Search results for "Hub"

showing 10 items of 207 documents

Emulating the one-dimensional Fermi-Hubbard model by a double chain of qubits

2016

The Jordan-Wigner transformation maps a one-dimensional spin-1/2 system onto a fermionic model without spin degree of freedom. A double chain of quantum bits with XX and ZZ couplings of neighboring qubits along and between the chains, respectively, can be mapped on a spin-full 1D Fermi-Hubbard model. The qubit system can thus be used to emulate the quantum properties of this model. We analyze physical implementations of such analog quantum simulators, including one based on transmon qubits, where the ZZ interaction arises due to an inductive coupling and the XX interaction due to a capacitive interaction. We propose protocols to gain confidence in the results of the simulation through measu…

PhysicsQuantum PhysicsHubbard modelCondensed Matter - Mesoscale and Nanoscale PhysicsCondensed Matter - SuperconductivityQuantum simulatorFOS: Physical sciences02 engineering and technologyTransmon021001 nanoscience & nanotechnology01 natural sciencesInductive couplingSuperconductivity (cond-mat.supr-con)Quantum mechanicsQubit0103 physical sciencesMesoscale and Nanoscale Physics (cond-mat.mes-hall)010306 general physics0210 nano-technologySuperconducting quantum computingQuantum Physics (quant-ph)QuantumSpin-½
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QUANTUM SPIN CHAINS WITH COMPOSITE SPIN

1988

The ground state of quantum spin chains with two spin-1/2 operators per site is determined from finite chain calculations and compared to predictions from the continuum limit. As particular cases, results for the spin-1 Heisenberg chain, the spin-1 model with bilinear and biquadratic exchange and the extended Hubbard model are analysed.

PhysicsQuantum spin chainsContinuum (measurement)Condensed matter physicsHubbard modelQuantum mechanicsComposite numberGeneral EngineeringBilinear interpolationCondensed Matter::Strongly Correlated ElectronsGround stateLe Journal de Physique Colloques
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Distance of matter inside an Einstein-Strauss vacuole

2008

PhysicsSolar masssymbols.namesakeGeodesics in general relativitysymbolsVacuoleAstrophysicsEinsteinGalaxy clusterHubble's law
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All good things come in threes: the third image of the lensed quasar PKS1830-211

2020

Strong gravitational lensing distorts our view of sources at cosmological distances but brings invaluable constraints on the mass content of foreground objects and on the geometry and properties of the Universe. We report the detection of a third continuum source toward the strongly lensed quasar PKS1830-211 in ALMA multi-frequency observations of high dynamic range and high angular resolution. This third source is point-like and located slightly to the north of the diagonal joining the two main lensed images, A and B, 0.3 arcsec away from image B. It has a flux density that is ~140 times weaker than images A and B and a similar spectral index, compatible with synchrotron emission. We concl…

PhysicsSpectral indexCosmology and Nongalactic Astrophysics (astro-ph.CO)Einstein ring010308 nuclear & particles physicsContinuum (design consultancy)Strong gravitational lensingFOS: Physical sciencesAstronomy and AstrophysicsQuasarAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics - Astrophysics of Galaxies01 natural sciencessymbols.namesakeSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)0103 physical sciencessymbolsMillimeterAngular resolution010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsAstrophysics - Cosmology and Nongalactic AstrophysicsHubble's law
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Relic neutrinos, thermal axions, and cosmology in early 2014

2014

We present up to date cosmological bounds on the sum of active neutrino masses as well as on extended cosmological scenarios with additional thermal relics, as thermal axions or sterile neutrino species. Our analyses consider all the current available cosmological data in the beginning of year 2014, including the very recent and most precise Baryon Acoustic Oscillation (BAO) measurements from the Baryon Oscillation Spectroscopic Survey. In the minimal three active neutrino scenario, we find Sum m_nu < 0.22 eV at 95% CL from the combination of CMB, BAO and Hubble Space Telescope measurements of the Hubble constant. A non zero value for the sum of the three active neutrino masses of about …

PhysicsSterile neutrinoParticle physicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundHigh Energy Physics::PhenomenologyCosmic background radiationFOS: Physical sciencesFísicaAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energyOmegaBaryonsymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)13. Climate actionsymbolsAstronomiaNeutrinoAxionHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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Cosmological limits on neutrino unknowns versus low redshift priors

2015

Recent Cosmic Microwave Background (CMB) temperature and polarization anisotropy measurements from the Planck mission have significantly improved previous constraints on the neutrino masses as well as the bounds on extended models with massless or massive sterile neutrino states. However, due to parameter degeneracies, additional low redshift priors are mandatory in order to sharpen the CMB neutrino bounds. We explore here the role of different priors on low redshift quantities, such as the Hubble constant, the cluster mass bias, and the reionization optical depth $\tau$. Concerning current priors on the Hubble constant and the cluster mass bias, the bounds on the neutrino parameters may di…

PhysicsSterile neutrinoParticle physicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)010308 nuclear & particles physicsCosmic microwave backgroundFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRedshiftMassless particlesymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencessymbolsPlanckNeutrino010303 astronomy & astrophysicsReionizationHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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Dynamical Density-Matrix Renormalization Group for the Mott--Hubbard insulator in high dimensions

2004

We study the Hubbard model at half band-filling on a Bethe lattice with infinite coordination number in the paramagnetic insulating phase 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 (FE) approach to the DMFT. In FE-DMFT the onset and the width of the Hubbard bands are adjusted self-consistently but the energies of the bath levels are kept fixed relatively to both band edges during the calculation of self-consistent hybridization strengths between impurity …

PhysicsStrongly Correlated Electrons (cond-mat.str-el)Condensed matter physicsBethe latticeHubbard modelDensity matrix renormalization groupCoordination numberFOS: Physical sciencesRenormalization groupCondensed Matter PhysicsParamagnetismCondensed Matter - Strongly Correlated ElectronsDensity of statesGeneral Materials ScienceCondensed Matter::Strongly Correlated ElectronsAnderson impurity model
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The Hubbard model beyond the two-pole approximation: a Composite Operator Method study

2014

Within the framework of the Composite Operator Method, a three-pole solution for the two-dimensional Hubbard model is presented and analyzed in detail. In addition to the two Hubbard operators, the operatorial basis comprises a third operator describing electronic transitions dressed by nearest-neighbor spin fluctuations. These latter, compared to charge and pair fluctuations, are assumed to be preeminent in the region of model-parameter space - small doping, low temperature and large on-site Coulomb repulsion - where one expects strong electronic correlations to dominate the physics of the system. This assumption and the consequent choice for the basic field, as well as the whole analytica…

PhysicsStrongly Correlated Electrons (cond-mat.str-el)Field (physics)Hubbard modelBasis (linear algebra)Numerical analysisCondensed Matter - SuperconductivityCrossoverFOS: Physical sciencesCharge (physics)Solid State and MaterialsCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsSuperconductivity (cond-mat.supr-con)Condensed Matter - Strongly Correlated ElectronsOperator (computer programming)Solid State and Materials;Statistical physicsSpin-½
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Magnetic properties of a strongly correlated system on the Bethe lattice

2010

We study the influence of an external magnetic field h on the phase diagram of a system of Fermi particles living on the sites of a Bethe lattice with coordination number z and interacting through on-site U and nearest-neighbor V interactions. This is a physical realization of the extended Hubbard model in the narrow-band limit. Our results establish that the magnetic field may dramatically affect the critical temperature below which a long-range charge ordered phase is observed, as well as the behavior of physical quantities, inducing, for instance, magnetization plateaus in the magnetization curves. Relevant thermodynamic quantities - such as the specific heat and the susceptibility - are…

PhysicsStrongly Correlated Electrons (cond-mat.str-el)Hubbard modelBethe latticeCondensed matter physicsFOS: Physical sciencesGeneral Physics and AstronomyCharge (physics)Magnetic fieldCondensed Matter - Strongly Correlated ElectronsMagnetizationPhase (matter)Phase diagramPhysical quantityJournal of Physical Studies
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Fourth-order perturbation theory for the half-filled Hubbard model in infinite dimensions

2003

We calculate the zero-temperature self-energy to fourth-order perturbation theory in the Hubbard interaction $U$ for the half-filled Hubbard model in infinite dimensions. For the Bethe lattice with bare bandwidth $W$, we compare our perturbative results for the self-energy, the single-particle density of states, and the momentum distribution to those from approximate analytical and numerical studies of the model. Results for the density of states from perturbation theory at $U/W=0.4$ agree very well with those from the Dynamical Mean-Field Theory treated with the Fixed-Energy Exact Diagonalization and with the Dynamical Density-Matrix Renormalization Group. In contrast, our results reveal t…

PhysicsStrongly Correlated Electrons (cond-mat.str-el)Hubbard modelBethe latticeFOS: Physical sciencesRenormalization groupCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsCondensed Matter - Strongly Correlated ElectronsFourth orderIterated functionQuasiparticleDensity of statesCondensed Matter::Strongly Correlated ElectronsPerturbation theory (quantum mechanics)Mathematical physicsThe European Physical Journal B - Condensed Matter
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