Search results for "quantum electrodynamics"

showing 10 items of 809 documents

Finding Electron-Hole Interaction in Quantum Kinetic Framework

2018

The present research has been supported by the Institute of Solid State Physics, the University of Latvia within the framework of National Research Program IMIS2. [Grant numbers VPPI IMIS2, IMIS4].

PhysicsHilbert spaces010308 nuclear & particles physicsPhysicsQC1-999General EngineeringHilbert spaceGeneral Physics and AstronomyElectron holeKinetic energy01 natural sciencessymbols.namesakeQuantum mechanics0103 physical sciencessymbols:NATURAL SCIENCES:Physics [Research Subject Categories]quantum electrodynamicsphotoexcited electron-hole pairhilbert spaces010306 general physicsQuantumLatvian Journal of Physics and Technical Sciences
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Kadanoff-Baym approach to time-dependent quantum transport in AC and DC fields

2010

We have developed a method based on the embedded Kadanoff-Baym equations to study the time evolution of open and inhomogeneous systems. The equation of motion for the Green's function on the Keldysh contour is solved using different conserving many-body approximations for the self-energy. Our formulation incorporates basic conservation laws, such as particle conservation, and includes both initial correlations and initial embedding effects, without restrictions on the time-dependence of the external driving field. We present results for the time-dependent density, current and dipole moment for a correlated tight binding chain connected to one-dimensional non-interacting leads exposed to DC …

PhysicsHistoryConservation lawCondensed Matter - Mesoscale and Nanoscale PhysicsField (physics)Time evolutionFOS: Physical sciencesEquations of motionSettore FIS/03 - Fisica della MateriaComputer Science ApplicationsEducationMoment (mathematics)DipoleHarmonicsQuantum electrodynamicsMesoscale and Nanoscale Physics (cond-mat.mes-hall)HarmonicJournal of Physics: Conference Series
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Relativistic MHD simulations of stellar core collapse and magnetars

2011

We present results from simulations of magneto-rotational stellar core collapse along with Alfven oscillations in magnetars. These simulations are performed with the CoCoA/CoCoNuT code, which is able to handle ideal MHD flows in dynamical spacetimes in general relativity. Our core collapse simulations highlight the importance of genuine magnetic effects, like the magneto-rotational instability, for the dynamics of the flow. For the modelling of magnetars we use the anelastic approximation to general relativistic MHD, which allows for an effective suppression of fluid modes and an accurate description of Alfven waves. We further compute Alfven oscillation frequencies along individual magneti…

PhysicsHistoryOscillationGeneral relativityCollapse (topology)MagnetarInstabilityComputer Science ApplicationsEducationMagnetic fieldClassical mechanicsHarmonicsQuantum electrodynamicsMagnetohydrodynamicsJournal of Physics: Conference Series
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From led light signboards to the Planck’s constant

2018

Recent studies have highlighted an alarming decline in young people’s interest towards the study of scientific subjects, often considered interesting but not easily understood and appreciated by students. In particular, the introduction of Modern Physics (MP) key-topics at secondary school level is a difficult and complex task because MP involves abstract ideas and requires a strong mathematical background. In this communication we present and discuss the results of an inquiry-based teaching/learning path aimed at surmounting the difficulties of an exclusively theoretical approach to the introduction of MP topics. In particular, we planned and realized an inquiry-driven learning environment…

PhysicsHistorysymbols.namesakeQuantum electrodynamicsSettore FIS/08 - Didattica E Storia Della FisicasymbolsModern Physics teaching Laboratory Inquiry-based approach Critical thinkingPlanckConstant (mathematics)Settore FIS/03 - Fisica Della MateriaSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Computer Science ApplicationsEducation
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Application of the Density Matrix Renormalization Group in momentum space

2001

We investigate the application of the Density Matrix Renormalization Group (DMRG) to the Hubbard model in momentum-space. We treat the one-dimensional models with dispersion relations corresponding to nearest-neighbor hopping and $1/r$ hopping and the two-dimensional model with isotropic nearest-neighbor hopping. By comparing with the exact solutions for both one-dimensional models and with exact diagonalization in two dimensions, we first investigate the convergence of the ground-state energy. We find variational convergence of the energy with the number of states kept for all models and parameter sets. In contrast to the real-space algorithm, the accuracy becomes rapidly worse with increa…

PhysicsHubbard modelStrongly Correlated Electrons (cond-mat.str-el)Density matrix renormalization groupExtrapolationFOS: Physical sciencesPosition and momentum spaceSpinonCondensed Matter - Strongly Correlated ElectronsDistribution functionQuantum electrodynamicsDispersion relationCondensed Matter::Strongly Correlated ElectronsStatistical physicsCurse of dimensionality
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Non-linear axisymmetric pulsations of rotating relativistic stars in the conformal flatness approximation

2005

We study non-linear axisymmetric pulsations of rotating relativistic stars using a general relativistic hydrodynamics code under the assumption of a conformal flatness. We compare our results to previous simulations where the spacetime dynamics was neglected. The pulsations are studied along various sequences of both uniformly and differentially rotating relativistic polytropes with index N = 1. We identify several modes, including the lowest-order l = 0, 2, and 4 axisymmetric modes, as well as several axisymmetric inertial modes. Differential rotation significantly lowers mode frequencies, increasing prospects for detection by current gravitational wave interferometers. We observe an exten…

PhysicsInertial frame of referenceGravitational waveFlatness (systems theory)Astrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsConformal mapAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)RotationAstrophysicsAsteroseismologyGeneral Relativity and Quantum CosmologySpace and Planetary ScienceHarmonicsQuantum electrodynamicsDifferential rotationAstrophysics::Solar and Stellar Astrophysics
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On the renormalization of ultraviolet divergences in the inflationary angular power spectrum

2015

We revise the role of ultraviolet divergences of cosmological observables and the corresponding renormalization from a space-time perspective. We employ the two-point function of primordial perturbations generated during inflation to derive an analytic expression for the multipole coefficients Cl in the Sachs-Wolfe regime. We analyzethe ultraviolet behaviorand stress the fact that the standard result in the literature is equivalent to a renormalization of the two-point function at zeroth adiabatic order. We also argue that renormalization at second adiabatic order seems to be more appropriate from a physical point of view. This may change significantly the predictions for Cl, while maintain…

PhysicsInflation (cosmology)HistoryObservableAstrophysics::Cosmology and Extragalactic AstrophysicsFunction (mathematics)Scale invarianceComputer Science ApplicationsEducationRenormalizationZeroth law of thermodynamicsQuantum electrodynamicsMultipole expansionAdiabatic processJournal of Physics: Conference Series
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Resummation of anisotropic quartic oscillator. Crossover from anisotropic to isotropic large-order behavior

1996

We present an approximative calculation of the ground-state energy for the anisotropic anharmonic oscillator Using an instanton solution of the isotropic action $\delta = 0$, we obtain the imaginary part of the ground-state energy for small negative $g$ as a series expansion in the anisotropy parameter $\delta$. From this, the large-order behavior of the $g$-expansions accompanying each power of $\delta$ are obtained by means of a dispersion relation in $g$. These $g$-expansions are summed by a Borel transformation, yielding an approximation to the ground-state energy for the region near the isotropic limit. This approximation is found to be excellent in a rather wide region of $\delta$ aro…

PhysicsInstantonQuantum PhysicsIsotropyFOS: Physical sciencesAtomic and Molecular Physics and OpticsQuartic functionDispersion relationQuantum electrodynamicsLimit (mathematics)ResummationAnisotropySeries expansionQuantum Physics (quant-ph)
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Resonant Kelvin-Helmholtz modes in sheared relativistic flows

2007

Qualitatively new aspects of the (linear and non-linear) stability of sheared relativistic (slab) jets are analyzed. The linear problem has been solved for a wide range of jet models well inside the ultrarelativistic domain (flow Lorentz factors up to 20; specific internal energies $\approx 60c^2$). As a distinct feature of our work, we have combined the analytical linear approach with high-resolution relativistic hydrodynamical simulations, which has allowed us i) to identify, in the linear regime, resonant modes specific to the relativistic shear layer ii) to confirm the result of the linear analysis with numerical simulations and, iii) more interestingly, to follow the instability develo…

PhysicsJet (fluid)Field (physics)Lorentz transformationNumerical analysisAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesLinear regimePerturbation (astronomy)MechanicsAstrophysicsInstabilityLorentz factorNonlinear systemsymbols.namesakeClassical mechanicsAstrophysical jetQuantum mechanicsQuantum electrodynamicsHelmholtz free energysymbolsLinear growthBackground flow
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Effective Field Theory for Jet Processes

2015

Processes involving narrow jets receive perturbative corrections enhanced by logarithms of the jet opening angle and the ratio of the energies inside and outside the jets. Analyzing cone-jet processes in effective field theory, we find that in addition to soft and collinear fields their description requires degrees of freedom which are simultaneously soft and collinear to the jets. These collinear-soft particles can resolve individual collinear partons, leading to a complicated multi-Wilson-line structure of the associated operators at higher orders. Our effective field theory provides, for the first time, a factorization formula for a cone-jet process, which fully separates the physics at …

PhysicsJet (fluid)Wilson loop010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaDegrees of freedom (physics and chemistry)FOS: Physical sciencesGeneral Physics and AstronomyPartonRenormalization group01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)FactorizationQuantum electrodynamics0103 physical sciencesEffective field theoryHigh Energy Physics::ExperimentResummation010306 general physicsPhysical Review Letters
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