Search results for "Wave"

showing 10 items of 6009 documents

Use of radiation sources with mercury isotopes for real-time highly sensitive and selective benzene determination in air and natural gas by different…

2015

A new analytical portable system is proposed for the direct determination of benzene vapor in the ambient air and natural gas, using differential absorption spectrometry with the direct Zeeman effect and innovative radiation sources: capillary mercury lamps with different isotopic compositions ((196)Hg, (198)Hg, (202)Hg, (204)Hg, and natural isotopic mixture). Resonance emission of mercury at a wavelength of 254 nm is used as probing radiation. The differential cross section of benzene absorption in dependence on wavelength is determined by scanning of magnetic field. It is found that the sensitivity of benzene detection is enhanced three times using lamp with the mercury isotope (204)Hg in…

Analytical chemistrychemistry.chemical_elementNatural GasMass spectrometryBiochemistryAnalytical Chemistrychemistry.chemical_compoundsymbols.namesakeLimit of DetectionEnvironmental ChemistryBenzeneSpectroscopyDetection limitAir PollutantsZeeman effectSpectrometerSpectrophotometry AtomicAbsorption RadiationBenzeneEquipment DesignTolueneMercury (element)WavelengthMercury IsotopeschemistrysymbolsEnvironmental MonitoringAnalytica chimica acta
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Polar bosons in one-dimensional disordered optical lattices

2013

We analyze the effects of disorder and quasi-disorder on the ground-state properties of ultra-cold polar bosons in optical lattices. We show that the interplay between disorder and inter-site interactions leads to rich phase diagrams. A uniform disorder leads to a Haldane-insulator phase with finite parity order, whereas the density-wave phase becomes a Bose-glass at very weak disorder. For quasi-disorder, the Haldane insulator connects with a gapped generalized incommesurate density wave without an intermediate critical region.

Anderson localization[PHYS.COND.GAS]Physics [physics]/Condensed Matter [cond-mat]/Quantum Gases [cond-mat.quant-gas]PACS : 67.85.-d 05.30.Jp 61.44.Fw 75.10.PqFOS: Physical sciences01 natural sciencesCondensed Matter::Disordered Systems and Neural NetworksUltracold atoms010305 fluids & plasmasDensity wave theoryCondensed Matter - Strongly Correlated ElectronsUltracold atomQuantum mechanics0103 physical sciencesAnderson localization010306 general physicsBosonPhase diagramPhysicsCondensed Matter::Quantum Gasesdipolar interactionsCondensed matter physicsStrongly Correlated Electrons (cond-mat.str-el)Parity (physics)Disordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksAubry-André transitionCondensed Matter PhysicsElectronic Optical and Magnetic MaterialsQuantum Gases (cond-mat.quant-gas)PolarCondensed Matter::Strongly Correlated ElectronsCondensed Matter - Quantum Gases
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Characteristics of the early flight phase in the Olympic ski jumping competition.

2004

Early flight phase (approximately 40 m) of the athletes participating in the final round of the individual large hill ski jumping competition in Salt Lake City Olympics was filmed with two high-speed pan & tilt video cameras. The results showed that jumpers' steady flight position was almost completed within 0.5s. The most significant correlation with the length of the jump was found in the angle between the skis and body (r=.714, p.001 at 1.1s after the take-off). This particular phase seemed to be important because the ski angle of attack was also related to the jumping distance at the same phase. Although the more upright ski position relative to flight path resulted in longer jumping di…

Angle of attackAltitudeRehabilitationBiomedical EngineeringBiophysicsPhase (waves)Steady flightVideotape RecordingEffects of high altitude on humansSki jumpingmedicine.disease_causeModels BiologicalBiomechanical PhenomenaCompetition (economics)JumpingAeronauticsSkiingmedicineJumpHumansOrthopedics and Sports MedicineComputer SimulationMathematicsJournal of biomechanics
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On the timing properties of SAX J1808.4-3658 during its 2015 outburst

2017

We present a timing analysis of the 2015 outburst of the accreting millisecond X-ray pulsar SAX J1808.4-3658, using non-simultaneous XMM-Newton and NuStar observations. We estimate the pulsar spin frequency and update the system orbital solution. Combining the average spin frequency from the previous observed, we confirm the long-term spin down at an average rate $\dot{\nu}_{\text{SD}}=1.5(2)\times 10^{-15}$ Hz s$^{-1}$. We also discuss possible corrections to the spin down rate accounting for mass accretion onto the compact object when the system is X-ray active. Finally, combining the updated ephemerides with those of the previous outbursts, we find a long-term orbital evolution compatibl…

Angular momentumAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesLagrangian pointAstrophysicsCompact star01 natural sciencespulsars: individual: SAX J1808.4-3658Gravitationstars: neutronX-rays: binariesSettore FIS/05 - Astronomia E AstrofisicaPulsar0103 physical sciences010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsOrbital periodaccretion accretion discs; stars: neutron; pulsars: individual: SAX J1808.4-3658; X-rays: binaries13. Climate actionSpace and Planetary ScienceQuadrupole:accretion accretion discAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Relativistic simulations of rotational core collapse : I. Methods, initial models, and code tests

2002

We describe an axisymmetric general relativistic code for rotational core collapse. The code evolves the coupled system of metric and fluid equations using the ADM 3+1 formalism and a conformally flat metric approximation of the Einstein equations. The relativistic hydrodynamics equations are formulated as a first-order flux-conservative hyperbolic system and are integrated using high-resolution shock-capturing schemes based on Riemann solvers. We assess the quality of the conformally flat metric approximation for relativistic core collapse and present a comprehensive set of tests which the code successfully passed. The tests include relativistic shock tubes, the preservation of the rotatio…

Angular momentumAstrophysics::High Energy Astrophysical PhenomenaRotational symmetryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsNumerical methodAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAGeneral Relativity and Quantum CosmologyGravitational wavesGravitationRelativitysymbols.namesakeWaveformPhysicsAstrophysics (astro-ph)Astronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Hyperbolic systemsNeutron starRiemann hypothesisClassical mechanicsSpace and Planetary ScienceGravitational waves ; Hydrodynamics ; Numerical method ; RelativitysymbolsHydrodynamicsFluid equationUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Wavelet analysis and HHG in nanorings: their applica-tions in logic gates and memory mass devices

2015

We study the application of one nanoring driven by a laser field in different states of polarization in logic circuits. In particular we show that assigning Boolean values to different states of the incident laser field and to the emitted signals, we can create logic gates such as OR, XOR and AND. We also show the possibility of making logic circuits such as half-adder and full-adder using one and two nanorings respectively. Using two nanorings we made the Toffoli gate. Finally we use the final angular momentum acquired by the electron to store information and hence show the possibility of using an array of nanorings as a mass memory device.

Angular momentumFOS: Physical sciencesToffoli gate02 engineering and technologyElectronTopology01 natural scienceslaw.inventionWaveletlaw0103 physical sciencesGeneral Materials Science010306 general physicsPhysicsQuantum Physics021001 nanoscience & nanotechnologyPolarization (waves)LaserLogic gateLogic gate quantum information nanoring quantum ring laser interaction wavelet high harmonic generationMaterials Science (all)0210 nano-technologyQuantum Physics (quant-ph)NanoringPhysics - OpticsHardware_LOGICDESIGNOptics (physics.optics)
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Production and detection of atomic hexadecapole at Earth's magnetic field

2007

Anisotropy of atomic states is characterized by population differences and coherences between Zeeman sublevels. It can be efficiently created and probed via resonant interactions with light, the technique which is at the heart of modern atomic clocks and magnetometers. Recently, nonlinear magneto-optical techniques have been developed for selective production and detection of higher polarization moments, hexadecapole and hexacontatetrapole, in the ground states of the alkali atoms. Extension of these techniques into the range of geomagnetic fields is important for practical applications. This is because hexadecapole polarization corresponding to the $\Delta M=4$ Zeeman coherence, with maxim…

Angular momentumLightEarth PlanetMagnetometerAtomic Physics (physics.atom-ph)TransducersPopulationFOS: Physical sciencesRadiation Dosagelaw.inventionPhysics - Atomic PhysicsMagneticssymbols.namesakelawPhysical Sciences and MathematicsScattering RadiationComputer SimulationPhysics::Atomic PhysicsRadiometryAnisotropyeducationPhysicseducation.field_of_studyZeeman effectEquipment DesignModels TheoreticalPolarization (waves)Atomic and Molecular Physics and OpticsAtomic clockMagnetic fieldEquipment Failure AnalysisBudker [BRII recipient]symbolsComputer-Aided DesignAtomic physicsEnvironmental Monitoring
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Evolutionary paths of binaries with a neutron star - I. The case of SAX J1808.4 - 3658

2018

The evolutionary status of the low mass X-ray binary SAX J1808.4-3658 is simulated by following the binary evolution of its possible progenitor system through mass transfer, starting at a period of $\sim$6.6 hr. The evolution includes angular momentum losses via magnetic braking and gravitational radiation. It also takes into account the effects of illumination of the donor by both the X-ray emission and the spin down luminosity of the pulsar. The system goes through stages of mass transfer and stages during which it is detached, where only the rotationally powered pulsar irradiates the donor. We show that the pulsar irradiation is a necessary ingredient to reach SAX J1808.4-3658 orbital pe…

Angular momentumastro-ph.SRAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesLuminosityPulsars: individual: SAX J1808.4Settore FIS/05 - Astronomia E AstrofisicaPulsarBinaries: closeMass transfer0103 physical sciencesBinaries: generalStars: low-maAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)3658 -X-rays: binarieHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HE010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsAstronomy and AstrophysicOrbital periodNeutron starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaLow Mass
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A second strain gradient elasticity theory with second velocity gradient inertia – Part II: Dynamic behavior

2013

Abstract This paper is the sequel of a companion Part I paper devoted to the constitutive equations and to the quasi-static behavior of a second strain gradient material model with second velocity gradient inertia. In the present Part II paper, a multi-cell homogenization procedure (developed in the Part I paper) is applied to a nonhomogeneous body modelled as a simple material cell system, in conjunction with the principle of virtual work (PVW) for inertial actions (i.e. momenta and inertia forces), which at the macro-scale level takes on the typical format as for a second velocity gradient inertia material model. The latter (macro-scale) PVW is used to determine the equilibrium equations …

Angular momentummedia_common.quotation_subjectRotary inertiaPolhodeContinuum thermodynamicsInertiaMoment of inertia factorsymbols.namesakeMaterials Science(all)Modelling and SimulationGeneral Materials ScienceEuler's equationsmedia_commonMathematicsWave propagationApplied MathematicsMechanical EngineeringMathematical analysisMoment of inertiaCondensed Matter PhysicsRigid body dynamicsDynamicsGradient elasticityClassical mechanicsHigher order inertiaMechanics of MaterialsModeling and SimulationsymbolsInternational Journal of Solids and Structures
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A gradient elasticity theory for second-grade materials and higher order inertia

2012

Abstract Second-grade elastic materials featured by a free energy depending on the strain and the strain gradient, and a kinetic energy depending on the velocity and the velocity gradient, are addressed. An inertial energy balance principle and a virtual work principle for inertial actions are envisioned to enrich the set of traditional theoretical tools of thermodynamics and continuum mechanics. The state variables include the body momentum and the surface momentum, related to the velocity in a nonstandard way, as well as the concomitant mass-accelerations and inertial forces, which do intervene into the motion equations and into the force boundary conditions. The boundary traction is the …

Angular momentummedia_common.quotation_subjectTraction (engineering)Continuum thermodynamicsInertiaMaterials Science(all)Modelling and SimulationWave dispersionGeneral Materials ScienceVirtual workBoundary value problemmedia_commonMathematicsContinuum mechanicsForce densityMechanical EngineeringApplied MathematicsMathematical analysisEquations of motionCondensed Matter PhysicsDynamicsGradient elasticityClassical mechanicsHigher order inertiaMechanics of MaterialsModeling and SimulationInternational Journal of Solids and Structures
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