Search results for "APPROXIMATION"

showing 10 items of 818 documents

Gaussian imaging transformation for the paraxial Debye formulation of the focal region in a low-Fresnel-number optical system

2000

The Debye formulation of focused fields has been systematically used to evaluate, for example, the point-spread function of an optical imaging system. According to this approximation, the focal wave field exhibits some symmetries about the geometrical focus. However, certain discrepancies arise when the Fresnel number, as viewed from focus, is close to unity. In that case, we should use the Kirchhoff formulation to evaluate accurately the three-dimensional amplitude distribution of the field in the focal region. We make some important remarks regarding both diffraction theories. In the end we demonstrate that, in the paraxial regime, given a defocused transverse pattern in the Debye approxi…

PhysicsFresnel zonePlane (geometry)business.industryParaxial approximationAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic Materialssymbols.namesakeCardinal pointClassical mechanicsOpticsThin lenssymbolsFresnel numberComputer Vision and Pattern RecognitionFocus (optics)businessDebyeJournal of the Optical Society of America. A, Optics, image science, and vision
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GW quasiparticle energies of atoms in strong magnetic fields

2019

Quasiparticle energies of the atoms H–Ne have been computed in the GW approximation in the presence of strong magnetic fields with field strengths varying from 0 to 0.25 atomic units (0.25 B 0 =0.25 ℏe −1 a −2 0 ≈58 763 0.25 B0=0.25 ℏe−1a0−2≈58 763 T). The GW quasiparticle energies are compared with equation-of-motion ionization-potential (EOM-IP) coupled-cluster singles-and-doubles (CCSD) calculations of the first ionization energies. The best results are obtained with the evGW@PBE0 method, which agrees with the EOM-IP-CCSD model to within about 0.20 eV. Ionization potentials have been calculated for all atoms in the series, representing the first systematic study of ionization potentials …

PhysicsGW approximation010304 chemical physicsField (physics)General Physics and AstronomyField strengthElectron010402 general chemistry01 natural sciences7. Clean energy0104 chemical sciencesMagnetic fieldIonization0103 physical sciencesPhysics::Atomic and Molecular ClustersQuasiparticlePhysics::Atomic PhysicsPhysical and Theoretical ChemistryAtomic physicsIonization energyThe Journal of Chemical Physics
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MBPT for the Green's function

2013

PhysicsGW approximationsymbols.namesakeSelf-energyPolarizabilityQuantum mechanicsMany-body theorysymbolsNon-equilibrium thermodynamicsFeynman diagramTopological conjugacyQuantum
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Theory of vibrational anomalies in glasses

2015

Abstract The theory of elasticity with spatially fluctuating elastic constants (heterogeneous-elasticity theory) is reviewed. It is shown that the vibrational anomalies associated with the boson peak can be qualitatively and quantitatively explained in terms of this theory. Two versions of a mean-field theory for solving the stochastic equation of motion are presented: the coherent-potential approximation (CPA) and the self-consistent Born approximation (SCBA). It is shown that the latter is included in the former in the Gaussian and weak-disorder limit. We are able to discuss and explain cases in which the change of the vibrational spectrum by varying an external parameter can be accounted…

PhysicsGaussianCondensed Matter Physics; ceramics and composites; electronic optical and magnetic materials; Materials Chemistry; metals and alloysEquations of motionVibrational spectrumCondensed Matter PhysicsDebye frequencyElectronic Optical and Magnetic Materialssymbols.namesakeQuantum mechanicsMaterials ChemistryCeramics and CompositessymbolsBoson peakElasticity (economics)Born approximationElastic modulus
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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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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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Focal-shift formula in apodized nontelecentric focusing systems

2007

A single analytical formulation for evaluating the focal shift in any apodized nontelecentric focusing setup is reported. The formulation is also useful in the case of imaged paraxial beams. We show explicitly that the magnitude of the focal shift is determined by only one parameter that depends on the effective width of the pupil filter and its axial position. To illustrate our approach we examine different focusing setups.

PhysicsGeometrical opticsbusiness.industryParaxial approximationAstrophysics::Instrumentation and Methods for AstrophysicsFilter (signal processing)Atomic and Molecular Physics and OpticsOpticsApodizationPosition (vector)Systems designFresnel numberbusinessFresnel diffractionOptics Letters
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Correlation and spin polarization in quantum dots: Local spin density functional theory revisited

2005

Using quantum dot artificial atoms as a simple toy model, we reflect on the question of whether spin density functional theory (SDFT) can accurately describe correlation effects in low-dimensional fermion systems. Different expressions for the local density approximation of the exchange-correlation energy for the two-dimensional electron gas, such as the much-used functional of Tanatar and Ceperley, and the recent suggestion by Attaccalite et al., are compared with the results of a numerical diagonalization of the many-body Hamiltonian matrix in the limit of small electron numbers. For systems with degeneracies, as shown in the present work for the example of a spin triplet with S = 1, the …

PhysicsHamiltonian matrixToy modelSpin polarizationCondensed matter physicsConfiguration interactionCondensed Matter PhysicsAtomic and Molecular Physics and OpticsQuantum mechanicsPhysical and Theoretical ChemistryLocal-density approximationFermi gasMultipletSpin-½International Journal of Quantum Chemistry
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Late time approach to Hawking radiation: Terms beyond leading order

2019

Black hole evaporation is studied using wave packets for the modes. These allow for approximate frequency and time resolution. The leading order late time behavior gives the well known Hawking radiation that is independent of how the black hole formed. The focus here is on the higher order terms and the rate at which they damp at late times. Some of these terms carry information about how the black hole formed. A general argument is given which shows that the damping is significantly slower (power law) than what might be naively expected from a stationary phase approximation (exponential). This result is verified by numerical calculations in the cases of 2D and 4D black holes that form from…

PhysicsHigh Energy Physics - Theory010308 nuclear & particles physicsWave packetAstrophysics::High Energy Astrophysical PhenomenaShell (structure)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesNull (physics)Power lawGeneral Relativity and Quantum CosmologyExponential functionBlack holeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum electrodynamics0103 physical sciencesStationary phase approximation010306 general physicsHawking radiation
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Super Heavy Dark Matter Anisotropies from D-particles in the Early Universe

2004

We discuss a way of producing anisotropies in the spectrum of superheavy Dark matter, which are due to the distortion of the inflationary space time induced by the recoil of D-particles upon their scattering with ordinary string matter in the Early Universe. We calculate such distortions by world-sheet Liouville string theory (perturbative) methods. The resulting anisotropies are found to be proportional to the average recoil velocity and density of the D-particles. In our analysis we employ a regulated version of de Sitter space, allowing for graceful exit from inflation. This guarantees the asymptotic flatness of the space time, as required for a consistent interpretation, within an effec…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsDe Sitter spaceSpace timeDark matterAstrophysics (astro-ph)FísicaFOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)String theoryAstrophysicsAtomic and Molecular Physics and OpticsGraceful exitWKB approximationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum electrodynamicsEffective field theoryFlatness (cosmology)
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