Search results for " Magnetic field"

showing 10 items of 165 documents

The chain length of anisotropic paramagnetic particles in a rotating field

2020

In this article, the maximal length of a chain of paramagnetic particles with magnetic anisotropy in a rotating magnetic field is studied. The theory of paramagnetic particle chains usually assumes that the particles are magnetically isotropic and do not rotate in a rotating field. In experiments it is seen that spherical paramagnetic particles rotate, which can be explained by small magnetic anisotropy. In this article, the maximal chain length is calculated for paramagnetic particles with magnetic anisotropy in a rotating magnetic field. Results show that the maximal chain length as a function of field frequency has the same trend for isotropic magnetic particles and particles with magnet…

ParamagnetismRotating magnetic fieldMagnetic anisotropyMaterials scienceCondensed matter physicsIsotropyMagnetic nanoparticlesParticleCondensed Matter - Soft Condensed MatterCondensed Matter PhysicsAnisotropyMicromagneticsElectronic Optical and Magnetic MaterialsJournal of Magnetism and Magnetic Materials
researchProduct

Next Generation Search for Axion and ALP Dark Matter with the International Axion Observatory

2018

International audience; More than 80 years after the postulation of dark matter, its nature remains one of the fundamental questions in cosmology. Axions are currently one of the leading candidates for the hypothetical, non-baryonic dark matter that is expected to account for about 25% of the energy density of the Universe. Especially in the light of the Large Hadron Collider at CERN slowly closing in on Weakly-Interacting Massive Particle (WIMP) searches, axions and axion-like particles (ALPs) provide a viable alternative approach to solving the dark matter problem. The fact that makes them particularly appealing is that they were initially introduced to solve a long-standing problem in qu…

Particle physicsCERN LabPhysics::Instrumentation and DetectorsDark matterObservatoriesaxion: detector7. Clean energy01 natural sciencesCosmologyHigh Energy Physics::TheoryPrimakoff effectSensitivityWIMP0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsAxionPrimakoff effectactivity reportPhysicsHelioscopeLarge Hadron Collider010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyToroidal magnetic fieldsDetectorsobservatory13. Climate actionCouplingsaxion-like particlesproposed experimentCERN Axion Solar Telescopeaxion: solarTelescopes
researchProduct

Transverse Oscillations in Slender Ca II H Fibrils Observed with Sunrise/SuFI

2016

S. Jafarzadeh et. al.

Physics010504 meteorology & atmospheric sciencesCondensed matter physicsoscillations [Sun]imaging spectroscopy [Techniques]Sun: chromosphereFOS: Physical sciencesAstronomy and Astrophysicschromosphere [Sun]Fibril01 natural sciencesTransverse planemagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciencesSunriseAstrophysics::Solar and Stellar Astrophysics14. Life underwaterSun: oscillationsTechniques: imaging spectroscopySun: magnetic fields010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciences
researchProduct

The First Terrestrial Electron Beam Observed by the Atmosphere‐Space Interactions Monitor

2019

We report the first Terrestrial Electron Beam detected by the Atmosphere‐Space Interactions Monitor. It happened on 16 September 2018. The Atmosphere‐Space Interactions Monitor Modular X and Gamma ray Sensor recorded a 2 ms long event, with a softer spectrum than typically recorded for Terrestrial Gamma ray Flashes (TGFs). The lightning discharge associated to this event was found in the World Wide Lightning Location Network data, close to the northern footpoint of the magnetic field line that intercepts the International Space Station location. Imaging from a GOES‐R geostationary satellite shows that the source TGF was produced close to an overshooting top of a thunderstorm. Monte‐Carlo si…

Physics010504 meteorology & atmospheric sciencesElectronSpace (mathematics)01 natural sciencesComputational physicsAtmosphereGeophysicsEarth's magnetic fieldPositron13. Climate actionSpace and Planetary ScienceCathode rayThunderstorm0105 earth and related environmental sciencesJournal of Geophysical Research: Space Physics
researchProduct

Moving Magnetic Features around a Pore

2017

A. J. Kaithakkal et. al.

Physics010504 meteorology & atmospheric sciencesphotosphere [Sun]Polarity (physics)Sun: photosphereFluxFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics01 natural sciencesMagnetic fieldmagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciencesSunriseStatistical analysisSun: magnetic fields010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciences
researchProduct

Mass accretion to young stars triggered by flaring activity in circumstellar discs

2011

Young low-mass stars are characterized by ejection of collimated outflows and by circumstellar disks which they interact with through accretion of mass. The accretion builds up the star to its final mass and is also believed to power the mass outflows, which may in turn remove the excess angular momentum from the star-disk system. However, although the process of mass accretion is a critical aspect of star formation, some of its mechanisms are still to be fully understood. A point not considered to date and relevant for the accretion process is the evidence of very energetic and frequent flaring events in these stars. Flares may easily perturb the stability of the disks, thus influencing th…

PhysicsAngular momentumStar formationAstrophysics::High Energy Astrophysical PhenomenaStellar magnetic fieldAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsThermal conductionAccretion (astrophysics)law.inventionStarsSpace and Planetary SciencelawAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsMagnetohydrodynamicsAstrophysics::Galaxy AstrophysicsFlareMonthly Notices of the Royal Astronomical Society
researchProduct

Order in the Chaos: Spin-up and Spin-down during the 2002 Outburst of SAX J1808.4-3658

2006

We present a timing analysis of the 2002 outburst of the accreting millisecond pulsar SAX J1808.4-3658. A study of the phase delays of the entire pulse profile shows a behavior that is surprising and difficult to interpret: superposed to a general trend, a big jump by about 0.2 in phase is visible, starting at day 14 after the beginning of the outburst. An analysis of the pulse profile indicates the presence of a significant first harmonic. Studying the fundamental and the first harmonic separately, we find that the phase delays of the first harmonic are more regular, with no sign of the jump observed in the fundamental. The fitting of the phase delays of the first harmonic with a model whi…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Phase (waves)X-ray binaryFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsPulse (physics)Neutron starPulsarSpace and Planetary ScienceMillisecond pulsarAstrophysics::Solar and Stellar AstrophysicsStars: Pulsars: General Stars: Pulsars: Individual: SAX J1808.4-3658 Stars: Magnetic Fields Stars: Neutron X-Rays: BinariesExponential decaySpin-½
researchProduct

Quantum dynamics of a nanomagnet in a rotating field

2005

Quantum dynamics of a two-state spin system in a rotating magnetic field has been studied. Analytical and numerical results for the transition probability have been obtained along the lines of the Landau-Zener-Stueckelberg theory. The effect of various kinds of noise on the evolution of the system has been analyzed.

PhysicsCondensed Matter - Materials ScienceRotating magnetic fieldCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed matter physicsField (physics)Quantum dynamicsMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciencesQuantum Hall effectCondensed Matter Physics01 natural sciencesNoise (electronics)Nanomagnet010305 fluids & plasmasElectronic Optical and Magnetic MaterialsBackground noiseSpin crossoverMesoscale and Nanoscale Physics (cond-mat.mes-hall)0103 physical sciences010306 general physicsPhysical Review B
researchProduct

High Magnetic Fields Thermodynamics of Heavy Fermion Metals

2014

In this chapter, we present the comprehensive theoretical analysis of thermodynamics of HF compounds at high magnetic fields. Such analysis permits to gain a deeper insight into the interplay of high magnetic field and temperature in suppressing and retrieving the Landau Fermi liquid state in these substances. Our analysis shows that although high magnetic fields and temperatures alter the properties of ordinary Landau quasiparticles, they survive, generating the experimentally observable anomalies in the thermodynamical quantities of HF compounds. We illustrate our theoretical findings by the example of the HF compound \(\mathrm{{YbRh_2Si_2}}\).

PhysicsCondensed matter physicsHeavy fermionQuasiparticleThermodynamicsCondensed Matter::Strongly Correlated ElectronsObservableFermi liquid theoryHigh magnetic fieldMagnetic field
researchProduct

Production and detection of atomic hexadecapole at Earth’s magnetic field

2007

We report a novel method that allows selective creation and detection of a macroscopic long lived hexadecapole polarization in the F = 2 ground state of 87Rb atoms at Earth's magnetic field (510 mG).

PhysicsEarth's magnetic fieldchemistryNonlinear opticschemistry.chemical_elementAtomic physicsGround statePolarization (waves)Magnetic fieldRubidiumFrontiers in Optics 2007/Laser Science XXIII/Organic Materials and Devices for Displays and Energy Conversion
researchProduct