationTrivial representationWheeler–DeWitt equationQuantum gravityLoop quantum gravityCanonical quantum gravityDiffeomorphism constraintPhysics Letters B
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A simple microsuperspace model in 2 + 1 spacetime dimensions

1992

Abstract We quantize the closed Friedmann model in 2 + 1 spacetime dimensions using euclidean path-integral approach and a simple microsuperspace model. A relationship between integration measure and operator ordering in the Wheeler-DeWitt equation is found within our model. Solutions to the Wheeler-DeWitt equation are exactly reproduced from the path integral using suitable integration contours in the complex plane.

PhysicsGeneral Relativity and Quantum CosmologyNuclear and High Energy PhysicsSpacetimeTwo-dimensional spaceQuantum mechanicsPath integral formulationEuclidean geometryMathematical analysisMeasure (physics)Wheeler–DeWitt equationQuantum gravityComplex planePhysics Letters B
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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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The Quantum Scalar Field in Spherically Symmetric Loop Quantum Gravity

2013

We consider the quantization of a spherically symmetric gravitational system coupled to a massless scalar field within the loop quantum gravity framework. Our results rely on the uniform discretizations method developed during the last years. We minimize the associated discrete “master constraint” using a trial state whose gravitational part is peaked around the classical Schwarzschild solution.

PhysicsGeneral Relativity and Quantum CosmologyQuantization (physics)Quantum geometryClassical mechanicsSpin foamQuantum gravitySemiclassical gravityLoop quantum gravityScalar fieldLoop quantum cosmology
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Aligned Electric and Magnetic Weyl Fields

2003

We analyze the spacetimes admitting a direction for which the relative electric and magnetic Weyl fields are aligned. We give an invariant characterization of these metrics and study the properties of its Debever null vectors. The directions 'observing' aligned electric and magnetic Weyl fields are obtained for every Petrov type. The results on the no existence of purely magnetic solutions are extended to the wider class having homothetic electric and magnetic Weyl fields.

PhysicsGeneral Relativity and Quantum CosmologyTheoretical physicsPhysics and Astronomy (miscellaneous)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Type (model theory)Invariant (mathematics)Null (physics)General Relativity and Quantum CosmologyHomothetic transformationGeneral Relativity and Gravitation
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A covariant determination of the Weyl canonical frames in Petrov type I spacetimes

1997

A covariant algorithm is given to obtain principal 2-forms, Debever null directions and canonical frames associated with Petrov type I Weyl tensors. The relationship between these Weyl elements is explained, and their explicit expressions depending on Weyl invariants are obtained. These results are used to determine a cosmological observer in type I universes, and their usefulness in spacetime intrinsic characterization is shown.

PhysicsGeneral Relativity and Quantum Cosmologysymbols.namesakePhysics and Astronomy (miscellaneous)SpacetimeNull (mathematics)symbolsWeyl transformationCovariant transformationCharacterization (mathematics)Type (model theory)Observer (physics)Mathematical physicsClassical and Quantum Gravity
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Particle-Hole Excitations and the Tamm-Dancoff Approximation

2007

This chapter describes the configuration mixing of particle-hole excitations in doubly magic nuclei. The discussion is confined to one-particle-one-hole excitations within the simplest scheme of configuration mixing, namely the Tamm-Dancoff approximation (TDA). We show that the TDA arises from a variational principle and leads to diagonalization of the residual Hamiltonian in a basis of particle-hole excitations of the particle-hole vacuum.

PhysicsGeneral Relativity and Quantum Cosmologysymbols.namesakeVariational principleAstrophysics::High Energy Astrophysical PhenomenaQuantum mechanicsBorn–Huang approximationsymbolsHamiltonian (quantum mechanics)
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Numerical 3+1 general relativistic magnetohydrodynamics: a local characteristic approach

2005

We present a general procedure to solve numerically the general relativistic magnetohydrodynamics (GRMHD) equations within the framework of the 3+1 formalism. The work reported here extends our previous investigation in general relativistic hydrodynamics (Banyuls et al. 1997) where magnetic fields were not considered. The GRMHD equations are written in conservative form to exploit their hyperbolic character in the solution procedure. All theoretical ingredients necessary to build up high-resolution shock-capturing schemes based on the solution of local Riemann problems (i.e. Godunov-type schemes) are described. In particular, we use a renormalized set of regular eigenvectors of the flux Jac…

PhysicsGeneral relativityAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsGeneral Relativity and Quantum CosmologyMagnetic fieldRiemann hypothesissymbols.namesakeClassical mechanicsRotating black holeSpace and Planetary ScienceMagnetorotational instabilitysymbolsSchwarzschild metricMagnetohydrodynamicsEigenvalues and eigenvectors
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