Search results for "Thermal equilibrium"

showing 10 items of 65 documents

Quantum dynamics of the intensity-dependent Tavis-Cummings model

1999

An exactly solvable generalization of the intensity-dependent Jaynes-Cummings model to the case of N0 atoms is introduced together with its solution. The quantum dynamics of the model including the squeezing properties of the su(1,1) Perelomov and Glauber coherent states is investigated. The cases of one and two atoms present in the cavity are analysed in detail. These two cases are compared in the situation when the atomic subsystem is initially prepared in the ground state, the Dicke state and the state of thermal equilibrium.

Thermal equilibriumPhysicsGeneralizationQuantum dynamicsGeneral Physics and AstronomyStatistical and Nonlinear PhysicsQuantum PhysicsState (functional analysis)Dark stateQuantum mechanicsQuantum electrodynamicsCoherent statesGround stateGlauberMathematical PhysicsJournal of Physics A: Mathematical and General
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A quantum model of Schwarzschild black hole evaporation

1996

We construct a one-loop effective metric describing the evaporation phase of a Schwarzschild black hole in a spherically symmetric null-dust model. This is achieved by quantising the Vaidya solution and by chosing a time dependent quantum state. This state describes a black hole which is initially in thermal equilibrium and then the equilibrium is switched off, so that the black hole starts to evaporate, shrinking to a zero radius in a finite proper time. The naked singularity appears, and the Hawking flux diverges at the end-point. However, a static metric can be imposed in the future of the end-point. Although this end-state metric cannot be determined within our construction, we show tha…

Thermal equilibriumPhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaNaked singularityFOS: Physical sciencesRadiusGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum stateQuantum mechanicsMetric (mathematics)Schwarzschild metricAstronomiaProper time
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Symmetries and solvable models for evaporating 2D black holes

1997

We study the evaporation process of a 2D black hole in thermal equilibrium when the ingoing radiation is suddenly switched off. We also introduce global symmetries of generic 2D dilaton gravity models which generalize the extra symmetry of the CGHS model. © Elsevier Science B.V

Thermal equilibriumPhysicsNuclear and High Energy PhysicsGravity (chemistry)CGHS modelEvaporationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Atomic and Molecular Physics and OpticsSymmetry (physics)General Relativity and Quantum CosmologyBlack holeTheoretical physicsHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHomogeneous spaceDilaton
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Microcanonical Determination of the Interface Tension of Flat and Curved Interfaces from Monte Carlo Simulations

2012

The investigation of phase coexistence in systems with multi-component order parameters in finite systems is discussed, and as a generic example, Monte Carlo simulations of the two-dimensional q-state Potts model (q=30) on LxL square lattices (40<=L<=100) are presented. It is shown that the microcanonical ensemble is well-suited both to find the precise location of the first order phase transition and to obtain an accurate estimate for the interfacial free energy between coexisting ordered and disordered phases. For this purpose, a microcanonical version of the heatbath algorithm is implemented. The finite size behaviour of the loop in the curve describing the inverse temperature vers…

Thermal equilibriumPhysicsPhase transitionSpinodalStatistical Mechanics (cond-mat.stat-mech)CondensationMonte Carlo methodFOS: Physical sciencesCondensed Matter Physics01 natural sciences010305 fluids & plasmasMicrocanonical ensemblePhase (matter)0103 physical sciencesGeneral Materials ScienceStatistical physics010306 general physicsCondensed Matter - Statistical MechanicsPotts model
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Relativistic kinematic approach to the classical ideal gas

2019

he necessary and sufficient conditions for a unit time-like vector field to be the unit velocity of a classical ideal gas are obtained. In a recent paper [Coll, Ferrando and S\'aez, Phys. Rev D {\bf 99} (2019)] we have offered a purely hydrodynamic description of a classical ideal gas. Here we take one more step in reducing the number of variables necessary to characterize these media by showing that a plainly kinematic description can be obtained. We apply the results to obtain test solutions to the hydrodynamic equation that model the evolution in local thermal equilibrium of a classical ideal gas. \end{abstract}

Thermal equilibriumPhysicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsMathematical analysisFOS: Physical sciencesKinematicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyIdeal gas0103 physical sciencesVector field010306 general physicsUnit (ring theory)
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Thermodynamic class II Szekeres-Szafron solutions. Singular models

2019

A family of parabolic Szekeres-Szafron class II solutions in local thermal equilibrium is studied and their associated thermodynamics are obtained. The subfamily with the hydrodynamic behavior of a generic ideal gas (defined by the equation of state $p = k n \Theta$) results to be an inhomogeneous generalization of flat FLRW $\gamma$-law models. Three significative interpretations that follow on from the choice of three specific thermodynamic schemes are analyzed in depth. First, the generic ideal gas in local thermal equilibrium; this interpretation leads to an inhomogeneous temperature $\Theta$. Second, the thermodynamics with homogeneous temperature considered by Lima and Tiomno (CQG 6 1…

Thermal equilibriumPhysicsPhysics and Astronomy (miscellaneous)Spacetime010308 nuclear & particles physicsEquation of state (cosmology)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesIdeal gasGeneral Relativity and Quantum CosmologyInterpretation (model theory)symbols.namesakeFriedmann–Lemaître–Robertson–Walker metric0103 physical sciencesCompressibilitysymbolsLimit (mathematics)010306 general physicsMathematical physics
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Local thermal equilibrium and ideal gas Stephani universes

2005

The Stephani universes that can be interpreted as an ideal gas evolving in local thermal equilibrium are determined. Five classes of thermodynamic schemes are admissible, which give rise to five classes of regular models and three classes of singular models. No Stephani universes exist representing an exact solution to a classical ideal gas (one for which the internal energy is proportional to the temperature). But some Stephani universes may approximate a classical ideal gas at first order in the temperature: all of them are obtained. Finally, some features about the physical behavior of the models are pointed out.

Thermal equilibriumPhysicsTheoretical physicsExact solutions in general relativityPhysics and Astronomy (miscellaneous)Internal energyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]First orderIdeal gasGeneral Relativity and Quantum Cosmology
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Computer Simulation Studies of Chain Dynamics in Polymer Brushes

2012

Center-of-mass and single monomer motion in grafted chains comprising a strongly stretched polymer brush in thermal equilibrium are studied by large scale molecular dynamics and Monte Carlo simulations of a coarse-grained model. Good solvent conditions are assumed. Our findings seriously question earlier theoretical predictions about the relaxation described by Rouse dynamics of brush coatings. Thus, the correlation functions of parallel and perpendicular components of the mean distance of the center-of-mass from the grafting site, the squared gyration radius and end-to-end distance, are found to deviate strongly from a simple exponential decay. While the relaxation times extracted from the…

Thermal equilibriumQuantitative Biology::BiomoleculesPolymers and PlasticsChemistryOrganic ChemistryMonte Carlo methodThermodynamicsRadiusPolymer brushGyrationCondensed Matter::Soft Condensed MatterInorganic ChemistryMolecular dynamicsComputational chemistryMaterials ChemistryRelaxation (physics)Exponential decayMacromolecules
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Transition probabilities for some infrared O I spectral lines—Application for determining excitation temperatures in low temperature plasmas

2008

Intensities of selected spectral transitions of neutral oxygen emitted from a wall-stabilized arc have been measured. Applying reliable transition probability data taken from literature, Boltzmann plots have been constructed and the temperatures of the plasma have been obtained. At arc plasma conditions ensuring partial local thermal equilibrium, transition probabilities for 4 O I spectral lines from the near infrared spectral range have been obtained. These new results, together with data for two other studied O I spectral lines taken from the National Institute of Standards and Technology data base, are proposed as a suitable set of transition probabilities applicable for diagnostics of l…

Thermal equilibriumRange (particle radiation)ChemistryInfraredNear-infrared spectroscopyPlasmaAtomic and Molecular Physics and OpticsSpectral lineAnalytical Chemistrysymbols.namesakeBoltzmann constantsymbolsAtomic physicsInstrumentationSpectroscopyExcitationSpectrochimica Acta Part B: Atomic Spectroscopy
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Quantitative interpretation of the red edge excitation (REE) effect of 9,9′-bianthryl in polyisobutene by band shape analysis of the temperature-depe…

1994

Optical fluorescence spectra of 9,9′-bianthryl (BA) in polyisobutene (PIB) were measured as a function of the excitation wavelength at various temperatures between 210 and 293 K. Irradiation at the red edge of the absorption spectra selectively excites distinct conformers with respect to the torsional angle. This leads to a strong dependence of the vibronic band shape of the fluorescence spectra on the excitation wavelength. The marked temperature dependence of the band shape may be attributed to the viscosity-dependent deceleration of the torsional relaxation of BA in the highly viscous polymer which prevents the excited state ensemble from reaching thermal equilibrium. The predominant bro…

Thermal equilibriumSmoluchowski coagulation equationAbsorption spectroscopyChemistryGeneral Chemical EngineeringRelaxation (NMR)Analytical chemistryMolecular physicsSpectral lineFluorescence spectroscopysymbols.namesakeExcited statesymbolsExcitationBerichte der Bunsengesellschaft für physikalische Chemie
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