Search results for "COSMO"

showing 10 items of 3164 documents

"Table 1" of "Measurement of the Inelastic Proton-Proton Cross Section at $\sqrt{s} = 13$ TeV with the ATLAS Detector at the LHC"

2016

The measured and extrapolated inelastic cross section. The statistical uncertainty is negligible and is therefore displayed as zero. The first systematic uncertainty is the experimental systematic uncertainty apart from the luminosity, the second is the luminosity uncertainty, and the third is the extrapolation uncertainty.

13000.0Proton-Proton ScatteringAstrophysics::High Energy Astrophysical PhenomenaIntegrated Cross SectionExclusiveHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGProton-Proton Total Cross SectionP P --> X
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"Table 3" of "Measurement of the $ZZ$ Production Cross Section in $pp$ Collisions at $\sqrt{s}$ = 13 TeV with the ATLAS Detector"

2016

Measured fiducial cross section in the $\mu^+\mu^-\mu^+\mu^-$ channel. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity uncertainty, the second is the luminosity uncertainty.

13000.0Z ProductionAstrophysics::High Energy Astrophysical PhenomenaP P --> Z0 Z0 XIntegrated Cross SectionAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGMuon productionInclusiveProton-Proton ScatteringAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentZ pair ProductionAstrophysics::Galaxy Astrophysics
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"Table 1" of "Measurement of the $ZZ$ Production Cross Section in $pp$ Collisions at $\sqrt{s}$ = 13 TeV with the ATLAS Detector"

2016

Measured fiducial cross section in the $e^+e^-e^+e^-$ channel. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity uncertainty, the second is the luminosity uncertainty.

13000.0Z ProductionElectron productionAstrophysics::High Energy Astrophysical PhenomenaP P --> Z0 Z0 XIntegrated Cross SectionAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGInclusiveProton-Proton ScatteringAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentZ pair ProductionAstrophysics::Galaxy Astrophysics
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"Table 2" of "Measurement of the $ZZ$ Production Cross Section in $pp$ Collisions at $\sqrt{s}$ = 13 TeV with the ATLAS Detector"

2016

Measured fiducial cross section in the $e^+e^-\mu^+\mu^-$ channel. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity uncertainty, the second is the luminosity uncertainty.

13000.0Z ProductionElectron productionAstrophysics::High Energy Astrophysical PhenomenaP P --> Z0 Z0 XIntegrated Cross SectionAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGMuon productionInclusiveProton-Proton ScatteringAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentZ pair ProductionAstrophysics::Galaxy Astrophysics
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"Table 1" of "Measurement of the t anti-t production cross section in p anti-p collisions at s**(1/2) = 1.96-TeV using lepton + jets events with life…

2006

TTBAR production cross section. Error contains statistical and systematics (excluding the luminosity uncertainty).

2.0478E+062.0478E+06PBAR P --> TOP TOPBARAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyIntegrated Cross SectionExclusiveHigh Energy Physics::ExperimentAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIG1960.0
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"Table 2" of "Measurement of the inclusive jet cross-section in p anti-p collisions at s**(1/2) =1.96-TeV"

1970

Measured inclusive jet cross section as a function of jet transverse momentum for absolute values of the jet rapidity from 0.4 to 0.8 for cone radius R = 0.7.

20477612047761Astrophysics::High Energy Astrophysical PhenomenaRapidity DependencePBAR P --> JET XAstrophysics::Cosmology and Extragalactic AstrophysicsJet Productionrespiratory systemequipment and suppliescomplex mixturesInclusiveHigh Energy Physics::ExperimentD2SIG/DPT/DYRAPTransverse Momentum Dependencehuman activitiesDouble Differential Cross Sectioncirculatory and respiratory physiology
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LA UNIVERSITAT RESPON: FORATS NEGRES

2007

Programa pilot de la sèrie de microespais 'La Universitat respon'. En este capítol es respon a pregunta: Què són els forats negres?.

2101 Astronomia i AstrofísicaDivulgació científica Astronomia Cosmologia Forats negres
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"Table 3" of "Measurement of inclusive jet and dijet cross sections in proton-proton collisions at 7 TeV centre-of-mass energy with the ATLAS detecto…

2010

Inclusive jet double-differential cross sections in the |rapidity| range 0.8 to 1.2, using a jet resolution R value of 0.4. The three (sys) errors are respectively, the Absolute JES, the Unfolding and the Luminosity uncertainties.

26119402611940Astrophysics::High Energy Astrophysical PhenomenaRapidity Dependence7000.0Astrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionP P --> JET XInclusiveProton-Proton ScatteringHigh Energy Physics::ExperimentD2SIG/DPT/DYRAPTransverse Momentum DependenceDouble Differential Cross SectionAstrophysics::Galaxy Astrophysics
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"Table 8" of "Measurement of inclusive jet and dijet cross sections in proton-proton collisions at 7 TeV centre-of-mass energy with the ATLAS detecto…

2010

Inclusive jet double-differential cross sections in the |rapidity| range 0.8 to 1.2, using a jet resolution R value of 0.6. The three (sys) errors are respectively, the Absolute JES, the Unfolding and the Luminosity uncertainties.

26119402611940Astrophysics::High Energy Astrophysical PhenomenaRapidity Dependence7000.0Astrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionP P --> JET XInclusiveProton-Proton ScatteringHigh Energy Physics::ExperimentD2SIG/DPT/DYRAPTransverse Momentum DependenceDouble Differential Cross SectionAstrophysics::Galaxy Astrophysics
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The richest superclusters : I Morphology

2007

We study the morphology of the richest superclusters from the catalogues of superclusters of galaxies in the 2dF Galaxy Redshift Survey and compare the morphology of real superclusters with model superclusters in the Millennium Simulation. We use Minkowski functionals and shapefinders to quantify the morphology of superclusters: their sizes, shapes, and clumpiness. We generate empirical models of simple geometry to understand which morphologies correspond to the supercluster shapefinders. We show that rich superclusters have elongated, filamentary shapes with high-density clumps in their core regions. The clumpiness of superclusters is determined using the fourth Minkowski functional $V_3$.…

2dF Galaxy Redshift SurveyPhysicsMorphology (linguistics)Large-scale structure of UniverseMinkowski functionalAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsGalaxiesAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]GalaxyCosmologyClustersSpace and Planetary ScienceSuperclusterMinkowski spaceUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Cosmology ; Large-scale structure of Universe ; Galaxies ; Clusters
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