Search results for "fluid"

showing 10 items of 5513 documents

Linking Jet Emission, X‐Ray States, and Hard X‐Ray Tails in the Neutron Star X‐Ray Binary GX 17 \documentclass{aastex} \usepackage{amsbsy} \usepackag…

2007

We present the results from simultaneous radio (Very Large Array) and X-ray (Rossi-X-ray Timing Explorer) observations of the Z-type neutron star X-ray binary GX~17+2. The aim is to assess the coupling between X-ray and radio properties throughout its three rapidly variable X-ray states and during the time-resolved transitions. These observations allow us, for the first time, to investigate quantitatively the possible relations between the radio emission and the presence of the hard X-ray tails and the X-ray state of the source. The observations show: 1) a coupling between the radio jet emission and the X-ray state of the source, i.e. the position in the X-ray hardness-intensity diagram (HI…

PhysicsJet (fluid)Neutron starSpace and Planetary ScienceOscillationAstrophysics::High Energy Astrophysical PhenomenaX-ray binarySpectral densityFluxAstronomy and AstrophysicsContext (language use)AstrophysicsPower lawThe Astrophysical Journal
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Measurement of Associated Production ofZBosons with Charm Quark Jets inpp¯Collisions ats=1.96  TeV

2014

We present the first measurements of the ratios of cross sections sigma(p (p) over bar -> Z + c jet)/sigma(p (p) over bar -> Z + jet) and sigma(p (p) over bar -> Z + jet)/sigma(p (p) over bar -> Z + b jet) for the associated production of a Z boson with at least one charm or bottom quark jet. Jets have transverse momentum p(T)(jet) > 20 GeV and pseudorapidity vertical bar eta(jet)vertical bar collisions collected with the D0 detector at the Fermilab Tevatron Collider at root s = 1.96 TeV. The measurements show significant deviations from perturbative QCD calculations and predictions from various event generators.

PhysicsJet (fluid)Particle physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyTevatronGeneral Physics and AstronomyPerturbative QCD7. Clean energyBottom quarkCharm quarkNuclear physicsPseudorapidityHigh Energy Physics::ExperimentNuclear ExperimentBar (unit)BosonPhysical Review Letters
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Measurement of the Inclusive Jet Cross Section inpp¯Collisions ats=1.96  TeV

2008

We report on a measurement of the inclusive jet cross section in p (p) over bar collisions at a center-of-mass energy root s = 1.96 TeV using data collected by the D0 experiment at the Fermilab Tevatron Collider corresponding to an integrated luminosity of 0: 70 fb(-1). The data cover jet transverse momenta from 50 to 600 GeV and jet rapidities in the range -2.4 to 2.4. Detailed studies of correlations between systematic uncertainties in transverse momentum and rapidity are presented, and the cross section measurements are found to be in good agreement with next-to-leading order QCD calculations.

PhysicsJet (fluid)Particle physicsLuminosity (scattering theory)010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaTevatronGeneral Physics and AstronomyD0 experiment01 natural scienceslaw.inventionNuclear physicsCross section (physics)law0103 physical sciencesHigh Energy Physics::ExperimentRapidityFermilab010306 general physicsColliderPhysical Review Letters
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Search for Large Extra Dimensions in Final States Containing One Photon or Jet and Large Missing Transverse Energy Produced inpp¯Collisions ats=1.96 …

2008

We present the results of searches for large extra dimensions in samples of events with large missing transverse energy E_{T} and either a photon or a jet produced in pp[over ] collisions at sqrt[s]=1.96 TeV collected with the Collider Detector at Fermilab II. For gamma+E_{T} and jet+E_{T} candidate samples corresponding to 2.0 and 1.1 fb;{-1} of integrated luminosity, respectively, we observe good agreement with standard model expectations and obtain a combined lower limit on the fundamental parameter of the large extra dimensions model M_{D} as a function of the number of extra dimensions in the model.

PhysicsJet (fluid)Particle physicsPhotonLuminosity (scattering theory)010308 nuclear & particles physicsGeneral Physics and Astronomy7. Clean energy01 natural sciencesStandard ModelNuclear physicsExtra dimensions0103 physical sciencesLarge extra dimensionHigh Energy Physics::Experiment010306 general physicsCollider Detector at FermilabEnergy (signal processing)Physical Review Letters
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ITER-relevant calibration technique for soft x-ray spectrometer

2010

The ITER-oriented JET research program brings new requirements for the low-Z impurity monitoring, in particular for the Be—the future main wall component of JET and ITER. Monitoring based on Bragg spectroscopy requires an absolute sensitivity calibration, which is challenging for large tokamaks. This paper describes both “component-by-component” and “continua” calibration methods used for the Be IV channel (75.9 Å) of the Bragg rotor spectrometer deployed on JET. The calibration techniques presented here rely on multiorder reflectivity calculations and measurements of continuum radiation emitted from helium plasmas. These offer excellent conditions for the absolute photon flux calibration d…

PhysicsJet (fluid)PhotonTokamakSpectrometerBragg's lawlaw.inventionComputational physicslawMeasuring instrumentCalibrationPlasma diagnosticsAtomic physicsInstrumentationReview of Scientific Instruments
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About some new possibilities of increasing the intrinsic output power of the photon beam: for definite laser active media

2006

Producers and users of laser beam equipment have some wishes as: to have economic machines, the machines must be as small and light as possible, the power supply must be also very light and small. All mentioned desires - and other related with them - may be accomplished by an adequate efficiency of laser beam process. As we know, the first laser began with 2% efficiency. In the process of time, the efficiency increased progressive, and in this way was possible after the year 2000 to have laser weapons mounted on jet planes, including the power supply. In a laser system, there are many points where photons are lost. To reduce this losses, we must treat with the utmost care all points of the …

PhysicsJet (fluid)Photonbusiness.industryProcess (computing)Physics::OpticsResonanceLaserlaw.inventionPower (physics)OpticslawMechanical efficiencybusinessEnergy (signal processing)Laser Beam Control and Applications
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The topology dependence of charged particle multiplicities in three-jet events

1997

A study of individual jet and whole-event charged particle multiplicities in three-jet events measured in e(+)e(-) annihilation at the Z reveals a significant topology dependence. Mean jet multiplicities are inadequately described by jet energies; interjet angles must also be specified. Quantitative tests suggest that it is necessary to use transverse-momentum-like scales to describe the data. RI ANTONELLI, ANTONELLA/C-6238-2011; Passalacqua, Luca/F-5127-2011; Murtas, Fabrizio/B-5729-2012; St.Denis, Richard/C-8997-2012; Sanchez, Federico/F-5809-2012; Forti, Francesco/H-3035-2011; Ferrante, Isidoro/F-1017-2012

PhysicsJet (fluid)Physics and Astronomy (miscellaneous)010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsElectron–positron annihilation01 natural sciencesCharged particleNuclear physics0103 physical sciencesTransverse momentum[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics::Experiment010306 general physicsParticle Physics - ExperimentTopology (chemistry)
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Jet transition values for the anti-$$k_{\bot }$$ k⊥ algorithm

2019

We define jet transition values for the anti-$k_{\bot}$ algorithm for both hadron and $e^+e^-$ colliders. We show how these transition values can be computed and how they can be used to improve the performance of clusterization when jet resolution parameters are varied over a larger set of values. Finally we present a simple performance test to illustrate the behavior of the new method compared to the original one.

PhysicsJet (fluid)Physics and Astronomy (miscellaneous)010308 nuclear & particles physicsHadronFOS: Physical scienceslcsh:Astrophysics01 natural sciencesComputer Science::Digital LibrariesHigh Energy Physics - ExperimentSet (abstract data type)High Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)lcsh:QB460-4660103 physical scienceslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityHigh Energy Physics::Experiment010306 general physicsEngineering (miscellaneous)AlgorithmComputer Science::DatabasesEuropean Physical Journal
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Generation of radiative knots in a randomly pulsed protostellar jet

2009

HH objects are characterized by a complex knotty morphology detected mainly along the axis of protostellar jets in a wide range of bands. Evidence of interactions between knots formed in different epochs have been found, suggesting that jets may result from the ejection of plasma blobs from the source. We aim at investigating the physical mechanism leading to the irregular knotty structure observed in jets in different bands and the complex interactions occurring among blobs of plasma ejected from the stellar source. We perform 2D axisymmetric HD simulations of a randomly ejected pulsed jet. The jet consists of a train of blobs which ram with supersonic speed into the ambient medium. The in…

PhysicsJet (fluid)Proper motionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsPlasmaThermal conductionAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceReflection (physics)Radiative transferOblique shockSupersonic speedhydrodynamics – Herbig-Haro objects – ISM: jets and outflows – X-rays: ISMSolar and Stellar Astrophysics (astro-ph.SR)Astronomy and Astrophysics
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The X-ray emission mechanism in the protostellar jet HH 154

2004

We study the mechanism causing the X-ray emission recently detected in protostellar jets, by performing a detailed modeling of the interaction between a supersonic jet originating from a young stellar object and the ambient medium, for various values of density contrast, ν, between the ambient density and the jet, and of Mach number, M; radiative losses and thermal conduction have been taken into account. Here we report a representative case which reproduces, without any ad hoc assumption, the characteristics of the X-ray emission recently observed in the protostellar jet HH 154. We find that the X-ray emission originates from a localized blob, consistent with observations, which moves with…

PhysicsJet (fluid)Proper motionAstrophysics::High Energy Astrophysical PhenomenaYoung stellar objectAstronomy and AstrophysicsAstrophysicsThermal conductionISM: Herbig-Haro objects ISM: individual objects: HH 154 ISM: jets and outflows X-rays: ISMSpace and Planetary ScienceRadiative transferSupersonic speedHerbig–Haro objectDensity contrastAstrophysics::Galaxy Astrophysics
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