Search results for " Rotation"

showing 10 items of 278 documents

Light-induced polarization effects in atoms with partially resolved hyperfine structure and applications to absorption, fluorescence, and nonlinear m…

2009

The creation and detection of atomic polarization is examined theoretically, through the study of basic optical-pumping mechanisms and absorption and fluorescence measurements, and the dependence of these processes on the size of ground- and excited-state hyperfine splittings is determined. The consequences of this dependence are studied in more detail for the case of nonlinear magneto-optical rotation in the Faraday geometry (an effect requiring the creation and detection of rank-two polarization in the ground state) with alkali atoms. Analytic formulas for the optical rotation signal under various experimental conditions are presented.

PhysicsAtomic Physics (physics.atom-ph)FOS: Physical sciencesPolarization (waves)FluorescenceAtomic and Molecular Physics and Opticslaw.inventionPhysics - Atomic PhysicsNonlinear systemlawLight inducedPhysics::Atomic PhysicsOptical rotationAtomic physicsFaraday cageGround stateHyperfine structure
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Surface Plasmon Platform for Angle-Resolved Chiral Sensing

2019

Chiral sensitive techniques have been used to probe the fundamental symmetries of the universe, study biomolecular structures, and even develop safe drugs. As chiral signals are inherently weak and...

PhysicsCircular dichroismHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologySurface plasmon02 engineering and technology021001 nanoscience & nanotechnology01 natural sciencesMolecular physicsAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic Materials010309 optics0103 physical sciencesElectrical and Electronic EngineeringThin filmSurface plasmon resonanceOptical rotation0210 nano-technologyChirality (chemistry)BiotechnologyACS Photonics
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Low-frequency internal waves in magnetized rotating stellar radiation zones

2012

Context. With the progress of observational constraints on dynamical processes in stars, it becomes necessary to understand the angular momentum and the rotation profile history. In this context, internal waves constitute an efficient transport mechanism over long distances in stellar radiation zones. Indeed, they could be one of the mechanisms responsible for the quasi-flat rotation profile of the solar radiative region up to 0.2 R ⊙ .Aims. Angular momentum transport induced by internal waves depends on the properties of their excitation regions and of their dissipation during propagation. Then, the bottom of convective envelopes (the top of convective cores, respectively) are differential…

PhysicsConvectionAngular momentumAstronomy and AstrophysicsAstrophysicsInternal wave01 natural sciences010305 fluids & plasmasMagnetic fieldsymbols.namesakeClassical mechanicsSpace and Planetary ScienceQuantum electrodynamics0103 physical sciencesAngular momentum of lightsymbolsRadiative transferDifferential rotation010303 astronomy & astrophysicsLorentz forceAstronomy & Astrophysics
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Origin invariant calculation of optical rotation without recourse to London orbitals

2004

We propose an inherently origin invariant formulation of specific optical rotation obtained from the conventional velocity gauge expression by subtracting the static limit from the electric dipole-magnetic dipole polarizability: 〈〈p→,L→〉〉ω→〈〈p→,L→〉〉ω-〈〈p→,L→〉〉0. London (gauge including) atomic orbitals are therefore not needed to ensure origin invariance and, consequently, this modified velocity gauge formulation may be employed in conjunction with variational and non-variational quantum chemical methods alike. Sample calculations on S-propylene oxide and 3,4- methylenedioxymethamphetamine using self-consistent field and coupled cluster wave functions…

PhysicsDipolePhysics and Astronomy (all)Coupled clusterAtomic orbitalPolarizabilityQuantum mechanicsGeneral Physics and AstronomyOptical rotationInvariant (physics)Physical and Theoretical ChemistryWave functionBasis set
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A First Assessment of the Corrections for the Consistency of the IAU2000 and IAU2006 Precession-Nutation Models

2020

The Earth precession-nutation model endorsed by resolutions of each the International Astronomical Union and the International Union of Geodesy and Geophysics is composed of two theories developed independently, namely IAU2006 precession and IAU2000A nutation. The IAU2006 precession was adopted to supersede the precession part of the IAU 2000A precession-nutation model and tried to get the new precession theory dynamically consistent with the IAU2000A nutation. However, full consistency was not reached, and slight adjustments of the IAU2000A nutation amplitudes at the micro arcsecond level were required to ensure consistency. The first set of formulae for these corrections derived by Capita…

PhysicsEarth rotation theoryEarth Orientation ParametersEarth rotation modelsConsistency (statistics)NutationPrecessionMatemática AplicadaEarth orientation parametersGeodesyPrecession-nutation
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The master two-loop two-point function. The general case

1991

Abstract We present a new calculation of the two-loop two-point function. Avoiding standard techniques such as Feynman parametrization and Wick rotation we end up with a simple double integral representation valid for arbitrary mass-cases. Numerical and analytical checks confirm our result.

PhysicsFeynman parametrizationNuclear and High Energy PhysicsRegularization (physics)Multiple integralWick rotationApplied mathematicsPropagatorPoint functionPhysics Letters B
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ONE-LOOP INTEGRALS REVISITED — THE THREE-POINT FUNCTIONS

1993

This paper presents results concerning a new calculation of the well-known one-loop n- point scalar and tensor functions. In this paper we treat the three-point functions. We give a systematic reduction to a certain class of functions which minimizes the effort for calculating scalar and tensor integrals drastically. We avoid standard techniques such as Feynman parametrization and Wick rotation.

PhysicsFeynman parametrizationNuclear and High Energy PhysicsWick rotationScalar (mathematics)Applied mathematicsAstronomy and AstrophysicsAtomic and Molecular Physics and OpticsInternational Journal of Modern Physics A
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THREE-DIMENSIONAL RELATIVISTIC SIMULATIONS OF ROTATING NEUTRON-STAR COLLAPSE TO A KERR BLACK HOLE

2006

We present a new three-dimensional fully general-relativistic hydrodynamics code using high-resolution shock-capturing techniques and a conformal traceless formulation of the Einstein equations. Besides presenting a thorough set of tests which the code passes with very high accuracy, we discuss its application to the study of the gravitational collapse of uniformly rotating neutron stars to Kerr black holes. The initial stellar models are modeled as relativistic polytropes which are either secularly or dynamically unstable and with angular velocities which range from slow rotation to the mass-shedding limit. We investigate the gravitational collapse by carefully studying not only the dynami…

PhysicsGeneral Relativity and Quantum CosmologyAngular momentumNeutron starClassical mechanicsDynamical horizonRotating black holeEvent horizonAstrophysics::High Energy Astrophysical PhenomenaApparent horizonGravitational collapseDifferential rotation
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Stability of the intrinsic energy vanishing in the Schwarzschild metric under a slow rotation

2014

The linearized Kerr metric is considered and put in some Gauss coordinates which are further {\em intrinsic} ones. The linear and angular 4-momenta of this metric are calculated in these coordinates and the resulting value is just zero. Thus, the global vanishing previously found for the Schwarzschild metric remains linearly stable under slow rotational perturbations of this metric.

PhysicsGravitacióPhysics and Astronomy (miscellaneous)GaussKerr metricZero (complex analysis)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Stability (probability)General Relativity and Quantum CosmologySlow rotationRelativitat general (Física)Metric (mathematics)Schwarzschild metricEnergy (signal processing)Mathematical physicsGeneral Relativity and Gravitation
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AMR simulations of the low bar-mode instability of neutron stars

2007

It has been recently argued through numerical work that rotating stars with a high degree of differential rotation are dynamically unstable against bar-mode deformation, even for values of the ratio of rotational kinetic energy to gravitational potential energy as low as O(0.01). This may have implications for gravitational wave astronomy in high-frequency sources such as core collapse supernovae. In this paper we present high-resolution simulations, performed with an adaptive mesh refinement hydrodynamics code, of such low T/|W| bar-mode instability. The complex morphological features involved in the nonlinear dynamics of the instability are revealed in our simulations, which show that the…

PhysicsGravitational waveAstrophysics (astro-ph)FOS: Physical sciencesGeneral Physics and AstronomyAstrophysicsAstrophysicsPotential energyInstabilityGravitational-wave astronomyRotational energyComputational physicsStarsNeutron starHardware and ArchitectureDifferential rotationComputer Physics Communications
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