Search results for "MAGNETIC FIELD"

showing 10 items of 1488 documents

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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Afterglow light curves from magnetized GRB flows

2010

AbstractUsing the RMHD code MRGENESIS and the radiative transfer code SPEV we compute multiwavelength afterglow light curves of magnetized ejecta of gamma-ray bursts interacting with a uniform circumburst medium. We are interested in the emission from the reverse shock when ejecta magnetization varies from σ0 = 0 to σ0 = 1. For typical parameters of the ejecta, the emission from the reverse shock peaks for magnetization σ0 ~ 0.01 − 0.1, and is suppressed for higher σ0. We fit the early afterglow light curves of GRB 990123 and 090102 and discuss the possible magnetization of the outflows of these bursts. Finally we discuss the amount energy left in the magnetic field which is available for d…

PhysicsShock waveMagnetizationSpace and Planetary ScienceRadiative transferAstronomy and AstrophysicsAstrophysicsLight curveGamma-ray burstEjectaMagnetic fieldAfterglowProceedings of the International Astronomical Union
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Modeling magnetohydrodynamics and non equilibrium SoHO/UVCS line emission of CME shocks

2008

We provide a guideline to interpret the UVCS emission lines (in particular O VI and Si XII) during shock wave propagation in the outer solar corona. We use a numerical MHD model performing a set of simulations of shock waves generated in the corona and from the result we compute the plasma emission for the O VI and Si XII including the effects of NEI. We analyze the radiative and spectral properties of our model with the support of a detailed radiation model including Doppler dimming and an analytical model for shocks, and, finally, we synthesize the expected O VI 1032A line profile. We explain several spectral features of the observations like the absence of discontinuities in the O VI emi…

PhysicsShock waveMagnetohydrodynamics (MHD)Sun: coronaSun: coronal mass ejections (CMEs)Astrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsPlasmaAstrophysicsShock (mechanics)Magnetic fieldSpace and Planetary SciencePhysics::Space PhysicsRadiative transferAstrophysics::Solar and Stellar AstrophysicsEmission spectrumMagnetohydrodynamicsAstrophysics::Galaxy AstrophysicsLine (formation)
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Magnetic excitations of the singlet ground state antiferromagnet CsFeBr3 in a magnetic field

1991

Abstract The magnetic excitations in the quasi-one-dimensional singlet ground state antiferromagnet CsFeBr3 have been studied by inelastic neutron scattering in the presence of an applied magnetic field, H‖c and H⊥c. With H‖c, the dispersion curves renormalise so that the exchange interaction has a decreasing influence with increasing field. H⊥c has little or no effect on the dispersion of the magnetic excitations.

PhysicsSinglet ground stateField (physics)Condensed matter physicsExchange interactionDispersion (optics)AntiferromagnetismElectrical and Electronic EngineeringCondensed Matter PhysicsInelastic neutron scatteringElectronic Optical and Magnetic MaterialsMagnetic fieldPhysica B: Condensed Matter
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First Direct Observation of the Interaction between a Comet and a Coronal Mass Ejection Leading to a Complete Plasma Tail Disconnection

2007

This a discovery report of the first direct imaging of the interaction a comet with a coronal mass ejection (CME) in the inner heliosphere with high temporal and spatial resolution. The observations were obtained by the Sun-Earth Connection Coronal and Heliospheric Investigation (SECCHI) Heliospheric Imager-1 (HI-1) aboard the STEREO mission. They reveal the extent of the plasma tail of comet 2P/Encke to unprecedented lengths and allow us to examine the mechanism behind a spectacular tail disconnection event. Our preliminary analysis suggests that the disconnection is driven by magnetic reconnection between the magnetic field entrained in the CME and the interplanetary field draped around t…

PhysicsSolar windSpace and Planetary ScienceCometCoronal mass ejectionAstronomyAstronomy and AstrophysicsMagnetic reconnectionPlasmaInterplanetary spaceflightHeliosphereMagnetic fieldThe Astrophysical Journal
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Many-electron transport in Aharonov-Bohm interferometers: Time-dependent density-functional study

2012

We apply time-dependent density-functional theory to study many-electron transport in Aharonov-Bohm interferometers in a non-equilibrium situation. The conductance properties in the system are complex and depend on the enclosed magnetic flux in the interferometer, the number of interacting particles, and the mutual distance of the transport channels at the points of encounter. Generally, the electron-electron interactions do not suppress the visibility of Aharonov-Bohm oscillations if the interchannel distance -- determined by the positioning of the incompressible strips through the external magnetic field -- is optimized. However, the interactions also impose an interesting Aharonov-Bohm p…

PhysicsSolid-state physicsStrongly Correlated Electrons (cond-mat.str-el)Condensed Matter - Mesoscale and Nanoscale PhysicsOscillationFOS: Physical sciences02 engineering and technologyElectron021001 nanoscience & nanotechnologyCondensed Matter PhysicsCondensed Matter::Mesoscopic Systems and Quantum Hall Effect01 natural sciencesMagnetic fluxElectronic Optical and Magnetic MaterialsMagnetic fieldInterferometryCondensed Matter - Strongly Correlated ElectronsAmplitudeQuantum electrodynamics0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)Astronomical interferometer010306 general physics0210 nano-technology
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Dynamic N14 nuclear spin polarization in nitrogen-vacancy centers in diamond

2020

We studied the dynamic nuclear spin polarization of nitrogen in negatively charged nitrogen-vacancy (NV) centers in diamond both experimentally and theoretically over a wide range of magnetic fields from 0--1100 G covering both the excited-state level anticrossing and the ground-state level anticrossing magnetic field regions. Special attention was paid to the less studied ground-state level anticrossing region. The nuclear spin polarization was inferred from measurements of the optically detected magnetic resonance signal. These measurements show that a very large (up to $96\ifmmode\pm\else\textpm\fi{}2%$) nuclear spin polarization of nitrogen can be achieved over a very broad range of mag…

PhysicsSpin polarizationchemistry.chemical_elementDiamond02 engineering and technologyengineering.material021001 nanoscience & nanotechnologyPolarization (waves)01 natural sciencesNitrogenMagnetic fieldchemistryVacancy defect0103 physical sciencesengineeringAtomic physics010306 general physics0210 nano-technologyExcitationPhysical Review B
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Spin pumping in noncollinear antiferromagnets

2021

The ac spin pumping of noncollinear antiferromagnets is theoretically investigated. Starting from an effective action description of the spin system, we derive the Onsager coefficients connecting the spin pumping and spin-transfer torque associated with the dynamics of the SO(3)-valued antiferromagnetic order parameter. Our theory is applied to a kagome antiferromagnet resonantly driven by a uniform external magnetic field. We demonstrate that the reactive (dissipative) spin-transfer torque parameter can be extracted from the pumped ac spin current in-phase (in quadrature) with the driving field. Furthermore, we find that the three spin-wave bands of the kagome AF generate spin currents wit…

PhysicsSpin pumpingCondensed Matter - Materials ScienceField (physics)Condensed matter physicsCondensed Matter - Mesoscale and Nanoscale PhysicsOrthogonal polarization spectral imagingPhase (waves)Materials Science (cond-mat.mtrl-sci)FOS: Physical sciencesMagnetic fieldMesoscale and Nanoscale Physics (cond-mat.mes-hall)Dissipative systemAntiferromagnetismCondensed Matter::Strongly Correlated ElectronsSpin-½
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Matter-wave interference versus spontaneous pattern formation in spinor Bose-Einstein condensates

2013

We describe effects of matter-wave interference of spinor states in the $^{87}$Rb Bose-Einstein condensate. The components of the F=2 manifold are populated by forced Majorana transitions and then fall freely due to gravity in an applied magnetic field. Weak inhomogeneities of the magnetic field, present in the experiment, impose relative velocities onto different $m_F$ components, which show up as interference patterns upon measurement of atomic density distributions with a Stern-Gerlach imaging method. We show that interference effects may appear in experiments even if gradients of the magnetic field components are eliminated but higher order inhomogeneity is present and the duration of t…

PhysicsSpinorFOS: Physical sciencesPattern formationInterference (wave propagation)Atomic and Molecular Physics and OpticsManifoldMagnetic fieldlaw.inventionMAJORANAQuantum Gases (cond-mat.quant-gas)lawQuantum mechanicsMatter waveCondensed Matter - Quantum GasesBose–Einstein condensatePhysical Review A
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Nuclear-spin comagnetometer based on a liquid of identical molecules

2018

Atomic comagnetometers are used in searches for anomalous spin-dependent interactions. Magnetic field gradients are one of the major sources of systematic errors in such experiments. Here we describe a comagnetometer based on the nuclear spins within an ensemble of identical molecules. The dependence of the measured spin-precession frequency ratio on the first-order magnetic field gradient is suppressed by over an order of magnitude compared to a comagnetometer based on overlapping ensembles of different molecules. Our single-species comagnetometer is shown to be capable of measuring the hypothetical spin-dependent gravitational energy of nuclei at the $10^{-17}$ eV level, comparable to the…

PhysicsSpinsAtomic Physics (physics.atom-ph)Frequency ratioGeneral Physics and AstronomyFOS: Physical sciences02 engineering and technologyMagnetic field gradient021001 nanoscience & nanotechnologyPolarization (waves)01 natural sciencesMolecular physicsGravitational energyPhysics - Atomic Physics0103 physical sciencesMolecule010306 general physics0210 nano-technologyNucleonOrder of magnitude
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