Search results for "NUMBER"

showing 10 items of 3939 documents

Cosmological shock waves: clues to the formation history of haloes

2012

Shock waves developed during the formation and evolution of cosmic structures encode crucial information on the hierarchical formation of the Universe. We analyze an Eulerian AMR hydro + N-body simulation in a $\Lambda$CDM cosmology focused on the study of cosmological shock waves. The combination of a shock-capturing algorithm together with the use of a halo finder allows us to study the morphological structures of the shock patterns, the statistical properties of shocked cells, and the correlations between the cosmological shock waves appearing at different scales and the properties of the haloes harbouring them. The shocks in the simulation can be split into two broad classes: internal w…

Shock waveCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesPower lawVirial theoremCosmologysymbols.namesake0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsShock (fluid dynamics)010308 nuclear & particles physicsAstronomyAstronomy and AstrophysicsRedshiftMach number13. Climate actionSpace and Planetary SciencesymbolsHaloAstrophysics - Cosmology and Nongalactic Astrophysics
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The Mach cone signal and energy deposition scenarios in linearized hydrodynamics

2010

Particle correlation measurements associated with a hard or semi-hard trigger in heavy-ion collisions may reflect Mach cone shockwaves excited in the bulk medium by partonic energy loss. This is of great interest because, when compared with theory, such measurements can provide information on the transport properties of the medium. Specifically, the formation of Mach cone shockwaves is sensitive to the viscosity and speed of sound, as well as the detailed nature of the jet medium interaction. However, modeling the physics of shockwave excitation to obtain a meaningful comparison with the measured correlations is very challenging since the correlations arise from an interplay of perturbative…

Shock wavePhysicsNuclear and High Energy PhysicsNuclear TheoryFluid Dynamics (physics.flu-dyn)FOS: Physical sciencesFluid mechanicsPartonPhysics - Fluid DynamicsComputational physicsMomentumPhysics::Fluid DynamicsNuclear Theory (nucl-th)High Energy Physics - Phenomenologysymbols.namesakeClassical mechanicsHigh Energy Physics - Phenomenology (hep-ph)Mach numberExcited stateSpeed of soundQuark–gluon plasmasymbols
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A flux-split algorithm applied to conservative models for multicomponent compressible flows

2003

In this paper we consider a conservative extension of the Euler equations for gas dynamics to describe a two-component compressible flow in Cartesian coordinates. It is well known that classical shock-capturing schemes applied to conservative models are oscillatory near the interface between the two gases. Several authors have addressed this problem proposing either a primitive consistent algorithm [J. Comput. Phys. 112 (1994) 31] or Lagrangian ingredients (Ghost Fluid Method by Fedkiw et al. [J. Comput. Phys. 152 (1999) 452] and [J. Comput. Phys. 169 (2001) 594]). We solve directly this conservative model by a flux-split algorithm, due to the first author (see [J. Comput. Phys. 125 (1996) …

Shock wavePhysicsNumerical AnalysisPhysics and Astronomy (miscellaneous)Computer simulationRichtmyer–Meshkov instabilityApplied MathematicsCompressible flowComputer Science Applicationslaw.inventionEuler equationsComputational Mathematicssymbols.namesakeMach numberlawModeling and SimulationCompressibilitysymbolsCartesian coordinate systemAlgorithmJournal of Computational Physics
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The nearest X-ray emitting protostellar jet observed with HST

2009

The HH 154 jet coming from the YSO binary L1551 IRS5 is one of the closest (about 150 pc) astrophysical jet known. It is therefore a unique laboratory for studies of outflow mechanisms and of the shocks forming at the interaction front between the expanding material and the ambient medium. The substructures (knots) observed within the HH 154 jet were imaged in several spectral bands using the Hubble Space Telescope. This allows us to derive a simple characterization of the physical conditions in different structures as well as to measure the proper motion of the knots in the jet, their flux variability and shock emission over a time base of about ten years. These knots in the jet undergo si…

Shock wavePhysicsProper motionAstrophysics::High Energy Astrophysical PhenomenaAstronomyBinary numberAstrophysicsSpectral bandsSettore FIS/05 - Astronomia E AstrofisicaKnot (unit)Astrophysical jetPlanetary bow shockCoincidentinterplanetary shocks X-ray binaries Astronomical and space-research instrumentationOutflowAstrophysics::Galaxy AstrophysicsAIP Conference Proceedings
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Crushing of interstellar gas clouds in supernova remnants II. X-ray emission

2006

AIMS. We study and discuss the time-dependent X-ray emission predicted by hydrodynamic modeling of the interaction of a SNR shock wave with an interstellar gas cloud. The scope includes: 1) to study the correspondence between modeled and X-ray emitting structures, 2) to explore two different physical regimes in which either thermal conduction or radiative cooling plays a dominant role, and 3) to investigate the effects of the physical processes at work on the emission of the shocked cloud in the two different regimes. METHODS. We use a detailed hydrodynamic model, including thermal conduction and radiation, and explore two cases characterized by different Mach numbers of the primary shock: …

Shock wavePhysicsRadiative coolingAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and Astrophysicsshock wavesAstrophysicsRadiationThermal conductionAstrophysicsISM: cloudsCoronaX-rays: ISMShock (mechanics)Supernovasymbols.namesakeMach numberSpace and Planetary SciencehydrodynamicssymbolsAstrophysics::Galaxy AstrophysicsISM: supernova remnants
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High order accurate shock capturing schemes for two-component Richtmyer-Meshkov instabilities in compressible magnetohydrodynamics

2011

We design a conservative and entropy satisfying numerical scheme to perform numerical simulations of two component Richtmyer-Meshkov (RM) instabilities in compressible magnetohydrodynamics (MHD). We first formulate a conservative model of a two-component compressible MHD fluid ruled under two ideal gases with different adiabatic exponents. The formulation includes a level set function that allows to evolve the two components of the plasma in a conservative and consistent way. We present a set of examples including two-component Riemann problems and high Mach shock wave interactions with entropy contact waves that validate the high order accurate numerical scheme. We observe that turbulent r…

Shock wavePhysicssymbols.namesakeClassical mechanicsMach numberTurbulencesymbolsCompressibilityPlasmaMechanicsMagnetohydrodynamicsAdiabatic processIdeal gas
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Discovery of the proton emitting nucleus $^{159}$Re

2007

Fund. para Cienc. Tecnol., FCT, Minist. Cienc. Tecnol.;Fundacao Calouste Gulbenkian;Fundacao Luso-Americana

Si detectorsnuclear spinMeasured E pProtonHadron02 engineering and technologyrhenium[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energyNuclear physicsIsotopes of cadmium0202 electrical engineering electronic engineering information engineeringnuclei with mass number 150 to 189Enriched targetsradioactive decay periodsNuclideIsotopeChemistryNuclear structure020206 networking & telecommunicationsT1/213. Climate action020201 artificial intelligence & image processing23.50.+z; 27.70.+q; 21.10.Tg; 21.10.HwGas-filled recoil separatorNucleonRadioactive decayNuclear reactions 58Ni + 106Cd at 300 MeV beam energyproton emission decay
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Generation of multidimensional random pulses for radioactivity measurements

2000

Multidimensional binary pseudo-random pulses are extremely useful for the set-up calibration and testing of radioactivity measuring equipment. A new method of generation of such signals, based on the parting operation of labeled pulse trains, is presented. The concept of a general coincidence ratio is introduced. Digital window comparators and prohibited or permitted state programmers capable of performing the parting operation and controlling the values of the coincidence ratio are proposed.

Signal generatorRandom number generationPulse generatorCalibrationElectronic engineeringBinary numberElectrical and Electronic EngineeringMultidimensional systemsInstrumentationCoincidenceMathematicsShift registerIEEE Transactions on Instrumentation and Measurement
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Physical modelling of the melt flow during large-diameter silicon single crystal growth

2003

Abstract The reported investigations concern physical modelling of Czochralski growth of silicon large-diameter single crystals. InGaSn eutectic was used as a modelling liquid, employing actual criteria of the real process (Prandtl, Reynolds, Grashof numbers, etc.) and geometric similarity. A multi-channel measuring system was used to collect and process the temperature and flow velocity data. The investigations were focused on the study of heat transfer, in particular, the instability of the “cold zone” of the melt at the crystallization front.

SiliconChemistryPrandtl numberGrashof numberMineralogychemistry.chemical_elementMechanicsCondensed Matter Physicslaw.inventionPhysics::Fluid DynamicsInorganic Chemistrysymbols.namesakeFlow velocitylawHeat transferMaterials ChemistrysymbolsCrystallizationMelt flow indexEutectic systemJournal of Crystal Growth
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Proton conducting composite electrolytes based on antimonic acid

1997

Abstract This report concerns a composite proton electrolyte suitable for use in electrochromic devices. The electrolyte consists of nanosize pyrochlore antimonic acid particles suspended in a poly(vinyl acetate) matrix by a gel route. It was found possible to substitute the antimonic acid by inert oxides of aluminum and silicon, thus making the electrolyte less harmful to the oxide electrodes of the electrochromic devices without considerably decreasing the conductivity. The proton conductivity of the antimonic acid electrolyte was ∼10 −4 S/cm at room temperature, practically independent of its amount of absorbed water.

SiliconInorganic chemistryComposite numberOxidechemistry.chemical_elementGeneral ChemistryElectrolyteConductivityCondensed Matter PhysicsElectrochromic deviceschemistry.chemical_compoundchemistryElectrochromismVinyl acetateGeneral Materials Science
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