Search results for "DRIVE"

showing 10 items of 543 documents

Entropy Driven Phase Separation

2006

PhysicsEntropy drivenStatistical physics
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Nonlinear energy dissipation in a cellular automaton magnetotail field model

1999

A magnetic field model of the magnetotail current sheet based on cellular automaton (CA) is presented. The present isotropic model is a continuously driven, two-dimensional running CA. The model has a physical interpretation in terms of magnetohydrodynamic (MHD) equations, and features self-organized critical (SOC) behavior with power-law scalings both in durations and sizes of instabilities (avalanches). The model has nonlinear energy dissipation, and shows avalanches with and without an external trigger. Thus the model reproduces some of the statistical features recently observed in the magnetotail.

PhysicsField (physics)MechanicsDissipationCellular automatonMagnetic fieldNonlinear systemCurrent sheetGeophysicsClassical mechanicsPhysics::Space PhysicsGeneral Earth and Planetary SciencesMagnetohydrodynamic driveMagnetohydrodynamicsGeophysical Research Letters
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A Comparison of 2D Magnetohydrodynamic Supernova Simulations with the CoCoNuT-FMT and Aenus-Alcar Codes

2021

Code comparisons are a valuable tool for the verification of supernova simulation codes and the quantification of model uncertainties. Here we present a first comparison of axisymmetric magnetohydrodynamic (MHD) supernova simulations with the CoCoNuT-FMT and Aenus-Alcar codes, which use distinct methods for treating the MHD induction equation and the neutrino transport. We run two sets of simulations of a rapidly rotating 35M gamma-ray burst progenitor model with different choices for the initial field strength, namely 10^12 G for the maximum poloidal and toroidal field in the strong-field case and 10^10 G in the weak-field case. We also investigate the influence of the Riemann solver and t…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsSupernovaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMagnetohydrodynamic driveMagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Solar and Stellar Astrophysics (astro-ph.SR)
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Time-dependent Landauer-Büttiker formula for transient dynamics

2013

We solve analyti ally the Kadano Baym equations for a nonintera ting jun tion onne ted to an arbitrary number of nonintera ting wide-band terminals. The initial equilibrium state is properly des ribed by the addition of an imaginary tra k to the time ontour. From the solution we obtain the time-dependent ele tron densities and urrents within the jun tion. The nal results are analyti expressions as a fun tion of time, and therefore no time propagation is needed either in transient or in steady-state regimes. We further present and dis uss some appli ations of the obtained formulae. peerReviewed

PhysicsHistoryCondensed Matter - Mesoscale and Nanoscale PhysicsThermodynamic equilibriumTrack (disk drive)Dynamics (mechanics)theoretical nanoscienceFunction (mathematics)ElectronCondensed Matter::Mesoscopic Systems and Quantum Hall EffectSettore FIS/03 - Fisica della MateriaComputer Science ApplicationsEducationClassical mechanicsTransient (oscillation)
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Numerical viscosity in simulations of the two-dimensional Kelvin-Helmholtz instability

2020

The Kelvin-Helmholtz instability serves as a simple, well-defined setup for assessing the accuracy of different numerical methods for solving the equations of hydrodynamics. We use it to extend our previous analysis of the convergence and the numerical dissipation in models of the propagation of waves and in the tearing-mode instability in magnetohydrodynamic models. To this end, we perform two-dimensional simulations with and without explicit physical viscosity at different resolutions. A comparison of the growth of the modes excited by our initial perturbations allows us to estimate the effective numerical viscosity of two spatial reconstruction schemes (fifth-order monotonicity preservin…

PhysicsHistoryNumerical analysisFOS: Physical sciences010103 numerical & computational mathematicsMechanicsComputational Physics (physics.comp-ph)Dissipation01 natural sciencesInstabilityComputer Science ApplicationsEducationPiecewise linear functionViscositySimple (abstract algebra)0103 physical sciencesConvergence (routing)Magnetohydrodynamic drive0101 mathematicsAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics - Computational Physics010303 astronomy & astrophysicsJournal of Physics: Conference Series
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Electron and nuclear dynamics of a molecular ion in an intense laser field

2004

The dynamics of a two-dimensional $\mathrm{H}_{2}^{+}$ molecule interacting with a strong laser pulse beyond the usual approximation of fixed nuclei is presented. The motion of the nuclei is studied by using the classical Newton laws while the electron is described with a full quantal treatment. The axis of the molecule, initially not aligned to the laser field, performs a long-period pendular motion around the laser polarization axis. Vibrational degrees of freedom are seen to be excited. The radiation emitted by the oscillating charges presents variations that are synchronous to the pendular motion. The possibility of monitoring the motion of the molecule through the emitted radiation is …

PhysicsI-2 MOLECULESField (physics)Dynamics (mechanics)Polyatomic ionALIGNING MOLECULESH-2(+)Degrees of freedom (physics and chemistry)INDUCED ALIGNMENTElectronDRIVENRadiationLaserPULSEAtomic and Molecular Physics and Opticslaw.inventionREVIVAL STRUCTURESlawExcited stateIONIZATIONAtomic physicsHARMONICSWAVE-FUNCTIONPhysical Review A
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Effect of coronal loop structure on wave heating through phase mixing

2020

Context. The mechanism(s) behind coronal heating still elude(s) direct observation and modelling of viable theoretical processes and the subsequent effect on coronal structures is one of the key tools available to assess possible heating mechanisms. Wave heating via the phase mixing of magnetohydrodynamic (MHD) transverse waves has been proposed as a possible way to convert magnetic energy into thermal energy, but MHD models increasingly suggest this is not an efficient enough mechanism. Aims. We modelled heating by phase mixing transverse MHD waves in various configurations in order to investigate whether certain circumstances can enhance the heating sufficiently to sustain the million deg…

PhysicsMagnetohydrodynamics (MHD)Magnetic energySun: corona010308 nuclear & particles physicsF300Astronomy and AstrophysicsTransverse waveAstrophysicsCoronal loopMechanicsF500Dissipation01 natural sciencesTransverse planeSpace and Planetary Science0103 physical sciencesPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamic driveBoundary value problemSun: oscillationsMagnetohydrodynamics010303 astronomy & astrophysicsSun: atmosphere
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Adiabatic eigenflows in a vertical porous channel

2014

AbstractThe existence of an infinite class of buoyant flows in a vertical porous channel with adiabatic and impermeable boundary walls, called adiabatic eigenflows, is discussed. A uniform heat source within the saturated medium is assumed, so that a stationary state is possible with a net vertical through-flow convecting away the excess heat. The simple isothermal flow with uniform velocity profile is a special adiabatic eigenflow if the power supplied by the heat source is zero. The linear stability analysis of the adiabatic eigenflows is carried out analytically. It is shown that these basic flows are unstable. The only exception, when the power supplied by the heat source is zero, is th…

PhysicsMechanical EngineeringIsothermal flowBoundary (topology)Bénard convectionMechanicsCondensed Matter PhysicsPhysics::Fluid DynamicsMechanics of MaterialsCombined forced and natural convectionconvection in porous mediaAdiabatic processbuoyancy-driven instabilityStationary stateCommunication channelRayleigh–Bénard convectionConvection cell
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Track reconstruction for theMu3eexperiment based on a novel Multiple Scattering fit

2017

The Mu3e experiment is designed to search for the lepton flavor violating decay μ + → e + e + e − . The aim of the experiment is to reach a branching ratio sensitivity of 10−16 . In a first phase the experiment will be performed at an existing beam line at the Paul-Scherrer Institute (Switzerland) providing 108 muons per second, which will allow to reach a sensitivity of 2 · 10−15 . The muons with a momentum of about 28 MeV/c are stopped and decay at rest on a target. The decay products (positrons and electrons) with energies below 53MeV are measured by a tracking detector consisting of two double layers of 50 μm thin silicon pixel sensors. The high granularity of the pixel detector with a …

PhysicsMuonPixelPhysics::Instrumentation and Detectors010308 nuclear & particles physicsScatteringBranching fractionPhysicsQC1-999Track (disk drive)DetectorPhase (waves)Tracking (particle physics)01 natural sciencesComputational physicsNuclear physics0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsEPJ Web of Conferences
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Traces of errors due to single ion in floating gate memories

2008

Single, high energy, high LET, ions impacting on a Floating gate array at grazing or near-grazing angles lead to the creation of long traces of FGs with corrupted information. Every time a FG is crossed by a single ion, it experiences a charge loss which permanently degrades the stored information. If the ion crosses more than one FG, the threshold voltage of all those FGs interested by its track will be degraded.

PhysicsNon-volatile memoryOpticsbusiness.industryGate arrayTrack (disk drive)Logic gateElectrical engineeringbusinessFlash memoryDegradation (telecommunications)IonThreshold voltage2008 IEEE International Conference on Integrated Circuit Design and Technology and Tutorial
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