Search results for "Magnetic dip"

showing 10 items of 219 documents

Rho resonance, timelike pion form factor, and implications for lattice studies of the hadronic vacuum polarization

2020

We study isospin-1 P-wave ππ scattering in lattice QCD with two flavors of O(a) improved Wilson fermions. For pion masses ranging from mπ=265 MeV to mπ=437 MeV, we determine the energy spectrum in the center-of-mass frame and in three moving frames. We obtain the scattering phase shifts using Lüscher’s finite-volume quantization condition. Fitting the dependence of the phase shifts on the scattering momentum to a Breit-Wigner form allows us to determine the corresponding ρ mass mρ and gρππ coupling. By combining the scattering phase shifts with the decay matrix element of the vector current, we calculate the timelike pion form factor, Fπ, and compare the results to the Gounaris-Sakurai repr…

1 [isospin]Particle physicsdecay constant [rho(770)]High Energy Physics::Latticeclover [fermion]energy spectrumFOS: Physical sciencesWilson [quark]01 natural sciencesphase shiftHigh Energy Physics - LatticePionvector [correlation function]Charge radius0103 physical sciencesmagnetic moment [muon]quantum chromodynamicsmass [rho(770)]hadronic [vacuum polarization]ddc:530Vacuum polarizationflavor: 2 [quark]010306 general physicsnumerical calculationscharge radius [pi]PhysicsMuonAnomalous magnetic dipole moment010308 nuclear & particles physicsScatteringHigh Energy Physics - Lattice (hep-lat)scatteringlattice field theoryLattice QCDFermionBreit-Wignermass dependence [quark]form factor [pi]effect [finite size]vector [current]quantizationPhysical Review D
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<title>Influence of radiation defects on exciton-magnon interactions in nickel oxide</title>

2005

Influence of radiation defects on the optical absorption spectrum of nickel oxide (NiO) was studied at 6 K in the near-IR energy range of 7750-8300 cm-1 corresponding to the magnetic-dipole transition 3A 2g(F )->3T 2g(F ) at nickel sites. NiO single crystals grown by the method of chemical transport reactions on the MgO(100) substrates were irradiated by the neutron fluences up to 5x1018 cm-2. Two sharp lines were observed at the low-energy side of the band: the peak at 7805 cm-1 is assigned to the pure exciton transition, whereas the peak at 7845 cm-1, to the exciton-magnon excitation that occurs at the Brillouin zone-center (BZC). An increase of the defect concentration at higher fluences…

Absorption spectroscopyCondensed matter physicsMagnetic dipole transitionNickel oxideMagnonExcitonchemistry.chemical_elementCondensed Matter::Materials ScienceNickelNuclear magnetic resonancechemistryCondensed Matter::Strongly Correlated ElectronsIrradiationAbsorption (electromagnetic radiation)SPIE Proceedings
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Binary neutron star mergers: a jet engine for short gamma-ray bursts

2016

We perform magnetohydrodynamic simulations in full general relativity (GRMHD) of quasi-circular, equal-mass, binary neutron stars that undergo merger. The initial stars are irrotational, $n=1$ polytropes and are magnetized. We explore two types of magnetic-field geometries: one where each star is endowed with a dipole magnetic field extending from the interior into the exterior, as in a pulsar, and the other where the dipole field is initially confined to the interior. In both cases the adopted magnetic fields are initially dynamically unimportant. The merger outcome is a hypermassive neutron star that undergoes delayed collapse to a black hole (spin parameter $a/M_{\rm BH} \sim 0.74$) imme…

AstrofísicaAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyArticlePulsar0103 physical sciencesBinary starAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsBlack holeNeutron starStarsSpace and Planetary ScienceAstronomiaAstrophysics::Earth and Planetary AstrophysicsGamma-ray burstAstrophysics - High Energy Astrophysical PhenomenaMagnetic dipole
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Indications of non-conservative mass-transfer in AMXPs

2019

Context. Since the discovery of the first Accreting Millisecond X-ray Pulsar SAX J1808.4-3658 in 1998, the family of these sources kept growing on. Currently, it counts 22 members. All AMXPs are transients with usually very long quiescence periods, implying that mass accretion rate in these systems is quite low and not constant. Moreover, for at least three sources, a non-conservative evolution was also proposed. Aims. Our purpose is to study the long term averaged mass-accretion rates in all the Accreting Millisecond X-ray Pulsars discovered so far, to investigate a non-conservative mass-transfer scenario. Methods. We calculated the expected mass-transfer rate under the hypothesis of a con…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)X-rays: starsAstrophysicsCompact star01 natural sciencesLuminositystars: neutronX-rays: binariesPulsarpulsars: general0103 physical sciencesX-rays: individuals: IGR J17498−2921X-rays: individuals: IGR J17498-2921010303 astronomy & astrophysicsX-rays: individuals: XTE J1814−338PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsX-rays: binarieX-rays: individuals: XTE J1814-338Radiation pressureSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Magnetic dipole
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Measurement of untruncated nuclear spin interactions via zero- to ultralow-field nuclear magnetic resonance

2015

Zero- to ultra-low-field nuclear magnetic resonance (ZULF NMR) provides a new regime for the measurement of nuclear spin-spin interactions free from effects of large magnetic fields, such as truncation of terms that do not commute with the Zeeman Hamiltonian. One such interaction, the magnetic dipole-dipole coupling, is a valuable source of spatial information in NMR, though many terms are unobservable in high-field NMR, and the coupling averages to zero under isotropic molecular tumbling. Under partial alignment, this information is retained in the form of so-called residual dipolar couplings. We report zero- to ultra-low-field NMR measurements of residual dipolar couplings in acetonitrile…

Atomic Physics (physics.atom-ph)Fluids & Plasmasphysics.chem-phFOS: Physical sciences010402 general chemistryJ-couplingphysics.atom-ph01 natural sciencesPhysics - Atomic Physicssymbols.namesakeEngineeringNuclear magnetic resonancequant-phPhysics - Chemical Physics0103 physical sciencesMagnetization transfer010306 general physicsChemical Physics (physics.chem-ph)PhysicsQuantum PhysicsZeeman effectCondensed matter physicsCondensed Matter Physics0104 chemical sciences3. Good healthElectronic Optical and Magnetic MaterialsMagnetic fieldSolid-state nuclear magnetic resonanceResidual dipolar couplingPhysical SciencesChemical SciencessymbolsQuantum Physics (quant-ph)Two-dimensional nuclear magnetic resonance spectroscopyMagnetic dipole–dipole interaction
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Dipole Moments and the Direction of the Transition Dipole Moment of Some Intramolecular Exciplexes

1988

The dipole moments of some intramolecular exciplex systems have been determined from the effect of an electric field on their fluorescence and are compared to those estimated from solvent shift measurements. The charge transfer between the donor and acceptor subunits is between 0.6 and 0.9 of a full charge transfer. The face-to-face type exciplexes show considerable deviations from the general behaviour what might be due to some admixture of locally excited configurations to the exciplex wave function, in this way reducing the dipole moment values and changing the direction of the transition dipole moment.

Bond dipole momentDipoleElectric dipole momentChemistryGeneral Chemical EngineeringChemical polarityMoment (physics)Transition dipole momentPhysics::Atomic and Molecular ClustersElectric dipole transitionAtomic physicsPhotochemistryMagnetic dipoleBerichte der Bunsengesellschaft für physikalische Chemie
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Heavy mass expansion, light-by-light scattering through pointlike quanta, and the anomalous magnetic moment of the muon

2003

Contributions from light-by-light scattering to ${(g}_{\ensuremath{\mu}}\ensuremath{-}2)/2,$ the anomalous magnetic moment of the muon, are mediated by the exchange of charged fermions or scalar bosons. Assuming large masses M, pointlike couplings for the virtual particles and employing the technique of large mass expansion, analytical results are obtained for virtual fermions and scalars in the form of a series in ${(m}_{\ensuremath{\mu}}{/M)}^{2}.$ This series is well convergent even for the case ${M=m}_{\ensuremath{\mu}}.$ For pointlike virtual fermions, the expansion confirms published analytical formulas. For virtual scalars, the result can be used to evaluate the contribution from poi…

Condensed Matter::Quantum GasesPhysicsNuclear and High Energy PhysicsParticle physicsMuonAnomalous magnetic dipole momentNeutron magnetic momentVirtual particleFermionElectron magnetic dipole momentBosonSpin magnetic momentPhysical Review D
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Exploring Quantum Matter with Ultracold Atoms in Optical Lattices

2005

Publisher Summary This chapter explores quantum matter with ultracold atoms in optical lattices. The chapter focuses on bosonic atoms in optical lattices and on the regime where strong correlations between the atoms become important. In the interaction of atoms with coherent light fields, two fundamental forces arise. The Doppler force is dissipative in nature and can be used to efficiently laser cool a gas of atoms and relies on the radiation pressure together with spontaneous emission. The dipole force creates a purely conservative potential in which the atoms can move. No cooling can be realized with this dipole force, however if the atoms are cold enough initially, they may be trapped i…

Condensed Matter::Quantum GasesPhysicsOptical latticeDipoleUltracold atomTransition dipole momentSpontaneous emissionPhysics::Atomic PhysicsElectronElectric dipole transitionAtomic physicsMagnetic dipole
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A self-consistent 2-D model for the dip angle ofmantle downflow beneath an overriding continent

1999

Abstract We demonstrate how the inclination of descending mantle flow is affected by thepresence of a continent overriding the downwelling zone. The mantle is modelled by a fluidhaving a temperature- and pressure-dependent viscosity which describes a low viscosityasthenosphere and a higher viscosity lower mantle. The fluid occupies a square x:y=10:1 boxheated from below. In the absence of overlying continents thermal convection sets in with colddownwellings being nearly vertical. A continent is placed on the convecting mantle and starts todrift. The continent is assumed to be a thick rigid plate. We consider models of two types. Model1 involves a free-floating continent. The continent is pu…

ConvectionViscosityGeophysicsConvective heat transfer2 d modelDownwellingMagnetic dipGeophysicsSelf consistentMantle (geology)GeologyEarth-Surface ProcessesJournal of Geodynamics
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Lateral indirect exchange coupling in a two-dimensional nanostripe array

2002

We observe a lateral indirect exchange coupling in a multistripe system of parallel Fe nanostripes grown by self-organized growth on a vicinal single-crystal W(110) surface. The width and the distance between the stripes of monolayer height were modified via the total amount of deposited Fe. The easy axis of the magnetization lies perpendicular to the stripe edges and in the surface plane, thus resulting in a ferromagnetic dipolar coupling. In addition to the dipolar coupling we observe an antiferromagnetic indirect exchange coupling for the nanostripe system covered by Au. The coupling causes a superferromagnetic phase transition in the nanostripe array.

CouplingMagnetizationPhase transitionMagnetic anisotropyMaterials scienceFerromagnetismCondensed matter physicsAntiferromagnetismVicinalMagnetic dipole–dipole interactionPhysical Review B
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