Search results for "Astrophysical"

showing 10 items of 4966 documents

Measurement of thett¯production cross section inpp¯collisions ats=1.96  TeVusing soft electronb-tagging

2010

The authors present a measurement of the t{bar t} production cross section using events with one charged lepton and jets from p{bar p} collisions at a center-of-mass energy of 1.96 TeV. A b-tagging algorithm based on the probability of displaced tracks coming from the event interaction vertex is applied to identify b quarks from top decay. Using 318 pb{sup -1} of data collected with the CDF II detector, they measure the t{bar t} production cross section in events with at least one restrictive (tight) b-tagged jet and obtain 8.9{sub -1.0}{sup +1.0}(stat.){sub -1.0}{sup +1.1}(syst.) pb. The cross section value assumes a top quark mass of m{sub t} is presented in the paper. This result is cons…

Top quarkCollider physicsHadronTevatronGeneral Physics and AstronomyElementary particleKinematicsElectronJet (particle physics)01 natural sciences7. Clean energyParticle identificationlaw.inventionlawInvariant massFermilabNuclear ExperimentQuantum chromodynamicsPhysicsLarge Hadron ColliderLuminosity (scattering theory)Supersymmetryb-taggingHadronizationTransverse planeProduction (computer science)Collider Detector at FermilabQuarkSemileptonic decayNuclear and High Energy PhysicsParticle physicsBar (music)Astrophysics::High Energy Astrophysical PhenomenaBottom quarkMeasure (mathematics)Standard ModelNuclear physicsCross section (physics)Particle decay0103 physical sciencesCollider010306 general physicsCompact Muon SolenoidMuonBranching fraction010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyMultiplicity (mathematics)FermionVertex (geometry)Pair productionHigh Energy Physics::ExperimentEnergy (signal processing)Bar (unit)LeptonPhysical Review D
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Combination of D0 measurements of the top quark mass

2017

We present a combination of measurements of the top quark mass by the D0 experiment in the lepton+jets and dilepton channels. We use all the data collected in Run I (1992--1996) at $\sqrt s=1.8$ TeV and Run II (2001--2011) at $\sqrt s=1.96$ TeV of the Tevatron $p \bar{p}$ collider, corresponding to integrated luminosities of 0.1 fb$^{-1}$ and 9.7 fb$^{-1}$, respectively. The combined result is: $m_t = 174.95 \pm0.40\,{\rm(stat)} \pm 0.64\,{\rm(syst)}\,{\rm{GeV}}=174.95 \pm 0.75 \, {\rm{GeV}}$.

Top quarkQ007TPtop: mass: measured((n)jet dilepton) [final state]Tevatronpair production [top]01 natural scienceslaw.inventionPhysics Particles & FieldsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)lawDZERO[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Batavia TEVATRON CollNuclear ExperimentPhysicsscattering [anti-p p]PhysicsGLOBAL QCD ANALYSISDetectorROOT-S=7ATLASPhysical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGmass: measured [top]top: pair production((n)jet lepton) [final state]Particle physics1800 GeV-cms1960 GeV-cmsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesfinal state: ((n)jet lepton)Astronomy & Astrophysicsanti-p p: colliding beamsNuclear physicsEVENTS[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesanti-p p: scatteringddc:530Combined resultHigh Energy Physics010306 general physicsColliderDETECTORScience & TechnologyPP COLLISIONS1960 GeV-cms010308 nuclear & particles physicsfinal state: ((n)jet dilepton)hep-exHigh Energy Physics::PhenomenologyD0 experimentDIFFERENCEPARTON DISTRIBUTIONSExperimental High Energy PhysicsPhysics::Accelerator PhysicsTEVHigh Energy Physics::Experiment1800 GeV-cmscolliding beams [anti-p p]Leptonexperimental results
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Precise measurement of the top quark mass in dilepton decays using optimized neutrino weighting

2016

We measure the top quark mass in dilepton final states of top-antitop events in proton-antiproton collisions at sqrt(s) = 1.96 TeV, using data corresponding to an integrated luminosity of 9.7 fb^-1 at the Fermilab Tevatron Collider. The analysis features a comprehensive optimization of the neutrino weighting method to minimize the statistical uncertainties. We also improve the calibration of jet energies using the calibration determined in top-antitop to lepton+jets events, which reduces the otherwise limiting systematic uncertainty from the jet energy scale. The measured top quark mass is mt = 173.32 +/- 1.36(stat) +/- 0.85(syst) GeV.

Top quarkdependence [flavor]TevatronATLAS DETECTORJet (particle physics)pair production [top]7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentPhysics Particles & FieldsSubatomär fysikHigh Energy Physics - Experiment (hep-ex)DZEROSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]HADRON COLLIDERSBatavia TEVATRON CollFermilabNuclear ExperimentGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)Physicsscattering [anti-p p]Luminosity (scattering theory)PhysicsNuclear & Particles Physicslcsh:QC1-999Physics NuclearPhysical SciencesPOLEflavor [quark]mass: measured [top]Neutrinotop quark mass; dilepton decays; neutrino weightingdata analysis methodParticle physicsNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaSTANDARD MODELFOS: Physical sciencesAstronomy & AstrophysicsAccelerator Physics and Instrumentation530Standard ModelNuclear physics0202 Atomic Molecular Nuclear Particle And Plasma Physicsfinal state [dilepton]0103 physical sciencesMODEL HIGGS-BOSONddc:530High Energy Physics010306 general physics1960 GeV-cmsScience & TechnologyPP COLLISIONSIDENTIFICATION010308 nuclear & particles physicsDATA processing & computer scienceHigh Energy Physics::PhenomenologyAcceleratorfysik och instrumenteringenergy [jet]PRODUCTION CROSS-SECTION(MS)OVER-BAR MASSEScalibration [jet]Experimental High Energy PhysicsPhysics::Accelerator PhysicsTEVHigh Energy Physics::Experimentddc:004statisticalcolliding beams [anti-p p]lcsh:Physicsexperimental resultsLepton
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Charged and Neutral Current Neutrino Induced Nucleon Emission Reactions

2006

Presented by J. Nieves at the XX Max Born Symposium “Nuclear Effects in Neutrino Interactions”, Wrocław, Poland, December 7–10, 2005.

UNESCO::FÍSICA::NucleónicaAstrophysics::High Energy Astrophysical PhenomenaNuclear TheoryUNESCO::FÍSICAFOS: Physical sciencesMonte Carlo cascade method:FÍSICA::Nucleónica [UNESCO]Nucleon emissionHigh Energy Physics - PhenomenologyNeutrino experimentsHigh Energy Physics - Phenomenology (hep-ph):FÍSICA [UNESCO]Monte Carlo cascade method ; Nucleon emission ; Neutrino experimentsNuclear Experiment
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Trigger and aperture of the surface detector array of the Pierre Auger Observatory

2010

The surface detector array of the Pierre Auger Observatory consists of 1600 water-Cherenkov detectors, for the study of extensive airshowers (EAS) generated by ultra-high-energy cosmic rays. We describe the trigger hierarchy, from the identification of candidates howers at the level of a single detector, amongst a large background (mainly random single cosmic ray muons), up to the selection of real events and the rejection of random coincidences. Such trigger makes the surface detector array fully efficient for the detection of EAS with energy above 3 x 1018 eV, for all zenith angles between 03 and 603, independently of the position of the impact point and of the mass of the primary particl…

Ultra high energy cosmic rays; Auger Observatory; Extensive air showers; Trigger; ExposurePhysics::Instrumentation and DetectorsAstronomyHigh-Energy Cosmi Ray7. Clean energy01 natural sciencesAugerAcceptance and Trigger Efficiency010303 astronomy & astrophysicsInstrumentationComputingMilieux_MISCELLANEOUSPhysicsRange (particle radiation)PhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryHigh energyFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsNuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]AIR SHOWERSApertureInstrumentationAstrophysics::High Energy Astrophysical PhenomenaExtensive air showerFOS: Physical sciencesCosmic rayENERGIACosmic RayUltra high energy cosmic rayExposureOpticsultra high energy cosmic rays Auger Observatory extensive airshowers trigger exposure0103 physical sciencesPARTICLESExtensive air showersSurface DetectorInstrumentation and Methods for Astrophysics (astro-ph.IM)ZenithCiencias ExactasNuclear and High Energy PhysicPierre Auger Observatory010308 nuclear & particles physicsbusiness.industryFísicaUltra high energy cosmic raysUltra-high energy cosmic rays[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]TriggerAuger ObservatoryExperimental High Energy PhysicsHigh Energy Physics::Experimentbusiness
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Quasi-periodic dipping in the ultraluminous X-ray source, NGC 247 ULX-1

2021

Most ultraluminous X-ray sources (ULXs) are believed to be stellar mass black holes or neutron stars accreting beyond the Eddington limit. Determining the nature of the compact object and the accretion mode from broadband spectroscopy is currently a challenge, but the observed timing properties provide insight into the compact object and details of the geometry and accretion processes. Here we report a timing analysis for an 800 ks XMM-Newton campaign on the supersoft ultraluminous X-ray source, NGC 247 ULX-1. Deep and frequent dips occur in the X-ray light curve, with the amplitude increasing with increasing energy band. Power spectra and coherence analysis reveals the dipping preferential…

Ultraluminous X-ray sourceStellar massAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCompact star01 natural sciencesSpectral linesymbols.namesakeX-rays: binariesaccretion0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAccretion (meteorology)010308 nuclear & particles physicsAstronomy and AstrophysicsLight curveaccretion discsX-rays: individual: NGC 247 ULX-1Neutron starSpace and Planetary ScienceEddington luminositysymbolsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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"Table 4" of "J/$\psi$ elliptic flow in Pb-Pb collisions at $\mathbf{\sqrt{s_{\rm NN}}}$ = 5.02 TeV"

2017

Transverse momentum dependence of inclusive J/$\psi$ $v_2$ at $\sqrt{s_{\rm NN}}=5.02$ TeV for the 40-60% centrality class (forward rapidity). The first uncertainty (stat) is statistical, the second (sys,uncorrel) is the uncorrelated systematic, while the third one (sys,correl) is a $p_{\rm T}$-correlated systematic uncertainty.

V25020.0PB PB --> J/PSI XAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::ExperimentNuclear Experiment
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"Table 2" of "J/$\psi$ elliptic flow in Pb-Pb collisions at $\mathbf{\sqrt{s_{\rm NN}}}$ = 5.02 TeV"

2017

Transverse momentum dependence of inclusive J/$\psi$ $v_2$ at $\sqrt{s_{\rm NN}}=5.02$ TeV for the 20-40% centrality class (mid-rapidity). The first uncertainty (stat) is statistical, the second (sys,uncorrel) is the uncorrelated systematic, while the third one (sys,correl) is a $p_{\rm T}$-correlated systematic uncertainty.

V25020.0PB PB --> J/PSI XAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::ExperimentNuclear Experiment
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"Table 1" of "J/$\psi$ elliptic flow in Pb-Pb collisions at $\mathbf{\sqrt{s_{\rm NN}}}$ = 5.02 TeV"

2017

Transverse momentum dependence of inclusive J/$\psi$ $v_2$ at $\sqrt{s_{\rm NN}}=5.02$ TeV for the 20-40% centrality class (forward rapidity). The first uncertainty (stat) is statistical, the second (sys,uncorrel) is the uncorrelated systematic, while the third one (sys,correl) is a $p_{\rm T}$-correlated systematic uncertainty.

V25020.0PB PB --> J/PSI XAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::ExperimentNuclear Experiment
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"Table 3" of "J/$\psi$ elliptic flow in Pb-Pb collisions at $\mathbf{\sqrt{s_{\rm NN}}}$ = 5.02 TeV"

2017

Transverse momentum dependence of inclusive J/$\psi$ $v_2$ at $\sqrt{s_{\rm NN}}=5.02$ TeV for the 5-20% centrality class (forward rapidity). The first uncertainty (stat) is statistical, the second (sys,uncorrel) is the uncorrelated systematic, while the third one (sys,correl) is a $p_{\rm T}$-correlated systematic uncertainty.

V25020.0PB PB --> J/PSI XAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::ExperimentNuclear Experiment
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