Search results for " jet"

showing 10 items of 3151 documents

"Table 2" of "A measurement of the ratio of the W and Z cross sections with exactly one associated jet in pp collisions at sqrt(s) = 7 TeV with ATLAS"

2013

The ratios of W to Z production in the fiducial region for the individual lepton channels and for the channels combined.

SIG/SIGZ ProductionHigh Energy Physics::PhenomenologyIntegrated Cross Section7000.0Astrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionCross SectionInclusiveP P --> Z0 JET XProton-Proton ScatteringP P --> W+ JET XHigh Energy Physics::ExperimentP P --> W- JET XW ProductionComputer Science::Information Theory
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"Table 14" of "Measurement of the production cross section for Z/gamma* in association with jets in pp collisions at sqrt(s) = 7 TeV with the ATLAS d…

2014

Ratio of cross sections for N/N-1 inclusive jet multiplicities for the electron channel and the muon channel in the individual lepton fiducial regions and uncorrected for QED effects.

SIG/SIGZ ProductionHigh Energy Physics::PhenomenologyIntegrated Cross SectionAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionCross SectionInclusiveP P --> Z0 JET XP P --> GAMMA* JET XProton-Proton ScatteringHigh Energy Physics::ExperimentComputer Science::Information Theory
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"Table 10" of "Energy dependence of event shapes and of alpha(s) at LEP-2."

1999

Moments of the the Total Jet Broadening (BSUM) distributions at cm energies 133, 161, 172 and 183 GeV.

SKEWNESSNAME=BSUMBSUM133.0-183.0Astrophysics::High Energy Astrophysical PhenomenaE+ E- --> HADRONSE+ E- --> JETSE+ E- ScatteringExclusiveHigh Energy Physics::ExperimentJet ProductionVARIANCENAME=BSUMNuclear Experiment
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Laboratory disruption of scaled astrophysical outflows by a misaligned magnetic field

2021

The shaping of astrophysical outflows into bright, dense, and collimated jets due to magnetic pressure is here investigated using laboratory experiments. Here we look at the impact on jet collimation of a misalignment between the outflow, as it stems from the source, and the magnetic field. For small misalignments, a magnetic nozzle forms and redirects the outflow in a collimated jet. For growing misalignments, this nozzle becomes increasingly asymmetric, disrupting jet formation. Our results thus suggest outflow/magnetic field misalignment to be a plausible key process regulating jet collimation in a variety of objects from our Sun’s outflows to extragalatic jets. Furthermore, they provide…

ScienceAstrophysics::High Energy Astrophysical PhenomenaNozzleoutflows magnetohydrodynamics(MHD) shockwaves astrophysical jetsGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics01 natural sciencesArticleGeneral Biochemistry Genetics and Molecular BiologyCollimated lightSettore FIS/05 - Astronomia E AstrofisicaAmbient field0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsMagnetic pressure010306 general physics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsLaboratory astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Jet (fluid)MultidisciplinaryQLaser-produced plasmasGeneral ChemistryPhysics - Plasma PhysicsMagnetic fieldPlasma Physics (physics.plasm-ph)Astrophysics - Solar and Stellar AstrophysicsPhysics::Accelerator PhysicsOutflowHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Measurement of the forward-backward asymmetry of e(+)e(-)-]z-]b(b)over-bar using prompt leptons and a lifetime tag

1995

The forward-backward asymmetry of the process e+e-→Z→b {Mathematical expression} has been measured using events collected by the DELPHI experiment during the 1991 and 1992 LEP runs. This data sample corresponded to 884 000 hadronic Z decays at a centre-of-mass energy {Mathematical expression}. The tagging of b-quark events was performed using two approaches; the first was based on the semileptonic decay channels b→X+μ and b→X+e, the second used a lifetime tag with jet-charge reconstruction. The results of these two methods were combined to give {Mathematical expression} With the semileptonic sample, the forward-backward asymmetry of the process e+e-→Z→ {Mathematical expression} was also mea…

Semileptonic decayParticle physicsFERMION PAIR PRODUCTIONPhysics and Astronomy (miscellaneous)LUND MONTE-CARLOENERGIESElectron–positron annihilationQED CORRECTIONSD-MESONSEMILEPTONIC DECAY01 natural sciencesJET FRAGMENTATIONb-taggingPartícules (Física nuclear)PHYSICSNuclear physics0103 physical sciencesDELPHI; forward-backward asymmetry; b-tagging; jet reconstructionFERMION PAIR PRODUCTION; LUND MONTE-CARLO; E+E-ANNIHILATION; SEMILEPTONIC DECAY; JET FRAGMENTATION; QED CORRECTIONS; FINAL-STATES; D-MESON; ENERGIES; PHYSICS010306 general physicsEngineering (miscellaneous)jet reconstructionDetectors de radiacióDELPHIPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyWeinberg angleE+E-ANNIHILATIONLARGE ELECTRON POSITRON COLLIDERFINAL-STATESb-taggingPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHILarge Electron–Positron ColliderPARTICLE PHYSICSHigh Energy Physics::Experimentforward-backward asymmetryEnergy (signal processing)Particle Physics - ExperimentLeptonBar (unit)
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EFFECT OF FRUIT-SET TIME ON THE QUALITY PERFORMANCE OF ANNONA CHERIMOLA MILL. FRUIT

2019

The aim of this work was to analyze the differences between fruits obtained by different dates of fruit set and identify the proper fruit-set time that allows to obtain the optimum fruit quality in Annona cherimola cv Fino de Jete, planted in Southern Italy. Six fruit-set dates were selected from the first week of June to the second week of July. Fruits were sampled from October to November, when 1500 Growing Degree Days (DD) were accumulated; The DD were calculated using a base temperature of 12 °C. Fruit fresh weight (FW) and skin colour were measured. These parameters were measured also after storage, and in addition, the following parameters were measured: fruit shape (FS), pulp colour,…

Settore AGR/03 - Arboricoltura Generale E Coltivazioni ArboreeDegree Days Antioxidant Ascorbic Acid Polyphenol fruit shape Finode Jete
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X-ray emission mechanisms in protostellar jets

2005

Prompted by the recent detection of X-ray emission from Herbig-Haro objects, we studied the interaction between a supersonic jet originating from a young stellar object and the ambient medium; our aim is to investigate the mechanisms causing the X-ray emission. Our model takes into account the radiative losses from optically in plasmas and Spitzer's thermal conduction including saturation effects. We explored the parameter space defined by the density contrast between the ambient medium and the jet and by the Mach number, to infer the configurations which can give rise to X-ray emission. From the models, we derived the X-ray emission as it would be observed with Chandra/ACIS-I and XMM-Newto…

Settore FIS/05 - Astronomia E AstrofisicaHerbig-Haro objects – ISM: individual jets and outflows – X-rays: ISM [SM]SM: Herbig-Haro objects – ISM: individual objects (HH 154) – ISM: jets and outflows – X-rays: ISM
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Modelling and bench scale investigation of inclined dense jets

2002

Settore ING-IND/24 - Principi Di Ingegneria ChimicaSettore ING-IND/25 - Impianti Chimicimodelling dense jet brine disposal
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Impact of red giant/AGB winds on active galactic nucleus jet propagation

2017

Astronomy and astrophysics 606, A40 (2017). doi:10.1051/0004-6361/201630117

Shock waveAstrofísicaActive galactic nucleusRed giantAstrophysics::High Energy Astrophysical PhenomenaContext (language use)AstrophysicsAstrophysics01 natural sciencesJets (Astrofísica)0103 physical sciencesAsymptotic giant branchAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsMixing (physics)Astrophysics::Galaxy AstrophysicsPhysicsJet (fluid)010308 nuclear & particles physicsAstronomy and Astrophysics520Astrophysical jetsStars13. Climate actionSpace and Planetary ScienceGalàxies activesActive galaxiesddc:520
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Testing jet geometries and disc-jet coupling in the neutron star LMXB 4U 0614 + 091 with the internal shocks model

2020

Multi-wavelength spectral energy distributions of Low Mass X-ray Binaries in the hard state are determined by the emission from a jet, for frequencies up to mid-infrared, and emission from the accretion flow in the optical to X-ray range. In the last years, the flat radio-to-mid-IR spectra of Black Hole (BH) X-ray binaries was described using the internal shocks model, which assumes that the fluctuations in the velocity of the ejecta along the jet are driven by the fluctuations in the accretion flow, described by the X-ray Power Density Spectrum (PDS). In this work we attempt to apply this model for the first time to a Neutron Star (NS) LMXB, i.e. 4U 0614+091. We used the multi-wavelength d…

Shock waveAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesSpectral linestars: jetsX-rays: binariesstars: neutronaccretion0103 physical sciencesEjecta010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsSpectral densityAstronomy and AstrophysicsConical surfaceshock wavesaccretion discsAccretion (astrophysics)Neutron starSpace and Planetary Scienceaccretion accretion discsAstrophysics - High Energy Astrophysical PhenomenaLow Mass[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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