Search results for "530"

showing 10 items of 1476 documents

Ultracold atomic Bose and Fermi spinor gases in optical lattices

2006

We investigate magnetic properties of Mott-insulating phases of ultracold Bose and Fermi spinor gases in optical lattices. We consider in particular the F=2 Bose gas, and the F=3/2 and F=5/2 Fermi gases. We derive effective spin Hamiltonians for one and two atoms per site and discuss the possibilities of manipulating the magnetic properties of the system using optical Feshbach resonances. We discuss low temperature quantum phases of a 87Rb gas in the F=2 hyperfine state, as well as possible realizations of high spin Fermi gases with either 6Li or 132Cs atoms in the F=3/2 state, and with 173Yb atoms in the F=5/2 state.

Condensed Matter::Quantum GasesPhysicseinstein condensationSpinorBose gasCondensed matter physicsFOS: Physical sciencesGeneral Physics and Astronomyresonant lightQuantum phasesState (functional analysis)quantum phasesCondensed Matter - Other Condensed Matterground-statesone bosonssystemsddc:530Condensed Matter::Strongly Correlated ElectronsantiferromagnetsDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikHyperfine structureOther Condensed Matter (cond-mat.other)Spin-½Fermi Gamma-ray Space TelescopeNew Journal of Physics
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Simulating quantum-optical phenomena with cold atoms in optical lattices

2010

We propose a scheme involving cold atoms trapped in optical lattices to observe different phenomena traditionally linked to quantum-optical systems. The basic idea consists of connecting the trapped atomic state to a non-trapped state through a Raman scheme. The coupling between these two types of atoms (trapped and free) turns out to be similar to that describing light–matter interaction within the rotating-wave approximation, the role of matter and photons being played by the trapped and free atoms, respectively. We explain in particular how to observe phenomena arising from the collective spontaneous emission of atomic and harmonic oscillator samples, such as superradiance and directiona…

Condensed Matter::Quantum GasesQuantum PhysicsQuantum opticsDDC 530 / PhysicsFísicaFOS: Physical sciencesddc:530Physics::Atomic PhysicsQuantum Physics (quant-ph)Quantenoptik
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Focus on atom optics and its applications

2010

Atom optics employs the modern techniques of quantum optics and laser cooling to enable applications which often outperform current standard technologies. Atomic matter wave interferometers allow for ultra-precise sensors; metrology and clocks are pushed to an extraordinary accuracy of 17 digits using single atoms. Miniaturization and integration are driven forward for both atomic clocks and atom optical circuits. With the miniaturization of information-storage and -processing devices, the scale of single atoms is approached in solid state devices, where the laws of quantum physics lead to novel, advantageous features and functionalities. An upcoming branch of atom optics is the control of …

Condensed Matter::Quantum GasesQuantum opticsPhysicsQuantum opticsDDC 530 / PhysicsGeneral Physics and AstronomyAtomic clockIonLaser coolingAtomPhysics::Atomic and Molecular ClustersAtom opticsMiniaturizationddc:530Physics::Atomic PhysicsMatter waveAtomic physicsQuantenoptik
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Colloidal layers in magnetic fields and under shear flow

2005

The behaviour of colloidal mono- and bilayers in external magnetic fields and under shear is discussed and recent progress is summarized. Superparamagnetic colloidal particles form monolayers when they are confined to a air–water interface in a hanging water droplet. An external magnetic field allows us to tune the strength of the mutual dipole–dipole interaction between the colloids and the anisotropy of the interaction can be controlled by the tilt angle of the magnetic field relative to the surface normal of the air–water interface. For sufficiently large magnetic field strength crystalline monolayers are found. The role of fluctuations in these two-dimensional crystals is discussed. Fur…

Condensed matter physicsChemistryEmulsions and suspensionsColloidal crystalCondensed Matter PhysicsSolid-liquid transitionsMagnetic fieldCondensed Matter::Soft Condensed MatterColloidShear (geology)MonolayerGeneral Materials Scienceddc:530Colloidspacs:82.70.Dd 64.70.D 82.70.KjAnisotropyShear flowSuperparamagnetism
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Nature of the non-exponential primary relaxation in structural glass-formers probed by dynamically selective experiments

1998

Several experimental methods feature the potential to distinguish between slow and fast contributions to the non-exponential, ensemble averaged primary response in glass-forming materials. Some of these techniques are based on the selection of subensembles using multi-dimensional nuclear magnetic resonance, optical bleaching, and non-resonant spectral hole burning. Others, such as the time-dependent solvation spectroscopy, measure microscopic responses induced by local perturbations. Using several of these methods it could be demonstrated for various glass-forming materials that the non-exponential relaxation results from a superposition of dynamically distinguishable entities. The experime…

Condensed matter physicsChemistrySolvationCondensed Matter Physics530Measure (mathematics)Electronic Optical and Magnetic MaterialsExponential functionSuperposition principleChemical physicsMaterials ChemistryCeramics and CompositesSpectral hole burningRelaxation (physics)Experimental methodsSpectroscopyJournal of Non-Crystalline Solids
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La disputa fronteriza entre India y China: origen y evolución de la controversia

2008

Con la emergencia de la India independiente y de la China maoísta a mediados del siglo pasado, los dos nuevos gobiernos de Delhi y Pekín comenzaron a convivir en un marco de armonía bajo los principios de coexistencia pacífica y una política de hermandad entre ambos pueblos, conocida como Hindi-Chini Bhai Bhai. Sin embargo, a pesar de estas actitudes amistosas iniciales, la herencia colonial británica en la India y las consecuencias de la anexión china del territorio tibetano, vinieron a desestabilizar este equilibrio, con el enfrentamiento de las pretensiones soberanistas de ambos Estados emergentes sobre distintas zonas fronterizas.El análisis del origen y la evolución de la controvertida…

Conflict in the Himalayas:CIENCIA POLÍTICA::Relaciones internacionales ::Problemas de las relaciones internacionales [UNESCO]UNESCO::CIENCIA POLÍTICA::Relaciones internacionales ::Problemas de las relaciones internacionalesconflicto armadolcsh:International relationsIndialcsh:Political sciencelcsh:K1-7720Convenció de Shimlaacuerdos amistososConflicto fronterizo: China; IndiaLínea Mc Mahonlcsh:Law in general. Comparative and uniform law. JurisprudenceConflicto en los HimalayasAcuerdo Panchsheelmutual agreementShimla ConventionChina [Conflicto fronterizo]Mc Mahon Linearmed conflictlcsh:Jlcsh:JZ2-6530Panchsheel Agreement
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The influence of absorbed solar radiation by Saharan dust on hurricane genesis

2015

To date, the radiative impact of dust and the Sahar an air layer (SAL) on North Atlantic hurricane activity is not yet known. According to previous studies, dust stabilizes the atmosphere due to absorption of solar radiation but thus shifts convection to regions more conducive for hurricane genesis. Here we analyze differences in hurricane genesis and frequency from ensemble sensitivity simulations with radiatively active and inactive dust in the aerosol-climate model ECHAM6-HAM. We investigate dust burden and other hurricane-related variables and determine their influence on disturbances which develop into hurricanes (developing disturbances, DDs) and those which do not (nondeveloping dist…

ConvectionSaharan Air LayerAtmospheric ScienceAtlantic hurricane530 PhysicsMineral dustAtmospheric sciencescomplex mixturesrespiratory tract diseasesAtmosphereGeophysicsSpace and Planetary ScienceClimatologyEarth and Planetary Sciences (miscellaneous)Radiative transferEnvironmental scienceClimate modelTropical cyclone550 Earth sciences & geology
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Search for topological defect dark matter with a global network of optical magnetometers

2021

Ultralight bosons such as axion-like particles are viable candidates for dark matter. They can form stable, macroscopic field configurations in the form of topological defects that could concentrate the dark matter density into many distinct, compact spatial regions that are small compared with the Galaxy but much larger than the Earth. Here we report the results of the search for transient signals from the domain walls of axion-like particles by using the global network of optical magnetometers for exotic (GNOME) physics searches. We search the data, consisting of correlated measurements from optical atomic magnetometers located in laboratories all over the world, for patterns of signals p…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsAtomic Physics (physics.atom-ph)Particle physicsGeneral Physics and AstronomyFOS: Physical sciences53001 natural sciencesArticleHigh Energy Physics - ExperimentPhysics - Atomic PhysicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesDark energy and dark matterddc:530Atomic and molecular physics010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Characteristics of the diffuse astrophysical electron and Tau neutrino flux with six years of IceCube high energy cascade data

2020

We report on the first measurement of the astrophysical neutrino flux using particle showers (cascades) in IceCube data from 2010-2015. Assuming standard oscillations, the astrophysical neutrinos in this dedicated cascade sample are dominated (∼90%) by electron and tau flavors. The flux, observed in the sensitive energy range from 16 TeV to 2.6 PeV, is consistent with a single power-law model as expected from Fermi-type acceleration of high energy particles at astrophysical sources. We find the flux spectral index to be γ=2.53±0.07 and a flux normalization for each neutrino flavor of φastro=1.66-0.27+0.25 at E0=100 TeV, in agreement with IceCube's complementary muon neutrino results and wit…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyElectronpower spectrumflux [electron]energy [particle]01 natural sciencesIceCubeNuclear physics5/3Tau neutrinomuon0103 physical scienceslow [energy]Muon neutrinoddc:530010303 astronomy & astrophysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMSpectral indexMuon010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyflavor [neutrino]RAYSflux [neutrino]accelerationshowersoscillationPhysics and Astronomy13. Climate actionEnergy cascadePhysique des particules élémentairesastro-ph.COhigh [energy]cascade [energy]High Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space TelescopeAstrophysics - Cosmology and Nongalactic Astrophysics
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Stochastic fluctuations of bosonic dark matter

2021

Numerous theories extending beyond the standard model of particle physics predict the existence of bosons that could constitute the dark matter (DM) permeating the universe. In the standard halo model (SHM) of galactic dark matter the velocity distribution of the bosonic DM field defines a characteristic coherence time $\tau_c$. Until recently, laboratory experiments searching for bosonic DM fields have been in the regime where the measurement time $T$ significantly exceeds $\tau_c$, so null results have been interpreted as constraints on the coupling of bosonic DM to standard model particles with a bosonic DM field amplitude $\Phi_0$ fixed by the average local DM density. However, motivate…

Cosmology and Nongalactic Astrophysics (astro-ph.CO)Atomic Physics (physics.atom-ph)530 PhysicsScienceQFOS: Physical sciences500Astrophysics::Cosmology and Extragalactic Astrophysics530 PhysikCharacterization and analytical techniquesArticlePhysics - Atomic PhysicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Dark energy and dark matterddc:500Astrophysics - Cosmology and Nongalactic AstrophysicsNature Communications
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