Search results for "Approx"

showing 10 items of 922 documents

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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Formation of Wigner molecules in small quantum dots

2000

It was recently argued that in small quantum dots the electrons could crystallize at much higher densities than in the infinite two-dimensional electron gas. We compare predictions that the onset of spin polarization and the formation of Wigner molecules occurs at a density parameter $r_s\approx 4 a_B^*$ to the results of a straight-forward diagonalization of the Hamiltonian matrix.

PhysicsHamiltonian matrixSpin polarizationCondensed matter physicsQuantum dotQuantum mechanicsMoleculeElectronApproxFermi gasPhysical Review B
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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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Anomalous dynamics triggered by a non-convex equation of state in relativistic flows

2017

The non-monotonicity of the local speed of sound in dense matter at baryon number densities much higher than the nuclear saturation density ($n_0 \approx 0.16\,$fm$^{-3}$) suggests the possible existence of a non-convex thermodynamics which will lead to a non-convex dynamics. Here, we explore the rich and complex dynamics that an equation of state (EoS) with non-convex regions in the pressure-density plane may develop as a result of genuinely relativistic effects, without a classical counterpart. To this end, we have introduced a phenomenological EoS, whose parameters can be restricted heeding to causality and thermodynamic stability constraints. This EoS shall be regarded as a toy-model wi…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsEquation of state (cosmology)Plane (geometry)Nuclear TheoryFluid Dynamics (physics.flu-dyn)FOS: Physical sciencesAstronomy and AstrophysicsPhysics - Fluid DynamicsApprox01 natural sciencesCausality (physics)Complex dynamicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceSpeed of sound0103 physical sciencesBaryon numberAstrophysics - High Energy Astrophysical PhenomenaRelativistic quantum chemistry010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Mathematical physics
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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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