Search results for "BAND"

showing 10 items of 2610 documents

Spontaneous magnetism of quantum dot lattices.

2003

The magnetism of square lattices of quantum dots with up to 12 electrons per dot is studied using the spin-density functional formalism. At small values of the lattice constant, all lattices are nonmagnetic and gapless. When the lattice constant is increased, the shell structure of the single dots governs the magnetism of the lattice. At closed shells, the lattices are nonmagnetic and have a gap at the Fermi level. At the beginning and at the end of a shell, they become ferromagnetic and stay gapless up to large values of the lattice constant. Antiferromagnetism was observed only at midshell after a band gap was opened.

PhysicsCondensed matter physicsMagnetismBand gapHigh Energy Physics::LatticeFermi levelGeneral Physics and AstronomyCondensed Matter::Mesoscopic Systems and Quantum Hall Effectsymbols.namesakeLattice constantFerromagnetismQuantum dotLattice (order)symbolsAntiferromagnetismCondensed Matter::Strongly Correlated ElectronsPhysical review letters
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Electronic structure calculations forZnFe2O4

2011

Local density approximation was applied to scrutinize the electronic structure and magnetic properties of the spinel ferrite ${\mathrm{ZnFe}}_{2}{\mathrm{O}}_{4}$. Various cation distributions were established to obtain the ground state for the system. In magnetic crystals, the position of the atoms is not enough for symmetry determination. A structure prediction by decreasing the octahedral point group symmetry ${\mathrm{O}}_{h}$ of Fe to ${\mathrm{D}}_{4h}$, ${\mathrm{C}}_{4v}$, and ${\mathrm{C}}_{3v}$ was carried out. The effect of the exchange and correlation terms on the band structure of ${\mathrm{ZnFe}}_{2}{\mathrm{O}}_{4}$ was studied by the generalized gradient approximation $+$ th…

PhysicsCondensed matter physicsOctahedral symmetryElectronic structureMagnetic semiconductorSymmetry (geometry)Local-density approximationCondensed Matter PhysicsGround stateElectronic band structureElectronic Optical and Magnetic MaterialsSpin-½Physical Review B
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Phonon Bandwidth and Rate Equations in Avalanche Relaxation

1973

PhysicsCondensed matter physicsPhononQuantum mechanicsBandwidth (signal processing)Rate equationPhysical Review B
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Electronic structure studies ofBaFe2As2by angle-resolved photoemission spectroscopy

2009

We report high resolution angle-resolved photoemission spectroscopy (ARPES) studies of the electronic structure of ${\text{BaFe}}_{2}{\text{As}}_{2}$, which is one of the parent compounds of the Fe-pnictide superconductors. ARPES measurements have been performed at 20 and 300 K, corresponding to the orthorhombic antiferromagnetic phase and the tetragonal paramagnetic phase, respectively. Photon energies between 30 and 175 eV and polarizations parallel and perpendicular to the scattering plane have been used. Measurements of the Fermi surface yield two hole pockets at the $\ensuremath{\Gamma}$ point and an electron pocket at each of the $X$ points. The topology of the pockets has been conclu…

PhysicsCondensed matter physicsPhotoemission spectroscopyInverse photoemission spectroscopyFermi levelAngle-resolved photoemission spectroscopyFermi surfaceElectronic structureCondensed Matter PhysicsElectronic Optical and Magnetic Materialssymbols.namesakeCondensed Matter::SuperconductivitysymbolsCondensed Matter::Strongly Correlated ElectronsElectronic band structurePseudogapPhysical Review B
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Pairing based cooling of Fermi gases

2007

We propose a pairing-based method for cooling an atomic Fermi gas. A three component (labels 1, 2, 3) mixture of Fermions is considered where the components 1 and 2 interact and, for instance, form pairs whereas the component 3 is in the normal state. For cooling, the components 2 and 3 are coupled by an electromagnetic field. Since the quasiparticle distributions in the paired and in the normal states are different, the coupling leads to cooling of the normal state even when initially $T_{paired}\geq T_{normal}$ (notation $T_S\geq T_N$). The cooling efficiency is given by the pairing energy and by the linewidth of the coupling field. No superfluidity is required: any type of pairing, or ot…

PhysicsCondensed matter physicsResolved sideband coolingCondensed Matter - SuperconductivityFOS: Physical sciencesCoupling (probability)7. Clean energy01 natural sciencesAtomic and Molecular Physics and Optics010305 fluids & plasmasSuperconductivity (cond-mat.supr-con)Condensed Matter - Other Condensed MatterLaser coolingPairing0103 physical sciencesQuasiparticleAtomic physicsConnection (algebraic framework)010306 general physicsFermi gasEnergy (signal processing)Other Condensed Matter (cond-mat.other)
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Optical studies of gap, hopping energies, and the Anderson-Hubbard parameter in the zigzag-chain compoundSrCuO2

2001

We have investigated the electronic structure of the zig-zag ladder (chain) compound ${\mathrm{SrCuO}}_{2}$ combining polarized optical absorption, reflection, photoreflectance, and pseudo-dielectric-function measurements with the model calculations. These measurements yield an energy gap of 1.42 eV (1.77 eV) at 300 K along (perpendicular to) the Cu-O chains. We have found that the lowest-energy gap, the correlation gap, is temperature independent. The electronic structure of this oxide is calculated using both the local-spin-density approximation with gradient correction method and the tight-binding theory for the correlated electrons. The calculated density of electronic states for noncor…

PhysicsCondensed matter physicsZigzagComputer Science::Systems and ControlBand gapCondensed Matter::Strongly Correlated ElectronsStrongly correlated materialAbsorption (logic)ElectronElectronic structureAtomic physicsElectronic band structureSpin-½Physical Review B
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Role of dispersion on zero-average-index bandgaps

2009

We consider periodic multilayers combining ordinary positive index materials and dispersive metamaterials with negative index in some frequency ranges. These structures can exhibit photonic bandgaps which, in contrast with the usual Bragg gaps, are not based on interference mechanisms. Changing the dispersion models for the constituent metamaterial, we investigate its role in the production of zero-average-index bandgaps. In particular, we show the effect of each constitutive parameter on both bandgap edges. Finally, we give some approximated analytical expressions in terms of average parameters for the determination of the upper and lower limits of the zero-average refractive-index bandgap…

PhysicsCondensed matter physicsbusiness.industryWave propagationBand gapCiencias FísicasPHOTONIC CRYSTALSPhysics::OpticsMetamaterialStatistical and Nonlinear PhysicsInterference (wave propagation)Atomic and Molecular Physics and OpticsNEGATIVE INDEXAstronomíaCondensed Matter::Materials ScienceOpticsPHOTONIC BAND GAPNegative refractionDispersion (optics)MULTILAYERSPhotonicsbusinessRefractive indexCIENCIAS NATURALES Y EXACTAS
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Structure of the Accretion Disk in the Lensed Quasar Q2237+0305 from Multi-Epoch and Multi-Wavelength Narrow Band Photometry

2015

We present estimates for the size and the logarithmic slope of the disk temperature profile of the lensed quasar Q2237+0305, independent of the component velocities. These estimates are based on six epochs of multi-wavelength narrowband images from the Nordic Optical Telescope. For each pair of lensed images and each photometric band, we determine the microlensing amplitude and chromaticity using pre-existing mid-IR photometry to define the baseline for no microlensing magnification. A statistical comparison of the combined microlensing data (6 epochs $\times$ 5 narrow bands $\times$ 6 image pairs) with simulations based on microlensing magnification maps gives Bayesian estimates for the ha…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010504 meteorology & atmospheric sciencesFOS: Physical sciencesAstronomy and AstrophysicsQuasarMulti wavelengthAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Astrophysics of Galaxies01 natural sciencesAccretion (astrophysics)NarrowbandAccretion discSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic Astrophysics0105 earth and related environmental sciences
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The evolution of the rest-frame J- and H-band luminosity function of galaxies to z=3.5

2011

We present the rest-frame J- and H-band luminosity function (LF) of field galaxies, based on a deep multi-wavelength composite sample from the MUSYC, FIRES and FIREWORKS survey public catalogues, covering a total area of 450 arcmin^2. The availability of flux measurements in the Spitzer IRAC 3.6, 4.5, 5.8, and 8 um channels allows us to compute absolute magnitudes in the rest-frame J and H bands up to z=3.5 minimizing the dependence on the stellar evolution models. We compute the LF in the four redshift bins 1.5<z<2.0, 2.0<z<2.5, 2.5<z<3.0 and 3.0<z<3.5. Combining our results with those already available at lower redshifts, we find that (1) the faint end slope is consistent with being const…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FluxFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsH bandJ bandRedshiftGalaxyLuminositySpace and Planetary ScienceStellar evolutionAstrophysics - Cosmology and Nongalactic AstrophysicsLuminosity function (astronomy)
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Unraveling exciton dynamics in amorphous silicon dioxide: Interpretation of the optical features from 8 to 11 eV.

2011

Physical review / B 83, 174201 (2011). doi:10.1103/PhysRevB.83.174201

PhysicsCoupling constantAbsorption spectroscopyPhononExcitonSettore FIS/01 - Fisica SperimentaleQuantum yieldCondensed Matter Physics530Exciton dynamicElectronic Optical and Magnetic MaterialsCondensed Matter::Materials ScienceDelocalized electronamorphous silicon dioxideLattice (order)ddc:530absorption and reflectivity spectraAtomic physicsElectronic band structure
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