Search results for "ARTICLES"

showing 10 items of 9626 documents

Probing the bond order wave phase transitions of the ionic Hubbard model by superlattice modulation spectroscopy

2017

An exotic phase, the bond order wave, characterized by the spontaneous dimerization of the hopping, has been predicted to exist sandwiched between the band and Mott insulators in systems described by the ionic Hubbard model. Despite growing theoretical evidences, this phase still evades experimental detection. Given the recent realization of the ionic Hubbard model in ultracold atomic gases, we propose here to detect the bond order wave using superlattice modulation spectroscopy. We demonstrate, with the help of time-dependent density-matrix renormalization group and bosonization, that this spectroscopic approach reveals characteristics of both the Ising and Kosterlitz-Thouless transitions …

BosonizationHubbard model[PHYS.COND.GAS]Physics [physics]/Condensed Matter [cond-mat]/Quantum Gases [cond-mat.quant-gas]SuperlatticeGeneral Physics and AstronomyIonic bondingFOS: Physical sciences01 natural sciencesCondensed Matter - Strongly Correlated ElectronsPhysics and Astronomy (all)0103 physical sciencesBosonizationCold atoms010306 general physicsPhysicsCondensed Matter::Quantum GasesCondensed matter physicsDensity Matrix Renormalization GroupStrongly Correlated Electrons (cond-mat.str-el)010308 nuclear & particles physicsMott insulatorBerezinskii-Kosterlitz-Thouless transitionIsing transitionRenormalization groupBond orderQuantum Gases (cond-mat.quant-gas)Ising modelCondensed Matter::Strongly Correlated ElectronsCondensed Matter - Quantum Gases
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Spectroscopic Observations of the Delta Scorpii Binary during Its Recent Periastron Passage

2001

The bright star delta Sco has been considered a typical B0-type object for many years. Spectra of the star published prior to 1990 showed no evidence of emission, but only of short-term line profile variations attributed to nonradial pulsations. Speckle interferometric observations show that delta Sco is a binary system with a highly-eccentric orbit and a period of 10.6 years. Weak emission in the H-alpha line was detected in its spectrum for the first time during a periastron passage in 1990. Shortly before the next periastron passage in the summer of 2000, the binary entered a strong H-alpha emission and enhanced mass loss phase. We monitored the spectroscopic development of the Be outbur…

Bright starAstrophysics::High Energy Astrophysical PhenomenaBinary numberFOS: Physical sciencesOrbital eccentricityAstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA01 natural sciencesSpectral lineSpectroscopic Technich0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsBinary systemSpectroscopy010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsLine (formation)Physics010308 nuclear & particles physicsBinariesAstrophysics (astro-ph)Astronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Emission-line ; Binaries ; Sco ; Spectroscopic TechnichOrbitScoSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaEmission-line:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Detection of Intrinsic Source Structure at ~3 Schwarzschild Radii with Millimeter-VLBI Observations of SAGITTARIUS A*

2018

We report results from very long baseline interferometric (VLBI) observations of the supermassive black hole in the Galactic center, Sgr A*, at 1.3 mm (230 GHz). The observations were performed in 2013 March using six VLBI stations in Hawaii, California, Arizona, and Chile. Compared to earlier observations, the addition of the APEX telescope in Chile almost doubles the longest baseline length in the array, provides additional {\it uv} coverage in the N-S direction, and leads to a spatial resolution of $\sim$30 $\mu$as ($\sim$3 Schwarzschild radii) for Sgr A*. The source is detected even at the longest baselines with visibility amplitudes of $\sim$4-13% of the total flux density. We argue th…

BrightnessAstrophysics::High Energy Astrophysical PhenomenaAstronomyFOS: Physical sciencesContext (language use)General Relativity and Quantum Cosmology (gr-qc)Astrophysics01 natural sciencesGeneral Relativity and Quantum Cosmologylaw.inventionTelescopelaw0103 physical sciencesVery-long-baseline interferometry010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsSupermassive black hole010308 nuclear & particles physicsGalactic CenterAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesSagittarius A*Space and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Schwarzschild radius
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Long-term optical and X-ray variability of the Be/X-ray binary H 1145-619: Discovery of an ongoing retrograde density wave

2017

Multiwavelength monitoring of Be/X-ray binaries is crucial to understand the mechanisms producing their outbursts. H 1145-619 is one of these systems, which has recently displayed X-ray activity. We investigate the correlation between the optical emission and the X-ray activity to predict the occurrence of new X-ray outbursts from the inferred state of the circumstellar disc. We have performed a multiwavelength study of H 1145-619 from 1973 to 2017 and present here a global analysis of its variability over the last 40 years. We have used optical spectra from the SAAO, SMARTS and SALT telescopes and optical photometry from INTEGRAL/OMC and ASAS. We also used X-ray observations from INTEGRAL/…

BrightnessBe starAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectX-ray binarystars: emission-lineFOS: Physical sciencesAstrophysics01 natural sciencesSpectral lineDensity wave theoryPhotometry (optics)X-rays: binariesstars: neutrontechniques: photometric0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsBeAstronomy and AstrophysicsLight curvestars: emission-line BeAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceSkyAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenatechniques: spectroscopicAstronomy & Astrophysics
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Relativistic beaming and gamma-ray brightness of blazars

2009

We investigate the dependence of gamma-ray brightness of blazars on intrinsic properties of their parsec-scale radio jets and the implication for relativistic beaming. By combining apparent jet speeds derived from high-resolution VLBA images from the MOJAVE program with millimetre-wavelength flux density monitoring data from Metsahovi Radio Observatory, we estimate the jet Doppler factors, Lorentz factors, and viewing angles for a sample of 62 blazars. We study the trends in these quantities between the sources which were detected in gamma-rays by the Fermi Large Area Telescope (LAT) during its first three months of science operations and those which were not detected. The LAT-detected blaz…

BrightnessCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical Phenomenajets [galaxies]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionTelescopesymbols.namesakeRelativistic beaminglawquasars: general0103 physical sciencesBlazar010303 astronomy & astrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::GalaxiasHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsgeneral [quasars]general [BL Lacertae objects]010308 nuclear & particles physicsGamma rayAstronomy and Astrophysicsgalaxies: jetsViewing angle:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Galaxias [UNESCO]Lorentz factorSpace and Planetary Scienceactive [galaxies]BL Lacertae objectssymbolsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaAstrophysics - High Energy Astrophysical Phenomenagalaxies: active; ; ; BL Lacertae objects : generalFermi Gamma-ray Space TelescopeAstrophysics - Cosmology and Nongalactic Astrophysics
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The large-scale magnetic field of the eccentric pre-main-sequence binary system V1878 Ori

2020

We report time-resolved, high-resolution optical spectropolarimetric observations of the young double-lined spectroscopic binary V1878 Ori. Our observations were collected with the ESPaDOnS spectropolarimeter at the Canada-France-Hawaii Telescope through the BinaMIcS large programme. V1878 Ori A and B are partially convective intermediate mass weak-line T Tauri stars on an eccentric and asynchronous orbit. We also acquired X-ray observations at periastron and outside periastron. Using the least-squares deconvolution technique (LSD) to combine information from many spectral lines, we clearly detected circular polarization signals in both components throughout the orbit. We refined the orbita…

BrightnessFOS: Physical sciencesAstrophysicsspectroscopic [binaries]01 natural sciencesSpectral lineSettore FIS/05 - Astronomia E AstrofisicaAstronomi astrofysik och kosmologi0103 physical sciencespolarimetric [techniques]Astronomy Astrophysics and CosmologyAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Circular polarizationPhysics010308 nuclear & particles physics[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]stars: magnetic fieldAstronomy and AstrophysicsZeeman–Doppler imagingMagnetic fieldtechniques: polarimetricT Tauri starStarsOrbitindividual: V1878 Ori [stars]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary Sciencemagnetic field [stars]spectroscopic [techniques]Astrophysics::Earth and Planetary Astrophysicsbinaries: spectroscopicstars: individual: V1878 Oritechniques: spectroscopic
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Vanadium pentoxide nanoparticles mimic vanadium haloperoxidases and thwart biofilm formation

2012

Marine biofouling—the colonization of small marine microorganisms on surfaces that are directly exposed to seawater, such as ships' hulls—is an expensive problem that is currently without an environmentally compatible solution1. Biofouling leads to increased hydrodynamic drag, which, in turn, causes increased fuel consumption and greenhouse gas emissions. Tributyltin-free antifouling coatings and paints1, 2, 3, 4 based on metal complexes or biocides have been shown to efficiently prevent marine biofouling. However, these materials can damage5 the environment through metal leaching (for example, of copper and zinc)6 and bacteria resistance7. Here, we show that vanadium pentoxide nanowires ac…

BromidesBiocideVanadium CompoundsBiofoulingBiomedical Engineeringchemistry.chemical_elementVanadiumBioengineeringZincBiofoulingchemistry.chemical_compoundHypobromous acidHumansPentoxideSeawaterGeneral Materials ScienceElectrical and Electronic EngineeringHydrogen peroxideShipsSinglet OxygenNanowiresChemistryHydrogen PeroxideCondensed Matter PhysicsCopperAtomic and Molecular Physics and OpticsAnti-Bacterial AgentsPeroxidasesChemical engineeringBiofilmsNanoparticlesNature Nanotechnology
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Multiple-scan voltammetry and OCP: Archaeometric tools for dating archaeological bronzes

2021

[EN] The application of a multiple-scan strategy to nanosamples taken from 18 cross-sections of Bronze Age arms and armour, as well as two Roman coins using two solid-state electrochemical techniques, the voltammetry of immobilized microparticles (VIMP) and open circuit potential measurements (OCP) is described. The voltammetric responses in contact with aqueous acetate buffer can be attributed to the reduction of cuprite with variable degree of compaction and crystallinity revealing significant differences in the gradient of such properties with depth. Such differences are also revealed by "dry" OCP measurements connecting points in the cross section near and separated from the corrosion l…

Bronze AgeDating archaeological bronzesCupriteGeneral Chemical Engineeringchemistry.chemical_elementContext (language use)02 engineering and technologyengineering.material010402 general chemistry01 natural sciencesAnalytical ChemistryCorrosionCrystallinityElectrochemistryBronzeCorrosion studiesVoltammetryDeposition (law)Voltammetry of immobilized particlesMetallurgy021001 nanoscience & nanotechnologyCopper0104 chemical scienceschemistryPINTURAvisual_artOCPvisual_art.visual_art_mediumengineering0210 nano-technologyJournal of Electroanalytical Chemistry
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Multi-channel search for squarks and gluinos in root s=7 TeV pp collisions with the ATLAS detector at the LHC

2013

A search for supersymmetric particles in final states with zero, one, and two leptons, with and without jets identified as originating from b-quarks, in 4.7 fb[superscript −1] of √s = 7 TeV pp collisions produced by the Large Hadron Collider and recorded by the ATLAS detector is presented. The search uses a set of variables carrying information on the event kinematics transverse and parallel to the beam line that are sensitive to several topologies expected in supersymmetry. Mutually exclusive final states are defined, allowing a combination of all channels to increase the search sensitivity. No deviation from the Standard Model expectation is observed. Upper limits at 95 % confidence level…

Brookhaven National LaboratoryParticle physicsPhysics and Astronomy (miscellaneous)Supergauge TransformationsContext (language use)ddc:500.253001 natural sciencesStandard ModelSet (abstract data type)CurrentsPions0103 physical sciencesddc:530Sensitivity (control systems)WeakHigh Energy Physics010306 general physicsEngineering (miscellaneous)QCCiencias ExactasPhysicsproton–proton collisionsHadron-Hadron ScatteringLarge Hadron ColliderATLAS detector010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleHigh Energy Physics::PhenomenologyFísicaSupersymmetryATLASgluinosHADRON-HADRON COLLISIONSExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGsquarksHigh Energy Physics::ExperimentSupersymmetryLHCEvent (particle physics)LeptonModel
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A brown dwarf orbiting an M-dwarf:MOA 2009-BLG-411L

2012

Context. Caustic crossing is the clearest signature of binary lenses in microlensing. In the present context, this signature is diluted by the large source star but a detailed analysis has allowed the companion signal to be extracted.Aims. MOA 2009-BLG-411 was detected on August 5, 2009 by the MOA-Collaboration. Alerted as a high-magnification event, it was sensitive to planets. Suspected anomalies in the light curve were not confirmed by a real-time model, but further analysis revealed small deviations from a single lens extended source fit.Methods. Thanks to observations by all the collaborations, this event was well monitored. We first decided to characterize the source star properties b…

Brown dwarfContext (language use)Astrophysicsgravitational lensing: microAstrophysics::Cosmology and Extragalactic AstrophysicsGravitational microlensing01 natural sciencesSettore FIS/05 - Astronomia e AstrofisicaPlanet0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsstars: individual: MOA 2009-BLG-411L010308 nuclear & particles physicsAstronomyMOA 2009-BLG-411L; gravitational lensing; starsAstronomy and AstrophysicsRadiusLight curveGalaxyGravitational lensbinaries: generalSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysicsbinaries: general; gravitational lensing: micro; stars: individual: MOA 2009-BLG-411L
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