Search results for "MAGNETIC FIELD"

showing 10 items of 1488 documents

Dynamics of a flexible ferromagnetic filament in a rotating magnetic field.

2017

Flexible magnetic filaments have garnered considerable attention as prospective materials for the creation of different microdevices. We describe a theoretical model of a ferromagnetic filament and derive its equations of motion by variational techniques. The numerical algorithm used to solve the filament dynamics in magnetic fields of different configurations is described. It is found that in a rotating field the filament transitions between synchronous and asynchronous regimes with respect to the rotating field, similarly to a rigid magnetic dipole. The mean angular velocity of the filament is well described by a relation valid for a rigid magnetic dipole with quantitative differences att…

PhysicsRotating magnetic fieldCondensed matter physicsField (physics)Equations of motionAngular velocity02 engineering and technology021001 nanoscience & nanotechnology01 natural sciences010305 fluids & plasmasMagnetic fieldQuantitative Biology::Subcellular ProcessesProtein filamentFerromagnetism0103 physical sciences0210 nano-technologyMagnetic dipolePhysical review. E
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3D motion of flexible ferromagnetic filaments under a rotating magnetic field.

2020

Ferromagnetic filaments in a rotating magnetic field are studied both numerically and experimentally. The filaments are made from micron-sized ferromagnetic particles linked with DNA strands. It is found that at low frequencies of the rotating field a filament rotates synchronously with the field and beyond a critical frequency it undergoes a transition to a three dimensional regime. In this regime the tips of the filament rotate synchronously with the field on circular trajectories in the plane parallel to the plane of the rotating field. The characteristics of this motion found numerically match the experimental data and allow us to obtain the physical properties of such filaments. We als…

PhysicsRotating magnetic fieldCondensed matter physicsField (physics)Plane (geometry)FOS: Physical sciences02 engineering and technologyGeneral ChemistryCondensed Matter - Soft Condensed Matter021001 nanoscience & nanotechnologyCondensed Matter Physics01 natural sciencesRodQuantitative Biology::Cell BehaviorProtein filamentQuantitative Biology::Subcellular ProcessesFerromagnetismCritical frequency0103 physical sciencesSoft Condensed Matter (cond-mat.soft)010306 general physics0210 nano-technologyMixing (physics)Soft matter
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Bending of ferrofluid droplet in rotating magnetic field

1999

Abstract This paper presents results concerning 2D ferrofluid droplet motion at high values of magnetic field and frequencies above a critical one with respect to droplet ability to follow field rotation. The boundary element method is used to solve 2D equations of a magnetic field and Stokes flow problems. If the viscosity of the ferrofluid is larger than that of the surrounding fluid, droplet exhibits bending, forming “S-shape”. Fluid flow inside the droplet is analyzed and the main stages of periodical rotation of a droplet are reported.

PhysicsRotating magnetic fieldFerrofluidField (physics)MechanicsStokes flowCondensed Matter PhysicsRotationElectronic Optical and Magnetic MaterialsMagnetic fieldPhysics::Fluid DynamicsViscosityClassical mechanicsPhysics::Atomic and Molecular ClustersFluid dynamicsJournal of Magnetism and Magnetic Materials
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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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Diffusion in active magnetic colloids

2013

Abstract Properties of active colloids of circle swimmers are reviewed. As a particular example of active magnetic colloids the magnetotactic bacteria under the action of a rotating magnetic field is considered. The relation for a diffusion coefficient due to the random switching of the direction of rotation of their rotary motors is derived on the basis of the master equation. The obtained relation is confirmed by the direct numerical simulation of random trajectory of a magnetotactic bacterium under the action of the Poisson type internal noise due to the random switching of rotary motors. The results obtained are in qualitative and quantitative agreement with the available experimental r…

PhysicsRotating magnetic fieldMagnetotactic bacteriaStatistical Mechanics (cond-mat.stat-mech)Direct numerical simulationFOS: Physical sciencesCondensed Matter - Soft Condensed MatterCondensed Matter PhysicsRotation01 natural sciences6. Clean waterAction (physics)010305 fluids & plasmasElectronic Optical and Magnetic MaterialsQuantitative Biology::Cell BehaviorQuantitative Biology::Subcellular ProcessesClassical mechanics0103 physical sciencesMaster equationTrajectorySoft Condensed Matter (cond-mat.soft)Diffusion (business)010306 general physicsCondensed Matter - Statistical MechanicsJournal of Magnetism and Magnetic Materials
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Parametric excitation of bending deformations of a rod by periodic twist

2013

A model of a semiflexible magnetic filament with magnetization frozen in the direction perpendicular to the tangent of its center line is formulated. It is shown that if the rod is magnetized at its ends in opposite directions, an AC magnetic field causes parametric excitation of bending deformations. Neutral curves of parametric excitation are calculated both analytically and numerically. The shapes arising upon parametric excitation of bending deformations are chiral. Periodic rotation of the chiral filament due to nonhomogeneous twist in a nonhomogeneous AC field causes its unidirectional motion.

PhysicsRotationTangentBendingMechanicsRotationMagnetic fieldMagnetizationElectromagnetic FieldsModels ChemicalPerpendicularNanoparticlesComputer SimulationExcitationParametric statisticsPhysical Review E
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Extreme increase in atomic transition probability of the Cs D_2 line in strong magnetic fields under selective reflection

2016

Selective reflection of 852-nm laser radiation from the interface between cesium vapor and the sapphire window of a 30-micrometer-thick microcell was used to record an extreme increase in the probability of the Fg=3→Fe=5 transitions associated with the Cs-atom D2 lines in magnetic fields with inductions ranging from 300 to 3200 Gauss. We showed that a group of seven transitions Fg=3, mF=−3, −2, −1, 0, +1, +2, +3→Fe=5, mF=−2, −1, 0, +1, +2, +3, +4 was formed in accordance with the selection rules ΔmF=+1 for σ+-circularly-polarized radiation. These seven transitions have much higher probabilities in 500–1000 Gauss magnetic fields, with three of the transitions having probabilities higher than…

PhysicsSapphire windowApplied MathematicsGaussGeneral EngineeringRadiationLaser01 natural sciencesCesium vaporAtomic and Molecular Physics and OpticsMagnetic fieldlaw.invention010309 opticsComputational Mathematicslaw0103 physical sciencesSelective reflectionAtomic physics010306 general physicsLine (formation)Journal of Optical Technology
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BeppoSAX serendipitous discovery of the X-ray pulsar SAX J1802.7-2017

2003

We report on the serendipitous discovery of a new X-ray source, SAX J1802.7-2017, ~22' away from the bright X-ray source GX 9+1, during a BeppoSAX observation of the latter source on 2001 September 16-20. SAX J1802.7-2017 remained undetected in the first 50 ks of observation; the source count rate in the following ~300 ks ranged between 0.04 c/s and 0.28 c/s, corresponding to an averaged 0.1-10 keV flux of 3.6 10^{-11} ergs cm^{-2} s^{-1}. We performed a timing analysis and found that SAX J1802.7-2017 has a pulse period of 139.612 s, a projected semimajor axis of a_x sin i ~ 70 lt-s, an orbital period of ~4.6 days, and a mass function f(M) ~ 17 Msun. The new source is thus an accreting X-ra…

PhysicsSemi-major axisAstrophysics (astro-ph)FluxFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsOrbital periodPulse periodSettore FIS/05 - Astronomia E AstrofisicaPulsarSpace and Planetary ScienceHigh massStars: Pulsars: General Stars: Pulsars: Individual: Alphanumeric: SAX J1802.7-2017 Stars: Magnetic Fields Stars: Neutron X-Rays: BinariesX-ray pulsar
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Billiards in magnetic fields: A molecular dynamics approach

2009

We present a computational scheme based on classical molecular dynamics to study chaotic billiards in static external magnetic fields. The method allows to treat arbitrary geometries and several interacting particles. We test the scheme for rectangular single-particle billiards in magnetic fields and find a sequence of regularity islands at integer aspect ratios. In the case of two Coulomb-interacting particles the dynamics is dominated by chaotic behavior. However, signatures of quasiperiodicity can be identified at weak interactions, as well as regular trajectories at strong magnetic fields. Our scheme provides a promising tool to monitor the classical limit of many-electron semiconductor…

PhysicsSequenceCondensed Matter - Mesoscale and Nanoscale PhysicsChaoticFOS: Physical sciencesNonlinear Sciences - Chaotic DynamicsClassical limitMagnetic fieldCondensed Matter - Other Condensed MatterNonlinear Sciences::Chaotic DynamicsMolecular dynamicsQuasiperiodicityClassical mechanicsQuantum dotMesoscale and Nanoscale Physics (cond-mat.mes-hall)Chaotic Dynamics (nlin.CD)Integer (computer science)Other Condensed Matter (cond-mat.other)
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3D YSO accretion shock simulations: a study of the magnetic, chromospheric and stochastic flow effects

2013

AbstractThe structure and dynamics of young stellar object (YSO) accretion shocks depend strongly on the local magnetic field strength and configuration, as well as on the radiative transfer effects responsible for the energy losses. We present the first 3D YSO shock simulations of the interior of the stream, assuming a uniform background magnetic field, a clumpy infalling gas, and an acoustic energy flux flowing at the base of the chromosphere. We study the dynamical evolution and the post-shock structure as a function of the plasma-beta (thermal pressure over magnetic pressure). We find that a strong magnetic field (~hundreds of Gauss) leads to the formation of fibrils in the shocked gas …

PhysicsShock waveAccretion (meteorology)Shock (fluid dynamics)Astrophysics::High Energy Astrophysical PhenomenaFluxAstronomy and AstrophysicsAstrophysicsshock waves[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]magnetohydrodynamics (MHD)Magnetic fieldSettore FIS/05 - Astronomia E AstrofisicaaccretionSpace and Planetary Scienceradiative transferinstabilitiesaccretion magnetohydrodynamics (MHD) radiative transfer shock waves instabilitiesRadiative transferAstrophysics::Solar and Stellar AstrophysicsMagnetic pressureChromosphereAstrophysics::Galaxy Astrophysics
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