Search results for "Gauss"

showing 10 items of 701 documents

Unconditional generation of bright coherent non-Gaussian light from exciton-polariton condensates

2012

Exciton-polariton condensates are considered as a deterministic source of bright, coherent non-Gaussian light. Exciton-polariton condensates emit coherent light via the photoluminescence through the microcavity mirrors due to the spontaneous formation of coherence. Unlike conventional lasers which emit coherent Gaussian light, polaritons possess a natural nonlinearity due to the interaction of the excitonic component. This produces light with a negative component to the Wigner function at steady-state operation when the phase is stabilized via a suitable method such as injection locking. In contrast to many other proposals for sources of non-Gaussian light, in our case, the light typically …

PhotonExcitonGaussianFOS: Physical sciencesPhysics::Opticslaw.inventionsymbols.namesakeOpticslawPolaritonWigner distribution functionQuantum informationCondensed Matter::Quantum GasesPhysicsQuantum PhysicsCondensed Matter::Otherbusiness.industryCondensed Matter PhysicsLaserElectronic Optical and Magnetic MaterialsQuantum Gases (cond-mat.quant-gas)symbolsQuantum Physics (quant-ph)Condensed Matter - Quantum GasesbusinessCoherence (physics)Physical Review B
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Classification of gravitational-wave glitches via dictionary learning

2018

We present a new method for the classification of transient noise signals (or glitches) in advanced gravitational-wave interferometers. The method uses learned dictionaries (a supervised machine learning algorithm) for signal denoising, and untrained dictionaries for the final sparse reconstruction and classification. We use a data set of 3000 simulated glitches of three different waveform morphologies, comprising 1000 glitches per morphology. These data are embedded in non-white Gaussian noise to simulate the background noise of advanced LIGO in its broadband configuration. Our classification method yields a 96% accuracy for a large range of initial parameters, showing that learned diction…

Physics and Astronomy (miscellaneous)Noise reductionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Data_CODINGANDINFORMATIONTHEORY01 natural sciencesGeneral Relativity and Quantum CosmologyBackground noiseTransient noisesymbols.namesake0103 physical sciencesWaveformAstrophysics::Solar and Stellar Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPattern recognitionLIGOGlitchGaussian noisesymbolsArtificial intelligenceAstrophysics - Instrumentation and Methods for Astrophysicsbusiness
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Benchmark coupled-cluster g-tensor calculations with full inclusion of the two-particle spin-orbit contributions.

2017

We present a parallel implementation to compute electron spin resonance g-tensors at the coupled-cluster singles and doubles (CCSD) level which employs the ACES III domain-specific software tools for scalable parallel programming, i.e., the super instruction architecture language and processor (SIAL and SIP), respectively. A unique feature of the present implementation is the exact (not approximated) inclusion of the five one- and two-particle contributions to the g-tensor [i.e., the mass correction, one- and two-particle paramagnetic spin-orbit, and one- and two-particle diamagnetic spin-orbit terms]. Like in a previous implementation with effective one-electron operators [J. Gauss et al.,…

Physics010304 chemical physicsbusiness.industryGaussGeneral Physics and Astronomy010402 general chemistry01 natural sciences0104 chemical sciencesTheoretical physicsSoftwareCoupled clusterClassical mechanics0103 physical sciencesScalabilityBenchmark (computing)TensorPhysical and Theoretical ChemistryOrbit (control theory)businessSecond derivativeThe Journal of chemical physics
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Discrete-Gauss states and the generation of focussing dark beams

2014

Discrete-Gauss states are a new class of gaussian solutions of the free Schr\"odinger equation owning discrete rotational symmetry. They are obtained by acting with a discrete deformation operator onto Laguerre-Gauss modes. We present a general analytical construction of these states and show the necessary and sufficient condition for them to host embedded dark beams structures. We unveil the intimate connection between discrete rotational symmetry, orbital angular momentum, and the generation of focussing dark beams. The distinguishing features of focussing dark beams are discussed. The potential applications of Discrete-Gauss states in advanced optical trapping and quantum information pro…

PhysicsAngular momentumQuantum PhysicsOperator (physics)GaussianGaussRotational symmetryFOS: Physical sciencesMathematical Physics (math-ph)Atomic and Molecular Physics and OpticsConnection (mathematics)symbols.namesakeClassical mechanicsOptical tweezersQuantum mechanicssymbolsQuantum Physics (quant-ph)Beam (structure)Mathematical PhysicsPhysics - OpticsOptics (physics.optics)
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Evidence against a glass transition in the 10-state short range Potts glass

2002

We present the results of Monte Carlo simulations of two different 10-state Potts glasses with random nearest neighbor interactions on a simple cubic lattice. In the first model the interactions come from a \pm J distribution and in the second model from a Gaussian one, and in both cases the first two moments of the distribution are chosen to be equal to J_0=-1 and Delta J=1. At low temperatures the spin autocorrelation function for the \pm J model relaxes in several steps whereas the one for the Gaussian model shows only one. In both systems the relaxation time increases like an Arrhenius law. Unlike the infinite range model, there are only very weak finite size effects and there is no evi…

PhysicsArrhenius equationStatistical Mechanics (cond-mat.stat-mech)GaussianMonte Carlo methodAutocorrelationFOS: Physical sciencesGeneral Physics and AstronomyDisordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural Networksk-nearest neighbors algorithmsymbols.namesakesymbolsStatistical physicsGlass transitionGaussian network modelCondensed Matter - Statistical MechanicsSpin-½
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Total-variation methods for gravitational-wave denoising: Performance tests on Advanced LIGO data

2018

We assess total-variation methods to denoise gravitational-wave signals in real noise conditions, by injecting numerical-relativity waveforms from core-collapse supernovae and binary black hole mergers in data from the first observing run of Advanced LIGO. This work is an extension of our previous investigation where only Gaussian noise was used. Since the quality of the results depends on the regularization parameter of the model, we perform an heuristic search for the value that produces the best results. We discuss various approaches for the selection of this parameter, either based on the optimal, mean, or multiple values, and compare the results of the denoising upon these choices. Mor…

PhysicsArtificial neural network010308 nuclear & particles physicsGravitational waveNoise reductionFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyLIGOsymbols.namesakeAstrophysics - Solar and Stellar AstrophysicsBinary black holeGaussian noiseLagrange multiplier0103 physical sciencessymbolsWaveformAstrophysics - Instrumentation and Methods for Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)AlgorithmSolar and Stellar Astrophysics (astro-ph.SR)Physical Review D
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Next-to-leading order Balitsky-Kovchegov equation beyond large Nc

2020

We calculate finite-Nc corrections to the next-to-leading order (NLO) Balitsky-Kovchegov (BK) equation. We find analytical expressions for the necessary correlators of six Wilson lines in terms of the two-point function using the Gaussian approximation. In a suitable basis, the problem reduces from the diagonalization of a six-by-six matrix to the diagonalization of a three-by-three matrix, which can easily be done analytically. We study numerically the effects of these finite-Nc corrections on the NLO BK equation. In general, we find that the finite-Nc corrections are smaller than the expected 1/Nc2∼10%. The corrections may be large for individual correlators, but have less of an influence…

PhysicsBasis (linear algebra)010308 nuclear & particles physicsFunction (mathematics)114 Physical sciences01 natural sciencesComputer Science::Digital LibrariesGaussian approximationMatrix (mathematics)DipoleAmplitude0103 physical sciencesOrder (group theory)Rapidity010306 general physicsMathematical physicsPhysical Review
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Comparison of cartesian and lobe function Gaussian basis sets

1970

The lobe function and cartesian (spherical harmonic) gaussian are compared with reference to calculations for second-row atoms. Single and grouped gaussian basis sets which have been reported for cartesian functions are taken over directly to construct corresponding lobe function bases with identical sets of exponents and with lobe separations chosen by a scaling procedure. Total and orbital energies and SCF coefficients resulting from calculations on the second-row atoms using the two types of functions for both primitive and grouped gaussian basis sets are seen to be in excellent agreement, thereby emphasizing the essential equivalence of lobe functions and cartesian gaussians, at the ver…

PhysicsBasis (linear algebra)GaussianMathematical analysisSpherical harmonicsFunction (mathematics)STO-nG basis setsLobelaw.inventionsymbols.namesakemedicine.anatomical_structurelawmedicinesymbolsCartesian coordinate systemChiropracticsPhysical and Theoretical ChemistryScalingTheoretica Chimica Acta
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Diffuse solar radiation statistics for Italy

1981

Abstract In this paper diffuse radiation is correlated with usually measured or more easy computable quantities in order to have a larger number of data available for the various applications of solar energy. Here are used two types of correlation: (a) diffuse radiation as a function of global and extraterrestrial radiation; (b) diffuse radiation as a function of ralative sunshine and extraterrestrial radiation. On the basis of the above correlations, empirical equations have been proposed and their coefficients have been calculated by fitting the experimental data of three Italian stations. The degree of accuracy of the fit has been estimated by a coefficient introduced and called by us “r…

PhysicsBasis (linear algebra)Renewable Energy Sustainability and the Environmentbusiness.industryGaussDegrees of freedom (statistics)Experimental dataFunction (mathematics)RadiationSolar energyComputational physicsTheoretical physicsGeneral Materials ScienceDegree (angle)businessSolar Energy
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Creating highly squeezed vacua in hybrid Laguerre-Gauss modes

2009

In this communication we study the above threshold quantum properties of a degenerate optical parametric oscillator (DOPO) tuned to a given transverse mode family at the signal frequency. We will show that under this configuration DOPOs are versatile sources of nonclassical light, in which one could be able to generate highly squeezed vacua with the non trivial shapes of Hybrid Laguerre-Gauss modes.

PhysicsClassical mechanicsQuantum mechanicsDegenerate energy levelsGaussOptical parametric oscillatorLaguerre polynomialsResonanceNonclassical lightQuantumTransverse mode
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