Search results for "Hub"

showing 10 items of 207 documents

Observational constraints on the LLTB model

2010

We directly compare the concordance LCDM model to the inhomogeneous matter-only alternative represented by LTB void models. To achieve a "democratic" confrontation we explore LLTB models with non-vanishing cosmological constant and perform a global likelihood analysis in the parameter space of cosmological constant and void radius. In our analysis we carefully consider SNe, Hubble constant, CMB and BAO measurements, marginalizing over spectral index, age of the universe and background curvature. We find that the LCDM model is not the only possibility compatible with the observations, and that a matter-only void model is a viable alternative to the concordance model only if the BAO constrain…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Age of the universeFOS: Physical sciencesAstronomy and AstrophysicsLambda-CDM modelCosmological constantAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyMetric expansion of spaceLocal Voidsymbols.namesakesymbolsDark energyBaryon acoustic oscillationsStatistical physicsAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's law
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Constraints on cosmological models from strong gravitational lensing systems

2012

Strong lensing has developed into an important astrophysical tool for probing both cosmology and galaxies (their structure, formation, and evolution). Using the gravitational lensing theory and cluster mass distribution model, we try to collect a relatively complete observational data concerning the Hubble constant independent ratio between two angular diameter distances $D_{ds}/D_s$ from various large systematic gravitational lens surveys and lensing by galaxy clusters combined with X-ray observations, and check the possibility to use it in the future as complementary to other cosmological probes. On one hand, strongly gravitationally lensed quasar-galaxy systems create such a new opportun…

PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Strong gravitational lensingFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsCosmologyRedshiftEinstein radiussymbols.namesakeGravitational lenssymbolsDark energyGalaxy clusterAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's lawJournal of Cosmology and Astroparticle Physics
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Ferromagnetism of the Hubbard Model at Strong Coupling in the Hartree-Fock Approximation

2005

As a contribution to the study of Hartree-Fock theory we prove rigorously that the Hartree-Fock approximation to the ground state of the d-dimensional Hubbard model leads to saturated ferromagnetism when the particle density (more precisely, the chemical potential mu) is small and the coupling constant U is large, but finite. This ferromagnetism contradicts the known fact that there is no magnetization at low density, for any U, and thus shows that HF theory is wrong in this case. As in the usual Hartree-Fock theory we restrict attention to Slater determinants that are eigenvectors of the z-component of the total spin, {S}_z = sum_x n_{x,\uparrow} - n_{x,\downarrow}, and we find that the ch…

PhysicsCoupling constantHubbard modelCondensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)Statistical Mechanics (cond-mat.stat-mech)Nuclear TheoryHartree–Fock methodFOS: Physical sciencesStatistical and Nonlinear PhysicsMathematical Physics (math-ph)Condensed Matter - Strongly Correlated ElectronsFerromagnetismSlater determinantCondensed Matter::Strongly Correlated ElectronsGround stateEnergy (signal processing)Condensed Matter - Statistical MechanicsMathematical PhysicsSpin-½
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Dynamical mean-field theory calculation with the dynamical density-matrix renormalization group

2006

Abstract We study the Hubbard model at half band-filling on a Bethe lattice with infinite coordination number at zero temperature. We use the dynamical mean-field theory (DMFT) mapping to a single-impurity Anderson model with a bath whose properties have to be determined self-consistently. For a controlled and systematic implementation of the self-consistency scheme we use the fixed-energy approach to the DMFT. Using the dynamical density–matrix renormalization group method (DDMRG) we calculate the density of states (DOS) with a resolution ranging from 3% of the bare bandwidth W = 4 t at high energies to 0.01% for the quasi-particle peak. The DDMRG resolution and accuracy for the DOS is sup…

PhysicsDensity matrixHubbard modelBethe latticeDensity matrix renormalization groupNumerical analysisRenormalization groupCondensed Matter Physics01 natural sciences010305 fluids & plasmasElectronic Optical and Magnetic MaterialsQuantum electrodynamics0103 physical sciencesDensity of statesCondensed Matter::Strongly Correlated ElectronsElectrical and Electronic Engineering010306 general physicsAnderson impurity modelMathematical physicsPhysica B: Condensed Matter
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Hole-doped Hubbard ladders

2005

The formation of stripes in six-leg Hubbard ladders with cylindrical boundary conditions is investigated for two different hole dopings, where the amplitude of the hole density modulation is determined in the limits of vanishing DMRG truncation errors and infinitely long ladders. The results give strong evidence that stripes exist in the ground state of these systems for strong but not for weak Hubbard couplings. The doping dependence of these findings is analysed.

PhysicsDensity matrixStrongly Correlated Electrons (cond-mat.str-el)Hubbard modelCondensed matter physicsDopingFOS: Physical sciencesCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsCondensed Matter - Strongly Correlated ElectronsAmplitudeCharge-carrier densityCondensed Matter::SuperconductivityQuantum mechanicsModulation (music)Condensed Matter::Strongly Correlated ElectronsBoundary value problemElectrical and Electronic EngineeringGround statePhysica B: Condensed Matter
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Spectral Function of the One-Dimensional Hubbard Model away from Half Filling

2004

We calculate the photoemission spectral function of the one-dimensional Hubbard model away from half filling using the dynamical density matrix renormalization group method. An approach for calculating momentum-dependent quantities in finite open chains is presented. Comparison with exact Bethe Ansatz results demonstrates the unprecedented accuracy of our method. Our results show that the photoemission spectrum of the quasi-one-dimensional conductor TTF-TCNQ provides evidence for spin-charge separation on the scale of the conduction band width.

PhysicsDensity matrixStrongly Correlated Electrons (cond-mat.str-el)Hubbard modelFOS: Physical sciencesGeneral Physics and AstronomyRenormalization groupThermal conductionSpinonBethe ansatzConductorCondensed Matter - Strongly Correlated ElectronsLuttinger liquidQuantum electrodynamicsQuantum mechanicsCondensed Matter::Strongly Correlated ElectronsPhysical Review Letters
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Landau Fermi Liquid Theory and Beyond

2014

In this chapter we consider the Landau theory of the Fermi liquid that has a long history and remarkable results in describing a numerous properties of the electron liquid in ordinary metals and Fermi liquids of the \(^3\)He type. The theory is based on the assumption that elementary excitations determine the physics at low temperatures, resembling that of weakly interacting Fermi gas. These excitations behave as quasiparticles with a certain effective mass. The effective mass \(M^*\) exhibits a simple universal behavior, for it is independent of the temperature, pressure, and magnetic field strength and is a parameter of the theory. Microscopically deriving the equation determining the eff…

PhysicsEffective mass (solid-state physics)Condensed matter physicsElectron liquidQuantum oscillationsFermi liquid theoryLandau quantizationFermi gasShubnikov–de Haas effectLandau theory
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Orbital-selective Mott transitions in a doped two-band Hubbard model with crystal field splitting

2013

We investigate the effects of crystal field splitting in a doped two-band Hubbard model with different bandwidths within dynamical mean-field theory (DMFT), using a quantum Monte Carlo impurity solver. In addition to an orbital-selective Mott phase (OSMP) of the narrow band, which is adiabatically connected with the well-studied OSMP in the half-filled case without crystal field splitting, we find, for sufficiently strong interaction and a suitable crystal field, also an OSMP of the wide band. We establish the phase diagram (in the absence of magnetic or orbital order) at moderate doping as a function of interaction strength and crystal field splitting and show that also the wide-band OSMP …

PhysicsField (physics)Hubbard modelCondensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)Quantum Monte CarloFOS: Physical sciencesCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsCrystalCondensed Matter - Strongly Correlated ElectronsCrystal field theoryStrongly correlated materialCondensed Matter::Strongly Correlated ElectronsSpin (physics)Phase diagram
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Spin and charge orderings in the atomic limit of the U-V-J model

2011

In this paper we study a generalization of the 1D Hubbard model by considering density-density and Ising-type spin-spin nearest neighbor (NN) interactions, parameterized by $V$ and $J$, respectively. We present the T=0 phase diagram for both ferro ($J>0$) and anti-ferro ($J<0$) coupling obtained in the narrow-band limit by means of an extension to zero-temperature of the transfer-matrix method. Based on the values of the Hamiltonian parameters, we identify a number of phases that involve orderings of the double occupancy, NN density and spin correlations, being these latter very fragile.

PhysicsHistoryHubbard modelStrongly Correlated Electrons (cond-mat.str-el)Condensed Matter - SuperconductivityParameterized complexityFOS: Physical sciencesComputer Science ApplicationsEducationk-nearest neighbors algorithmSuperconductivity (cond-mat.supr-con)symbols.namesakeCondensed Matter - Strongly Correlated ElectronssymbolsCondensed Matter::Strongly Correlated ElectronsHamiltonian (quantum mechanics)Mathematical physicsPhase diagram
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Deciding the fate of the false Mott transition in two dimensions by exact quantum Monte Carlo methods

2015

We present an algorithm for the computation of unbiased Green functions and self-energies for quantum lattice models, free from systematic errors and valid in the thermodynamic limit. The method combines direct lattice simulations using the Blankenbecler Scalapino-Sugar quantum Monte Carlo (BSS-QMC) approach with controlled multigrid extrapolation techniques. We show that the half-filled Hubbard model is insulating at low temperatures even in the weak-coupling regime; the previously claimed Mott transition at intermediate coupling does not exist.

PhysicsHistoryHubbard modelStrongly Correlated Electrons (cond-mat.str-el)Quantum Monte CarloComputationExtrapolationFOS: Physical sciencesComputer Science ApplicationsEducationMott transitionCondensed Matter - Strongly Correlated ElectronsMultigrid methodThermodynamic limitCondensed Matter::Strongly Correlated ElectronsStatistical physicsQuantum
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