Search results for "classical"

showing 10 items of 2294 documents

Geometric efficiency for a circular detector and a linear source of arbitrary orientation and position

2010

A new axisymmetric radiation vector potential which is singular along its entire axis of symmetry is derived for a spherically symmetric point radiation source. This potential and a previously given non-singular point source potential are integrated to give radiation vector potentials for a straight linear source of constant strength. Analytical solutions are given for the geometric efficiency G of a line source and a circular disk detector when the line source is parallel to the detector axis. The analytical solution is also given for the case where the line source is parallel to the disk surface, such that the source axis and the detector axis intersect. All other cases are given as simpl…

PhysicsNuclear and High Energy PhysicsClassical mechanicsPlane (geometry)Position (vector)Point sourceOrientation (geometry)Mathematical analysisDetectorRotational symmetryInstrumentationLine sourceVector potentialNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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The two-loop three-point functions. General massive cases

1992

Abstract We present a calculation of the two-loop three-point scalar functions for the two overlapping topologies. These are the master functions for the ladder and the crossed ladder graphs. We also present a method for the extraction of possible (on-shell) mass singularities.

PhysicsNuclear and High Energy PhysicsClassical mechanicsScalar (mathematics)Condensed Matter::Strongly Correlated ElectronsGravitational singularityTopologyNetwork topologyPhysics Letters B
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Triaxial shape with rotation around the longest principal axis inGd142

2008

The cranking model is used to describe rotational bands. We investigate the approach of using diabatic configurations and minimizing the particle-number projected energy in a mesh of both lambda, Delta and deformation parameters. We use the method to interpret recent experimental data in Gd-142 and conclude that for the highest spin states observed (I approximate to 30), the nucleus is triaxial and builds spin by rotating around the classically unfavored longest axis.

PhysicsNuclear and High Energy PhysicsClassical mechanicsSpin statesNuclear TheoryDiabaticGeometryDeformation (meteorology)Spin (physics)LambdaRotationPrincipal axis theoremPhysical Review C
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A comment on time-dependent variational-principles

1977

Two time-dependent variational principles are compared; the one varies the action integral, the other minimises the deviation from the Schrodinger-equation. They are shown to be equivalent for a variation with complex parameters, but different for a restricted variation.

PhysicsNuclear and High Energy PhysicsClassical mechanicsVariation (linguistics)Variational principleNuclear fusionElementary particleAction (physics)Zeitschrift f�r Physik A Atoms and Nuclei
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Non-Gaussian Signatures in the Lens Deformations of the CMB Sky. A New Ray-Tracing Procedure

2003

We work in the framework of an inflationary cold dark matter universe with cosmological constant, in which the cosmological inhomogeneities are considered as gravitational lenses for the CMB photons. This lensing deforms the angular distribution of the CMB maps in such a way that the induced deformations are not Gaussian. Our main goal is the estimation of the deviations with respect to Gaussianity appeared in the distribution of deformations. In the new approach used in this paper, matter is evolved with a particle-mesh N-body code and, then, an useful ray-tracing technique designed to calculate the correlations of the lens deformations induced by nonlinear structures is applied. Our appro…

PhysicsNuclear and High Energy PhysicsCold dark matterGaussianCosmic microwave backgroundAstrophysics (astro-ph)FOS: Physical sciencesCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicslaw.inventionComputational physicsRay tracing (physics)Lens (optics)Gravitationsymbols.namesakeClassical mechanicslawObservational cosmologysymbols
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THE SPACE OF STRING CONFIGURATIONS IN STRING FIELD THEORY

1990

In this paper we consider the set of maps from the interval [0, π] which constitute the argument of the functionals of a String Field Theory. We show that in order to correctly reproduce results of the dual model one has to include all square integrable functions in the functional integral, or Ω0 in terms of Sobolev spaces.

PhysicsNuclear and High Energy PhysicsCompactification (physics)FísicaAstronomy and AstrophysicsString field theoryType I string theoryRelationship between string theory and quantum field theoryAtomic and Molecular Physics and OpticsSobolev spaceNon-critical string theoryTheoretical physicsClassical mechanicsSquare-integrable functionString cosmologyInternational Journal of Modern Physics A
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Combinatorics of theSU(2)black hole entropy in loop quantum gravity

2009

We use the combinatorial and number-theoretical methods developed in previous works by the authors to study black hole entropy in the new proposal put forth by Engle, Noui, and Perez. Specifically, we give the generating functions relevant for the computation of the entropy and use them to derive its asymptotic behavior, including the value of the Immirzi parameter and the coefficient of the logarithmic correction.

PhysicsNuclear and High Energy PhysicsConfiguration entropyImmirzi parameterTheoryofComputation_GENERALLoop quantum gravityBinary entropy functionGeneral Relativity and Quantum CosmologyTheoretical physicsClassical mechanicsQuantum gravityBlack hole thermodynamicsEntropy (arrow of time)Joint quantum entropyPhysical Review D
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Mathematical Issues in a Fully-Constrained Formulation of Einstein Equations

2008

Bonazzola, Gourgoulhon, Grandcl\'ement, and Novak [Phys. Rev. D {\bf 70}, 104007 (2004)] proposed a new formulation for 3+1 numerical relativity. Einstein equations result, according to that formalism, in a coupled elliptic-hyperbolic system. We have carried out a preliminary analysis of the mathematical structure of that system, in particular focusing on the equations governing the evolution for the deviation of a conformal metric from a flat fiducial one. The choice of a Dirac's gauge for the spatial coordinates guarantees the mathematical characterization of that system as a (strongly) hyperbolic system of conservation laws. In the presence of boundaries, this characterization also depen…

PhysicsNuclear and High Energy PhysicsConservation lawPartial differential equationSpace timeMathematical analysisFOS: Physical sciencesConformal mapGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyNumerical relativityClassical mechanicsEinstein field equationsBoundary value problemMathematical structure
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Biases on cosmological parameters by general relativity effects

2012

General relativistic corrections to the galaxy power spectrum appearing at the horizon scale, if neglected, may induce biases on the measured values of the cosmological parameters. In this paper, we study the impact of general relativistic effects on non standard cosmologies such as scenarios with a time dependent dark energy equation of state, with a coupling between the dark energy and the dark matter fluids or with non-Gaussianities. We then explore whether general relativistic corrections affect future constraints on cosmological parameters in the case of a constant dark energy equation of state and of non-Gaussianities. We find that relativistic corrections on the power spectrum are no…

PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsEquation of state (cosmology)Dark matterScalar field dark matterFísicaFOS: Physical sciencesLambda-CDM modelAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesPhysical cosmologyTheoretical physicsThermodynamics of the universeClassical mechanics0103 physical sciencesDark energy010303 astronomy & astrophysicsDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
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Gravitational waves from first order phase transitions as a probe of an early matter domination era and its inverse problem

2016

We investigate the gravitational wave background from a first order phase transition in a matter-dominated universe, and show that it has a unique feature from which important information about the properties of the phase transition and thermal history of the universe can be easily extracted. Also, we discuss the inverse problem of such a gravitational wave background in view of the degeneracy among macroscopic parameters governing the signal.

PhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Gravitational-wave observatory010308 nuclear & particles physicsGravitational waveSpeed of gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Gravitational acceleration01 natural scienceslcsh:QC1-999General Relativity and Quantum CosmologyGravitational energyGravitational wave backgroundHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Classical mechanicsGravitational field0103 physical sciences010306 general physicslcsh:PhysicsAstrophysics - Cosmology and Nongalactic AstrophysicsGravitational redshiftPhysics Letters
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