Search results for "Internal energy"

showing 10 items of 30 documents

Dynamics and Thermodynamics of Traffic Flow

2009

Application of thermodynamics to traffic flow is discussed. On a microscopic level, traffic flow is described by Bando’s optimal velocity model in terms of accelerating and decelerating forces. It allows us to introduce kinetic, potential, as well as a total energy, which is the internal energy of the car system in view of thermodynamics. The total energy is however not conserved, although it has a certain value in any of the two possible stationary states corresponding either to a fixed point or to a limit cycle solution in the space of headways and velocities.

PhysicsMicroscopic traffic flow modelInternal energyLimit cycleThermodynamicsFixed pointSpace (mathematics)Traffic flowKinetic energyStationary state
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Coulomb and nuclear excitations of narrow resonances in 17Ne

2016

Physics letters / B 759, 200 - 205 (2016). doi:10.1016/j.physletb.2016.05.073

PhysicsNuclear and High Energy PhysicsTeoría de los quantaInternal energySpins010308 nuclear & particles physicsProjectile310601 natural sciences530lcsh:QC1-999Mass formulaNuclear physics0103 physical sciencesPhysical SciencesCoulombIsobaric processFysikddc:530Atomic physics010306 general physicsMultipletExcitationlcsh:PhysicsPhysics Letters B
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Application of thermodynamics to driven systems

2007

Application of thermodynamics to driven systems is discussed. As particular examples, simple traffic flow models are considered. On a microscopic level, traffic flow is described by Bando's optimal velocity model in terms of accelerating and decelerating forces. It allows to introduce kinetic, potential, as well as total energy, which is the internal energy of the car system in view of thermodynamics. The latter is not conserved, although it has certain value in any of two possible stationary states corresponding either to fixed point or to limit cycle in the space of headways and velocities. On a mesoscopic level of description, the size n of car cluster is considered as a stochastic varia…

PhysicsPhysics - Physics and SocietyInternal energyOther Physics TopicsStatistical Mechanics (cond-mat.stat-mech)ThermodynamicsFOS: Physical sciencesDetailed balanceAnnan fysikPhysics and Society (physics.soc-ph)Condensed Matter PhysicsElectronic Optical and Magnetic MaterialsTraffic flow (computer networking)Microscopic traffic flow modelEquilibrium thermodynamicsLimit cycleMaster equationCondensed Matter - Statistical MechanicsStationary state
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Influence of Internal Energy on the Stability of Relativistic Flows

2003

A set of simulations concerning the influence of internal energy on the stability of relativistic jets is presented. Results show that perturbations saturate when the amplitude of the velocity perturbation approaches the speed of light limit. Also, contrary to what predicted by linear stability theory, jets with higher specific internal energy appear to be more stable.

PhysicsShear layerClassical mechanicsAmplitudeInternal energyAstrophysical jetLinear stability theoryLinear stability analysisAstrophysics::High Energy Astrophysical PhenomenaPerturbation (astronomy)MechanicsAstrophysicsRelativistic particle
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Probing the Internal Structure of Magnetized, Relativistic Jets with Numerical Simulations

2016

From an observational point of view, unveiling the physical processes behind the nature of the jets emanating from radio-loud AGN demands the resolution of the structure across the jet with the highest angular resolutions. Relying on a magneto-fluid dynamical description, numerical simulations can help to characterize the internal structure of jets (transversal structure, magnetic field structure, internal shocks, etc.). In the first part of the paper, we shall discuss equilibrium models of magnetized, relativistic, infinite, axisymmetric jets with rotation propagating through a homogeneous, static, unmagnetized ambient medium. Then, these transversal equilibrium profiles will be used to bu…

PhysicsShock waveJet (fluid)Internal energyMagnetic energyMHDlcsh:Astronomy010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical Phenomenagalaxies: activeAstronomy and Astrophysicsshock wavesgalaxies: jets01 natural sciencesmethods: numericalComputational physicsMagnetic fieldlcsh:QB1-991galaxies: active; galaxies: jets; methods: numerical; MHD; shock wavesRelativistic beamingClassical mechanicsAstrophysical jet0103 physical sciencesMagnetohydrodynamics010303 astronomy & astrophysicsGalaxies
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Thermodynamic pressure in nonlinear nonequilibrium thermodynamics of dilute nonviscous gases.

2000

In this paper, using extended thermodynamics, we build up a nonlinear theory for a dilute nonviscous gas under heat flux. The fundamental fields are the density, the velocity, the internal energy density, and the heat flux. The constitutive theory is builtup without approximations. We single out the nonlinear complete expressions of the Gibbs equation and of the nonequilibrium pressure. In particular, we determine the complete expressions furnished by the theory for the nonequilibrium pressure tensor and thermodynamic pressure, i.e., the derivative of the nonequilibrium internal specific entropy with respect to the specific volume, times the nonequilibrium temperature. In a second-order app…

Physicssymbols.namesakeEntropy (classical thermodynamics)Nonlinear systemInternal energyFundamental thermodynamic relationHeat fluxGibbs–Helmholtz equationsymbolsThermodynamicsNon-equilibrium thermodynamicsThermal conductionPhysical review. E, Statistical, nonlinear, and soft matter physics
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A Divergence-Free High-Resolution Code for MHD

2001

We describe a 2.5D numerical code to solve the equations of ideal magnetohydrodynamics (MHD). The numerical code, based on high-resolution shock-capturing (HRSC) techniques, solves the equations written in conservation form and computes the numerical fluxes using a linearized Riemann solver. A special procedure is used to force the conservation of magnetic flux along the time.

Physicssymbols.namesakeIdeal (set theory)Internal energyCode (cryptography)symbolsApplied mathematicsMagnetohydrodynamicsDivergence (statistics)Conservation formMagnetic fluxRiemann solver
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First-order interface localization-delocalization transition in thin Ising films using Wang-Landau sampling

2004

Using extensive Monte Carlo simulations, we study the interface localization- delocalization transition of a thin Ising film with antisymmetric competing walls for a set of parameters where the transition is strongly first-order. This is achieved by estimating the density of states (DOS) of the model by means of Wang-Landau sampling (WLS) in the space of energy, using both, single-spin-flip as well as N-fold way updates. From the DOS we calculate canonical averages related to the configurational energy, like the internal energy, the specific heat, as well as the free energy and the entropy. By sampling microcanonical averages during simulations we also compute thermodynamic quantities relat…

Statistical Mechanics (cond-mat.stat-mech)Internal energyCondensed matter physicsAntisymmetric relationMonte Carlo methodFOS: Physical sciencesMaxima and minimaDensity of statesIsing modelStatistical physicsMaximaScalingCondensed Matter - Statistical MechanicsMathematicsPhysical Review E
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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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Entropy theory and glass transition: A test by Monte Carlo simulation

1997

This article reviews the results of a test of the Gibbs-DiMarzio theory by Monte Carlo Simulation. The simulation employed the bond-fluctuation model on a simple cubic lattice. This model incorporates two kinds of interactions: the excluded volume interaction among all monomers of the melt and an internal energy of the chains, which favors large bonds and makes the chains stiffen with decreasing temperature. The stiffening of the chains leads to an increase of their volume requirements, which competes with the packing constraints at low temperatures. This competition strongly slows down the structural relaxation of the melt and induces the glassy behavior. The model therefore takes into acc…

chemistry.chemical_classificationQuantitative Biology::Biomoleculesbond-fluctuation modelMaterials scienceInternal energyMonte Carlo methodGibbs-DiMarzio theoryGeneral EngineeringThermodynamicsSimple cubic latticePolymerArticleStiffeningCondensed Matter::Soft Condensed Matterentropy measurementchemistryExcluded volumeAdam-Gibbs theoryEntropy (information theory)chemical potentialglass transitionStatistical physicsdiffusion coefficientGlass transitionMonte Carlo simulation
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