Search results for "Magnetic flux"

showing 10 items of 80 documents

Quantum rings for beginners: Energy spectra and persistent currents

2003

Theoretical approaches to one-dimensional and quasi-one-dimensional quantum rings with a few electrons are reviewed. Discrete Hubbard-type models and continuum models are shown to give similar results governed by the special features of the one-dimensionality. The energy spectrum of the many-body states can be described by a rotation-vibration spectrum of a 'Wigner molecule' of 'localized' electrons, combined with the spin-state determined from an effective antiferromagnetic Heisenberg Hamiltonian. The persistent current as a function of the magnetic flux through the ring shows periodic oscillations arising from the 'rigid rotation' of the electron ring. For polarized electrons the periodic…

PhysicsCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)Heisenberg modelFOS: Physical sciencesPersistent currentElectronic structureElectronCondensed Matter PhysicsAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsCondensed Matter - Strongly Correlated Electronssymbols.namesakeLuttinger liquidQuantum mechanicsMagnetic flux quantumMesoscale and Nanoscale Physics (cond-mat.mes-hall)symbolsHamiltonian (quantum mechanics)Quantum
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Experimental investigation of the breakdown of the Onsager-Casimir relations

2006

We use magnetoconductance fluctuation measurements of phase-coherent semiconductor billiards to quantify the contributions to the nonlinear electric conductance that are asymmetric under reversal of magnetic field. We experimentally determine that the average asymmetric contribution is linear in magnetic field (for magnetic flux much larger than one flux quantum) and that its magnitude depends on billiard geometry. In addition, we find an unexpected asymmetry in the power spectrum characteristics of the magnetoconductance with respect to reversal of magnetic field and bias voltage.

PhysicsCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed matter physicsmedia_common.quotation_subjectGeneral Physics and AstronomySpectral densityFOS: Physical sciencesBiasingCondensed Matter::Mesoscopic Systems and Quantum Hall EffectAsymmetryMagnetic fluxMagnetic fieldCasimir effectMagnetic flux quantumMesoscale and Nanoscale Physics (cond-mat.mes-hall)Dynamical billiardsmedia_common
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Local control of domain wall dynamics in ferromagnetic rings

2015

Ferromagnetic nanorings are of great interest due to prospective applications in memory and logic devices based on domain wall (DW) motion.1-3A key-prerequisite for their realization is a reproducible domain wall spin structure with a well-controllable wall velocity. We have found that DW propagation in magnetic ring is characterized by non-constant vortex DW velocity even below Walker breakdown4 (as opposed to straight wires). Several studies have been devoted to the optimization of ring reversal on a global scale using out-of plane field5 or flux charges emanating from neighboring rings if placed in close proximity6. However, these methods involve DW pinning and vortex nucleation processe…

PhysicsDomain wall (magnetism)Condensed matter physicsMagnetic domainSingle domainMagnetic susceptibilityMicromagneticsMagnetic fluxMagnetic fieldVortex2015 IEEE Magnetics Conference (INTERMAG)
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Automotive domain wall propagation in ferromagnetic rings

2015

Automotive domain wall propagation is a self-propelling motion utilizing the energy stored in a particular energy reservoir of the spin structure to speed up domain wall beyond its equilibrium value given by external driving force and damping. Such a concept of DW motion is of great interest due to recent development of spintronic devices based on domain walls, where automotion could be used to assist or prevent domain wall pinning at low driving fields1-2. In turn, most of studies so far have been devoted to the automotion invoked by DW transformations from metastable to stable states3-4; appearing at sufficiently high magnetic fields strong and enough to trigger domain wall spin structure…

PhysicsDomain wall (magnetism)Magnetic domainSpintronicsCondensed matter physicsZeeman energySingle domainMagnetostaticsMagnetic fluxMagnetic field2015 IEEE Magnetics Conference (INTERMAG)
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Melvin Universe in Born-Infeld gravity

2015

We consider a magnetic flux pointing in the $z$ direction of an axially symmetric space-time (Melvin Universe) in a Born-Infeld-type extension of General Relativity (GR) formulated in the Palatini approach. Large magnetic fields could have been produced in the early Universe, and given rise to interesting phenomenology regarding wormholes and black hole remnants. We find a formal analytic solution to this problem that recovers the GR result in the appropriate limits. Our results set the basis for further extensions that could allow the embedding of pairs of black hole remnants in geometries with intense magnetic fields.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsGeneral relativitySpace timeAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Magnetic fluxGeneral Relativity and Quantum CosmologyMagnetic fieldGravitationTheoretical physicsGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Born–Infeld modelWormholePhenomenology (particle physics)
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MHD modelling of coronal loops: injection of high-speed chromospheric flows

2014

Observations reveal a correspondence between chromospheric type II spicules and bright upwardly moving fronts in the corona observed in the EUV band. However, theoretical considerations suggest that these flows are unlikely to be the main source of heating in coronal magnetic loops. We investigate the propagation of high-speed chromospheric flows into coronal magnetic flux tubes, and the possible production of emission in the EUV band. We simulate the propagation of a dense $10^4$ K chromospheric jet upwards along a coronal loop, by means of a 2-D cylindrical MHD model, including gravity, radiative losses, thermal conduction and magnetic induction. The jet propagates in a complete atmospher…

PhysicsJet (fluid)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsCoronal loopCoronaMagnetic fluxMagnetic fieldSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsRadiative transferAstrophysics::Solar and Stellar AstrophysicsMagnetohydrodynamicsSun: chromosphere Sun: corona Sun: UV radiation magnetohydrodynamics (MHD)chromosphere Sun: corona Sun: UV radiation magnetohydrodynamics (MHD) [Sun]ChromosphereSolar and Stellar Astrophysics (astro-ph.SR)
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Magnetic field analysis and leakage inductance calculation in current transformers by means of 3-D integral methods

1996

This paper presents 3D integral approach to power current transformer magnetic field and inductance calculations. A minimization of the kernel norm has been carried out for the integral equation governing the field. The software package TRACAL3, based on the integral methods for field and inductance calculations, has been developed and implemented for personal computers. The application of the 3D mathematical models has been made for the leakage field in a current transformer. The results of calculations were compared with measurement data. The comparison yields good agreement.

PhysicsLeakage inductanceMathematical analysisEquivalent series inductanceMagnetic flux leakageDerivation of self inductanceIntegral equationCurrent transformerElectronic Optical and Magnetic Materialslaw.inventionInductancelawElectrical and Electronic EngineeringTransformerIEEE Transactions on Magnetics
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Coherent Excitation of Heterosymmetric Spin Waves with Ultrashort Wavelengths

2017

In the emerging field of magnonics, spin waves are foreseen as signal carriers for future spintronic information processing and communication devices, owing to both the very low power losses and a high device miniaturisation potential predicted for short-wavelength spin waves. Yet, the efficient excitation and controlled propagation of nanoscale spin waves remains a severe challenge. Here, we report the observation of high-amplitude, ultrashort dipole-exchange spin waves (down to 80 nm wavelength at 10 GHz frequency) in a ferromagnetic single layer system, coherently excited by the driven dynamics of a spin vortex core. We used time-resolved x-ray microscopy to directly image such propagati…

PhysicsMagnonicsCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed matter physicsSpintronicsOscillationGeneral Physics and AstronomyFOS: Physical sciencesLarge scale facilities for research with photons neutrons and ionsPhysik (inkl. Astronomie)01 natural sciencesMagnetic fluxWavelengthSpin wave0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)Condensed Matter::Strongly Correlated Electrons010306 general physicsExcitationSpin-½Physical Review Letters
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Determination of the stochastic evolution equation from noisy experimental data

2003

We have determined the coefficients of the Kardar-Parisi-Zhang equation as functions of coarse graining, which best describe the time evolution and spatial behavior observed for slow-combustion fronts in sheets of paper and magnetic flux fronts in a thin-film high-Tc superconductor. Reconstruction of the relevant equation of motion and its coefficients was mainly based on the inverse method proposed by Lam and Sander [Phys. Rev. Lett. 71, 561 (1993)]. The coefficient of the nonlinear term was also determined from the local slope-dependence of the front velocity.

PhysicsNonlinear systemStochastic processCondensed Matter::Statistical MechanicsFront velocityTime evolutionEquations of motionStatistical physicsInverse problemCondensed Matter PhysicsMagnetic fluxElectronic Optical and Magnetic MaterialsKardar–Parisi–Zhang equationThe European Physical Journal B - Condensed Matter
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Development and test of iron-free quadrupole lenses with high magnetic flux densities

2003

Abstract Iron-free magnetic quadrupole lenses have been developed for the focusing of energetic bunched heavy-ion beams. These devices are operated in a pulsed mode and provide very strong magnetic fields. A magnetic flux density of more than 14 T has been reached in a 100 mm long quadrupole with a 20 mm wide aperture, which corresponds to a magnetic flux density of ∼1400 T/m. The pulse duration of the applied electric current is approximately 300 μs with a flat top of several μs. The calculated and measured field properties of the quadrupoles are presented. In a first test experiment with a fast-extracted 650 MeV/u 197 Au 79+ beam (bunch length ∼500 ns) at GSI the focusing properties could…

PhysicsNuclear and High Energy PhysicsMagnetQuadrupolePhysics::Accelerator PhysicsPulse durationElectric currentAtomic physicsQuadrupole magnetInstrumentationMagnetic fluxStorage ringMagnetic fieldNuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms
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