Search results for "Field strength"

showing 10 items of 42 documents

First Versus Second Order Phase Transitions in the Three-Dimensional Three-State Potts Model in Random Fields

1995

The ordering of three-states Potts ferromagnets on the simple cubic lattice exposed to random fields is investigated by extensive Monte Carlo simulations. Evidence is presented that the transition is second order for intermediate strength of the fields, while it presumably is first order for large field strength. The implications for various theoretical predictions are briefly discussed.

PhysicsPhase transitionRandom fieldFerromagnetismTricritical pointMonte Carlo methodOrder (group theory)Field strengthStatistical physicsPotts model
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Carrier localization effect in polarized InGaN multiple quantum wells

2005

Carrier localization effects in polarized InGaN/GaN multiple quantum wells (MQWs) were investigated as a function of well width, d, and In content, x. Using photoreflectance (PR), photoluminescence (PL), PL excitation (PLE), selective excitation of PL, PL excitation power, and time-resolved PL spectroscopy, the dominance of the localization effect against the built-in field effect on carrier recombination dynamics in InxGa1–xN MQWs of different well width (d = 2.0–4.0 nm, x ≈ 0.15) and In content (x ≈ 0.22–0.27, d = 2.5 nm) was revealed. Based on the modeling of the PL spectra by Monte Carlo simulation of exciton hopping and the spectroscopic reference provided by PR, increased In content a…

PhysicsPhotoluminescenceCondensed matter physicsExcitonMultiple quantumMonte Carlo methodField effectField strengthMolecular physicsExcitationRecombinationphysica status solidi (c)
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FULLY RESOLVED QUIET-SUN MAGNETIC FLUX TUBE OBSERVED WITH THE SUNRISE/IMAX INSTRUMENT

2010

Until today, the small size of magnetic elements in quiet Sun areas has required the application of indirect methods, such as the line-ratio technique or multi-component inversions, to infer their physical properties. A consistent match to the observed Stokes profiles could only be obtained by introducing a magnetic filling factor that specifies the fraction of the observed pixel filled with magnetic field. Here, we investigate the properties of a small magnetic patch in the quiet Sun observed with the IMaX magnetograph on board the balloon-borne telescope Sunrise with unprecedented spatial resolution and low instrumental stray light. We apply an inversion technique based on the numerical s…

PhysicsPhotosphereFlux tubeStray lightFOS: Physical sciencesAstronomy and AstrophysicsField strengthAstrophysicsMagnetic fluxMagnetic fieldAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceRadiative transferAstrophysics::Solar and Stellar AstrophysicsSunriseSolar and Stellar Astrophysics (astro-ph.SR)The Astrophysical Journal
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NON-LINEAR MECHANICAL, ELECTRICAL AND THERMAL PHENOMENA IN PIEZOELECTRIC CRYSTALS

2003

Mechanical, electrical and thermal phenomena occurring in piezoelectric crystals were examined by non-linear approximation. For this purpose, use was made of the thermodynamic function of state, which describes an anisotropic body. Considered was the Gibbs function. The calculations included strain tensor εij = f(σkl , En, T), induction vector Dm = f(σkl , En, T) and entropy S = f(σkl , En, T) as function of stress σkl , field strength En and temperature difference T. The equations obtained apply to anisotropic piezoelectric bodies provided that the “forces” σkl , En, T acting on the crystal are known. Механічні, електричні та термічні явища у п’єзоелектричних кристалах вивчаються у неліній…

PhysicsPhysics and Astronomy (miscellaneous)Condensed matter physicsInfinitesimal strain theorypiezoelectric crystalsField strengthCondensed Matter PhysicsPiezoelectricitylcsh:QC1-999Gibbs free energyCrystalthermodynamicssymbols.namesakeNonlinear systemtensorsThermalsymbolsAnisotropylcsh:Physicsanisotropic bodiesCondensed Matter Physics
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Three-dimensional dynamics of a particle with a finite energy of magnetic anisotropy in a rotating magnetic field.

2013

A model of a single ferromagnetic particle with a finite coupling energy of the magnetic moment with the body of the particle is formulated, and regimes of its motion in a rotating magnetic field are investigated. Regimes are possible that are synchronous and asynchronous with the field. In a synchronous regime the easy axis of the particle is in the plane of the rotating magnetic field at low frequencies (a planar regime) and on the cone at high frequencies (a precession regime). The stability of these regimes is investigated, and it is shown that the precession regime is stable for field strengths below the critical value. In a particular range of field strength value, irreversible jumps …

PhysicsRotating magnetic fieldMagnetic anisotropyNuclear magnetic resonanceCondensed matter physicsMagnetic energyDemagnetizing fieldField strengthMagnetic pressureMagnetic dipoleMagnetosphere particle motionPhysical review. E, Statistical, nonlinear, and soft matter physics
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AC Stark shift of the ground state of atomic hydrogen

2004

An analytical expression for the second-order AC Stark shift of the ground state of atomic hydrogen is derived, which is convergent for negative as well as for positive energies of intermediate states except for the resonances. To clarify the applicability of the second-order perturbation theory, we compared results with those which are obtained by us and other authors using nonperturbative methods. It appears that values obtained for the AC Stark shift using our simple formula agree on average with Floquet-method calculations up to the field strength F=0.12 (a.u.), which corresponds to I=1015 W/cm2.

PhysicsSecond order theoryQuantum opticsPhysics and Astronomy (miscellaneous)Condensed matter physicsHydrogenGeneral EngineeringGeneral Physics and Astronomychemistry.chemical_elementField strengthsymbols.namesakeStark effectchemistrysymbolsIntermediate statePhysics::Atomic PhysicsPerturbation theoryAtomic physicsGround stateApplied Physics B: Lasers and Optics
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Inferring possible magnetic field strength of accreting inflows in EXor-type objects from scaled laboratory experiments

2021

Aims. EXor-type objects are protostars that display powerful UV-optical outbursts caused by intermittent and powerful events of magnetospheric accretion. These objects are not yet well investigated and are quite difficult to characterize. Several parameters, such as plasma stream velocities, characteristic densities, and temperatures, can be retrieved from present observations. As of yet, however, there is no information about the magnetic field values and the exact underlying accretion scenario is also under discussion. Methods. We use laboratory plasmas, created by a high power laser impacting a solid target or by a plasma gun injector, and make these plasmas propagate perpendicularly to …

Shock waveAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesField strengthAstrophysicsstars: pre-main sequence01 natural sciencesmagnetohydrodynamics (MHD)Settore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesProtostarAstrophysics::Solar and Stellar Astrophysics010306 general physics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics[PHYS]Physics [physics]accretion disksAstronomy and AstrophysicsRadiusPlasmashock wavesAccretion accretion disksAccretion (astrophysics)Magnetic fieldT Tauri starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Scienceinstabilitiesstars: individual: V1118 OriAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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3D MHD modeling of the expanding remnant of SN 1987A : role of magnetic field and non-thermal radio emission

2018

Aims. We investigate the role played by a pre-supernova (SN) ambient magnetic field on the dynamics of the expanding remnant of SN 1987A and the origin and evolution of the radio emission from the remnant, in particular, during the interaction of the blast wave with the nebula surrounding the SN. Methods. We model the evolution of SN 1987A from the breakout of the shock wave at the stellar surface to the expansion of its remnant through the surrounding nebula by 3D MHD simulations. The model considers the radiative cooling, the deviations from equilibrium of ionization, the deviation from temperature-equilibration between electrons and ions, and a plausible configuration of the pre-SN ambie…

Shock waveH II regionMagnetohydrodynamics (MHD)shock waveAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesField strengthISM [radio continuum]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesmagnetohydrodynamics (MHD)Radio spectrumindividual: SN 1987A [supernovae]0103 physical sciencesISM [X-rays]010303 astronomy & astrophysicsBlast waveISM: supernova remnantAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Nebulasupernovae: individual: SN 1987A010308 nuclear & particles physicssupernova remnants [ISM]Astronomy and Astrophysicsshock wavesX-rays: ISMMagnetic fieldradio continuum: ISMSpace and Planetary ScienceMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena
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P 56 tDCS shows no effects on motor cortex excitability at rest

2017

Introduction Transcranial direct current stimulation (tDCS) is a widely used technique in research and clinics. However, the underlying physiological mechanisms are not yet clear. Modeling studies suggest that the electric field during tDCS is dominated by a tangential component which predominantly modifies active synaptic connections ( Radman et al., 2007 ). We have previously shown that tDCS with an increased tangential compared to the conventional montage introduced by Nitsche and Paulus (2000) , suppresses the effects of paired associative stimulation of the supplementary motor area and the primary motor cortex (PASSMA-M1) independent of tDCS polarity (Faber et al., under submission). H…

Transcranial direct-current stimulationSupplementary motor areamedicine.medical_treatment05 social sciencesField strength050105 experimental psychologySensory Systems03 medical and health sciences0302 clinical medicineSlice preparationmedicine.anatomical_structureNeurologyPhysiology (medical)Motor systemmedicine0501 psychology and cognitive sciencesNeurology (clinical)Primary motor cortexPsychologyNeuroscience030217 neurology & neurosurgeryRest (music)Motor cortexClinical Neurophysiology
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The dynamical equation of the effective gluon mass

2011

In this article we derive the integral equation that controls the momentum dependence of the effective gluon mass in the Landau gauge. This is accomplished by means of a well-defined separation of the corresponding "one-loop dressed" Schwinger-Dyson equation into two distinct contributions, one associated with the mass and one with the standard kinetic part of the gluon. The entire construction relies on the existence of a longitudinally coupled vertex of nonperturbative origin, which enforces gauge invariance in the presence of a dynamical mass. The specific structure of the resulting mass equation, supplemented by the additional requirement of a positive-definite gluon mass, imposes a rat…

Ward–Takahashi identityPhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsDifferential equationHigh Energy Physics::LatticeHigh Energy Physics - Lattice (hep-lat)High Energy Physics::PhenomenologyPropagatorFísicaFOS: Physical sciencesIntegral equationGluonMass formulaHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - LatticeHigh Energy Physics - Theory (hep-th)Gluon field strength tensorQuantum electrodynamicsGluon fieldMathematical physics
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