0000000000263932

AUTHOR

Jan Ridky

showing 27 related works from this author

Measurement of the lifetime of tau-lepton

1996

The tau lepton lifetime is measured with the L3 detector at LEP using the complete data taken at centre-of-mass energies around the Z pole resulting in tau_tau = 293.2 +/- 2.0 (stat) +/- 1.5 (syst) fs. The comparison of this result with the muon lifetime supports lepton universality of the weak charged current at the level of six per mille. Assuming lepton universality, the value of the strong coupling constant, alpha_s is found to be alpha_s(m_tau^2) = 0.319 +/- 0.015(exp.) +/- 0.014 (theory). The tau lepton lifetime is measured with the L3 detector at LEP using the complete data taken at centre-of-mass energies around the Z pole resulting in τ τ =293.2 ± 2.0 (stat) ± 1.5 (syst) fs . The c…

COLLISIONSNuclear and High Energy PhysicsParticle physicsLUND MONTE-CARLOPAIR PRODUCTIONElectron–positron annihilationFOS: Physical sciencesElementary particleddc:500.201 natural sciences7. Clean energyResonance (particle physics)JET FRAGMENTATIONDECAYSHigh Energy Physics - ExperimentNuclear physicsParticle decayHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SILICON MICROVERTEX DETECTORPRECISE MEASUREMENTLimit (mathematics)QCD ANALYSIS010306 general physicsL3 EXPERIMENTCoupling constantPhysicsMuonAnnihilationTEST BEAME+E-PHYSICS010308 nuclear & particles physicsALPHA(S)High Energy Physics::PhenomenologyDetectorPair productionSPECTRAL FUNCTIONSComputingMethodologies_DOCUMENTANDTEXTPROCESSINGHigh Energy Physics::ExperimentParticle Physics - ExperimentLeptonNuclear and Particle Physics Proceedings
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A search for neutral higgs particles in Z$^0$ decays

1992

Abstract The search in DELPHI data for neutral Higgs bosons is described. No candidate for the Standard Model Higgs is seen in Z0 decays to H 0 ν ν , H 0 μ + μ − or H0τ+τ− after selections that proved efficient for finding simulated H0. One remaining candidate for Z0 → H0e+e− is consistent with background. Together with our earlier studies, these results restrict the H0 mass to be above 38 GeV/c2 at the 95% confidence level. No signal is found for decays of Minimal Supersymmetric Standard Model neutral Higgs bosons to τ+τ−. Limits are obtained for their decays to produce four jets.

Nuclear and High Energy PhysicsParticle physicsElectron–positron annihilationSTANDARD MODEL01 natural sciencesLower limitStandard ModelNuclear physicsPHYSICSLIMITS0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsBosonPhysicsMASS SCALAR BOSONLIGHT SCALAR010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyZ0 DECAYE+E COLLISIONSSupersymmetrySUPERSYMMETRIC MODELSLEPNUCLEAR DECAYHiggs bosonHigh Energy Physics::ExperimentFísica nuclearMASS SCALAR BOSON; Z0 DECAY; SUPERSYMMETRIC MODELS; STANDARD MODEL; E+E COLLISIONS; NUCLEAR DECAY; LIGHT SCALAR; LIMITS; LEP; PHYSICSParticle Physics - ExperimentMinimal Supersymmetric Standard Model
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Performance of the DELPHI detector

1996

DELPHI (DEtector with Lepton, Photon and Hadron Identification) is a detector for e(+)e(-) physics, designed to provide high granularity over a 4 pi solid angle, allowing an effective particle identification, It has been operating at the LEP (Large Electron-Positron) collider at CERN since 1989. This article reviews its performance.

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsENERGIESHadronDENSITY PROJECTION CHAMBER; IMAGING CHERENKOV DETECTOR; RADIATIVE-CORRECTIONS; LEP; SIMULATION; ENERGIES; Z(0); SCATTERING; PROGRAM; SYSTEM01 natural sciencesPartícules (Física nuclear)Particle identificationlaw.inventionNuclear physicslaw0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]PROGRAMRADIATIVE-CORRECTIONSSCATTERINGDetectors and Experimental Techniques010306 general physicsColliderInstrumentationDELPHINuclear and High Energy PhysicPhysicsLarge Hadron Colliderhigh granularityCalorimeter (particle physics)LEP; DELPHI; high granularity; particle identification010308 nuclear & particles physicsDetectorHigh Energy Physics::PhenomenologyLEPZ(0)LARGE ELECTRON POSITRON COLLIDERIMAGING CHERENKOV DETECTORFIS/01 - FISICA SPERIMENTALEPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHILarge Electron–Positron ColliderSIMULATIONPARTICLE PHYSICSPhysics::Accelerator PhysicsFísica nuclearHigh Energy Physics::ExperimentDENSITY PROJECTION CHAMBERparticle identificationSYSTEMLepton
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Observation of orbitally excited B mesons

1995

Experimental evidence for the existence of orbitally excited B meson states is presented in an analysis of the Bπ and B*π distribution of Q = m(B**) - m(B(*)) - m(π) using Z0decay data taken with the DELPHI detector at LEP. The mean Q-value of the decays B**→ B(*)π is measured to be 284 ± 5 (stat.) ± 15 (syst.) MeV/c2, and the Gaussian width of the signal is 79 ± 5 (stat.) ± 8 (syst.) MeV/c2. This signal can be described as a single resonance of mass m = 5732 ± 5 (stat.) ± 20 (syst.) MeV/c2and full width Γ = 145 ± 28 MeV/c2. The observed shape is also consistent with the production of several broad and narrow states as predicted by the quark model and partly observed in the D-…

Nuclear and High Energy PhysicsE+E ANNIHILATIONLUND MONTE-CARLOElectron–positron annihilationDELPHI; B meson; fragmentation; b-jetB meson01 natural sciencesResonance (particle physics)Full widthPartícules (Física nuclear)JET FRAGMENTATIONDECAYSNuclear physicsPHYSICSfragmentation0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]B meson010306 general physicsNuclear ExperimentDetectors de radiacióDELPHIPhysics010308 nuclear & particles physicsQuark modelb-jetLARGE ELECTRON POSITRON COLLIDERExcited statePARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSHigh Energy Physics::ExperimentLUND MONTE-CARLO; JET FRAGMENTATION; E+E ANNIHILATION; DECAYS; PHYSICSParticle Physics - ExperimentProduction ratePhysics Letters B
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A Search for Sleptons and Gauginos in Z0 Decays

1990

Using a data sample corresponding to 10 000 hadronic Z0 decays, we have searched for the production of sleptons and gauginos in the two-prong decays of Z0. No candidate remains after straightforward selections. For neutralinos, we use selection methods developed in our previous search for neutral Higgs particles. The negative results are translated into improved mass limits and parameter constraints on the minimal supersymmetric extension of the standard model.

PhysicsParticle physicsNuclear and High Energy Physics010308 nuclear & particles physicsElectron–positron annihilationHadronHigh Energy Physics::Phenomenology01 natural sciencesStandard Model0103 physical sciencesHiggs bosonPhysique des particules élémentairesFísica nuclearHigh Energy Physics::ExperimentSelection method010306 general physicsParticle Physics - Experiment
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Search for heavy charged scalars in Z$^0$ Decays

1990

Using a sample of Z0's corresponding to about 12 000 events, we have searched for the production of charged scalars, primarily charged Higgs particles, decaying into c̄scs̄, τν+jets, and τντν. The average detection efficiency is 20%. No candidate was found in the leptonic modes. Masses in the range up to 30-36 GeV/c2 are excluded, extending the mass domain covered by previous e+e- machines.

PhysicsNuclear and High Energy PhysicsParticle physicsRange (particle radiation)Internet010308 nuclear & particles physicsElectron–positron annihilation01 natural sciencesteachingNuclear physics0103 physical sciencesDomain (ring theory)course packsPhysique des particules élémentairesHiggs bosonComputingMilieux_COMPUTERSANDEDUCATIONeditors[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics::ExperimentFísica nuclear010306 general physicsParticle Physics - Experiment
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A comparison of jet production rates on the Z0 resonance to perturbative QCD

1990

The production rates for 2-, 3-, 4- and 5-jet hadronic final states have been measured with the DELPHI detector at the e+e- storage ring LEP at centre of mass energies around 91.5 GeV. Fully corrected data are compared to O(αs 2) QCD matrix element calculations and the QCD scale parameter ΛMS is determined for different parametrizations of the renormalization scale μ2. Including all uncertainties our result is αs(MZ 2)=0.114±0.003[stat.]±0.004[syst.]±0.012[theor.] .

PhysicsQuantum chromodynamicsParticle physicsNuclear and High Energy Physics010308 nuclear & particles physicsElectron–positron annihilationHadronPerturbative QCDJet (particle physics)01 natural sciences7. Clean energyResonance (particle physics)Nuclear physicsRenormalization0103 physical sciencesPhysique des particules élémentairesHigh Energy Physics::Experiment010306 general physicsStorage ringParticle Physics - Experiment
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A measurement of the tau lifetime

1993

The tau lepton lifetime is measured using four different methods with the DELPHI detector. Three measurements using one prong decays are combined, accounting for correlations, resulting in tau(tau) = 298 +/- 7 (stat.) +/- 4 (syst.) fs while the decay length distribution of three prong decays gives tau(tau) = 298 +/- 13 (stat.) +/- 5 (syst.) fs. The combined result is tau(tau) = 298 +/- 7 fs. The ratio of the Fermi coupling constant from tau decay relative to that from muon decay is found to be 0.985 +/- 0.013, compatible with lepton universality.

PhysicsCoupling constantParticle physicsArgusNuclear and High Energy PhysicsMuonPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsElectron–positron annihilation01 natural sciences7. Clean energyNuclear physics0103 physical sciencesDecay lengthLEPTONS[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics::ExperimentFísica nuclearCombined result010306 general physicscomputerParticle Physics - ExperimentFermi Gamma-ray Space TelescopeLeptoncomputer.programming_language
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Measurement of $\mbox{B}^0_d$ - $\overline{\mbox{B}^0_d}$ oscillations

1997

PhysicsNuclear magnetic resonancePhysics and Astronomy (miscellaneous)010308 nuclear & particles physics0103 physical sciences010306 general physics01 natural sciencesZeitschrift f�r Physik C Particles and Fields
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Design and implementation of the AMIGA embedded system for data acquisition

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and admin-istrative staff in Malargtie. We are very grateful to the following agencies and organizations for financial support: Comision Nacional de Energla Atomica, Agencia Nacional de Promocion Cientffica y Tec-nologica (ANPCyT) , Consejo Nacional de Investigaciones Cientfficas y Tecnicas (CONICET) , Gobierno de la Provincia de Mendoza, Municipalidad de Malargtie, NDM Holdings and Valle Las Leilas, in gratitude for their continuing cooperation over land access, Argentina; the Australian Research Council; Conselho…

muon: showersDetector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases)Physics::Instrumentation and Detectorsdata acquisitionAstronomycosmic radiation: electromagnetic componentengineeringprimary [cosmic radiation]Particle detectors01 natural sciencesenergy: thresholdData acquisition concepthardwareInstrumentationMathematical Physicsshowers [muon]media_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEControl and monitor systems onlinePhysicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsthreshold [energy]16. Peace & justiceAugerelectromagnetic component [cosmic radiation]observatoryDetector control systems (detector andexperiment monitoring and slow-control systemslanguageupgradeAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical Phenomenadatabases)atmosphere [showers]Land accessarchitectureEuropean communityairAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesalgorithmsPolitical science0103 physical sciencesmedia_common.cataloged_instanceddc:530High Energy Physics[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]ddc:610Control and monitor systems online; Data acquisition concepts; Detector control systems (detector and experiment monitoring and slow-control systems architecture hardware algorithms databases); Particle detectorsEuropean union010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Ciencias Exactasscintillation countershowers: atmosphere010308 nuclear & particles physicsDetector control systems (detector and experiment monitoring and slow-control systemsData acquisition conceptsFísicastabilitylanguage.human_languagecosmic radiation: primarymonitoringResearch councilExperimental High Energy PhysicsHigh Energy Physics::ExperimentControl and monitor systems on-linePortuguese[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HumanitiesRAIOS CÓSMICOSastro-ph.IM
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The Fluorescence Detector of the Pierre Auger Observatory

2010

The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays. It combines a surface array to measure secondary particles at ground level together with a fluorescence detector to measure the development of air showers in the atmosphere above the array. The fluorescence detector comprises 24 large telescopes specialized for measuring the nitrogen fluorescence caused by charged particles of cosmic ray air showers. In this paper we describe the components of the fluorescence detector including its optical system, the design of the camera, the electronics, and the systems for relative and absolute calibration. We also discuss the operation and the monitoring of the detecto…

Physics::Instrumentation and DetectorsAstronomyAUGERPIERRE7. Clean energy01 natural sciencesAugerFluorescence detectorData acquisitionDEPENDENCEATMOSPHERIC MULTIPLE-SCATTERINGInstrumentationPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsCOSMIC-RAYSUltra High Energy Cosmic RayCharged particleLIGHTSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAUGERNuclear and High Energy Physics[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaMeasure (physics)FOS: Physical sciencesCosmic rayEXTENSIVE AIR-SHOWERSENERGIAFluorescence spectroscopyOptics0103 physical sciencesCosmic rays; Fluorescence detectorRECONSTRUCTION010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger ObservatoryPIERRE010308 nuclear & particles physicsbusiness.industryFísicaULTRA-HIGH ENERGY[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Experimental High Energy PhysicsPierre Auger observatoryCAPABILITIESHigh Energy Physics::Experimentbusiness
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Searches for heavy neutrinos from Z decays

1992

We have searched for possible fourth family heavy neutrinos, pair produced in Z0 decays, in a sample of about 112 000 hadronic Z0 final states collected with the DELPHI detector. For all mixing matrix elements we exclude a new Dirac neutrino lighter than 44.5 GeV at a 95% confidence level, if the neutrino couples to the electron or muon family, and lighter than 44.0 GeV, if the neutrino couples to the tau family. Depending on the values of the mixing element and to which lepton family the neutrino couples, we obtain mass limits up to 46.2 GeV. For all mixing matrix elements we exclude a new Majorana neutrino lighter than 39.0 GeV, if it couples to the electron or the muon family, and lighte…

Z-PEAK; LEPTONS; RESONANCE; LIMITS; QUARKSNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaElectron–positron annihilationHadron01 natural sciencesNuclear physicsLIMITS0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]QUARKSNuclear Experiment010306 general physicsMixing (physics)PhysicsMuon010308 nuclear & particles physicsDirac (video compression format)High Energy Physics::PhenomenologyRESONANCEZ-PEAKMAJORANALEPTONSPhysique des particules élémentairesFísica nuclearHigh Energy Physics::ExperimentNeutrinoParticle Physics - ExperimentLepton
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Testing effects of Lorentz invariance violation in the propagation of astroparticles with the Pierre Auger Observatory

2021

The successful installation, commissioning, and operation of the Pierre Auger Observatory would not have been possible without the strong commitment and effort from the technical and administrative staff in Malargüe. We are very grateful to the following agencies and organizations for financial support: Argentina — Comisión Nacional de Energía Atómica; Agencia Nacional de Promoción Científica y Tecnológica (ANPCyT); Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET); Gobierno de la Provincia de Mendoza; Municipalidad de Malargüe; NDM Holdings and Valle Las Leñas; in gratitude for their continuing cooperation over land access; Australia — the Australian Research Council; Be…

interaction [cosmic radiation]mass spectrum [cosmic radiation]dispersion relationAstronomyAstrophysics::High Energy Astrophysical Phenomenaenergy spectrumcosmic ray experimentFOS: Physical sciencesultra high energy cosmic rayscosmic radiation: interactioninvariance: Lorentz01 natural sciences530UHEultra high energy cosmic rayenergy: thresholdFundamental physics gravitational waves LISA Tests of general relativityCosmic ray experiments0103 physical sciencespropagationddc:530physics of the early universeHigh Energy PhysicsLorentz [invariance]010303 astronomy & astrophysicsphoton: fluxflux [photon]Lorentz [violation]High Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEenergy: high010308 nuclear & particles physicscosmic radiation: mass spectrumcosmic ray experiments; ultra high energy cosmic rays; physics of the early universeSettore FIS/01 - Fisica SperimentaleAstronomy and AstrophysicsASTROFÍSICAUltra-high energy cosmic raysthreshold [energy]violation: LorentzAugerobservatoryelectromagnetickinematicsExperimental High Energy Physicshigh [energy]cosmic ray experimentsAstrophysics - High Energy Astrophysical PhenomenaPhysics of the early universe
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Search For Light Neutral Higgs Particles Produced In Z0-decays

1990

A search for the neutral Higgs boson in Z0-decays has been performed using the DELPHI detector at the Large Electron Positron collider (LEP) at CERN. We looked for the decay of Z0 into a neutral Higgs particle and a pair of fermions. No events fulfilled the criteria for H0-production. Our results, which are based on an integrated luminosity of 530 nb-1, exclude a minimal Standard Model Higgs boson with a mass in the range 210 MeV/c2 to 14 GeV/c2 at 95% confidence level.

PhysicsNuclear and High Energy PhysicsParticle physicsLarge Hadron ColliderLuminosity (scattering theory)010308 nuclear & particles physicsElectron–positron annihilationHigh Energy Physics::PhenomenologyElementary particleFermion01 natural sciences7. Clean energyStandard ModelNuclear physics0103 physical sciencesLarge Electron–Positron ColliderPhysique des particules élémentairesHiggs boson[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Física nuclearHigh Energy Physics::Experiment010306 general physicsParticle Physics - Experiment
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Muons in air showers at the Pierre Auger Observatory

2015

We present the first hybrid measurement of the average muon number in air showers at ultrahigh energies, initiated by cosmic rays with zenith angles between 62° and 80°. The measurement is based on 174 hybrid events recorded simultaneously with the surface detector array and the fluorescence detector of the Pierre Auger Observatory. The muon number for each shower is derived by scaling a simulated reference profile of the lateral muon density distribution at the ground until it fits the data. A 1019eV shower with a zenith angle of 67°, which arrives at the surface detector array at an altitude of 1450 m above sea level, contains on average (2.68±0.04±0.48(sys))×107 muons with energies large…

[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Nuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsCosmic-ray interactionsAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayextensive atmospherical showers muon density muon number Pierre Auger Observatory cosmic radiation UHEHadronic interaction models7. Clean energyAugerSettore FIS/04 - Fisica Nucleare e SubnucleareNuclear physicsAltitudeSettore FIS/05 - Astronomia e AstrofisicaObservatoryNERGY COSMIC-RAYS DETECTOR MODEL.Extensive air showerscosmic radiation UHEDETECTORScalingCosmic raysZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryMuonNERGY COSMIC-RAYSSettore FIS/01 - Fisica Sperimentaleenergy cosmic-rays; detector; modelAstrophysics::Instrumentation and Methods for AstrophysicsFísica[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Pierre Auger ObservatoryASTROFÍSICAextensive atmospherical showersmuon numberMODELmuon densityExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaPhysical Review D
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A study of intermittency in Hadronic Z$^0$ Decays

1990

The correlations in rapidity in hadron production from e+e- annihilation near the Z0 resonance were studied by means of the method of factorial moments, using data taken with the DELPHI detector at LEP. The parton shower hadronization model was found to be in quantitative agreement with the data, in contrast with previous results at lower energies. © 1990.

Nuclear and High Energy PhysicsParticle physicsHadron7. Clean energy01 natural sciencesResonance (particle physics)hypertextlaw.inventionauthorNuclear physicslawIntermittency0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]RapidityNuclear Experiment010306 general physicsParton showerComputingMilieux_MISCELLANEOUSPhysicsAnnihilation010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHadronizationlectorMoment (physics)Physique des particules élémentairesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearHigh Energy Physics::ExperimentParticle Physics - Experimenttext
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A precise measurement of the Z resonance parameters through its hadronic decays

1990

A measurement of the cross section for e+e-→ hadrons using 11 000 hadronic decays of the Z boson at ten different center-of-mass energies is presented. A three-parameter fit gives the following values for the Z mass MZ, the total width ΓZ, the product of the electronic and hadronic partial widths ΓeΓh, and the unfolded pole cross section σ0: MZ = 91.171 ± 0.030 (stat.) ± 0.030 (beam) GeV, ΓZ = 2.511 ± 0.065 GeV, ΓeΓh = 0.148 ± 0.006 (stat.) ± 0.004 (syst.) GeV2, σ0 = 41.6 ± 0.7 (stat.) ± 1.1 (syst.) nb, Good agreement with the predictions of the standard model is observed. From a two-parameter fit the number of massless neutrino generations is found to be Nv = 2.91 ± 0.26. Thus the hypothes…

Nuclear and High Energy PhysicsParticle physics[PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex]pragmatismtruthElectron–positron annihilationHadronfictionpossible worlds01 natural sciencesResonance (particle physics)webStandard ModelRDFNuclear physicsCross section (physics)semantic webesthetics0103 physical sciencesmemetic[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNuclear Experimentmetalanguagemodal logicPhysicsInternet010308 nuclear & particles physicstrust3. Good healthMassless particlePhysique des particules élémentairesHigh Energy Physics::ExperimentFísica nuclearNeutrinoBeam (structure)Particle Physics - Experiment
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Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

2010

Data collected by the Pierre Auger Observatory through 31 August 2007 showed evidence for anisotropy in the arrival directions of cosmic rays above the Greisen-Zatsepin-Kuz'min energy threshold, 6 x 10(19) eV. The anisotropy was measured by the fraction of arrival directions that are less than 3.1 degrees from the position of an active galactic nucleus within 75 Mpc (using the Veron-Cetty and Veron 12th catalog). An updated measurement of this fraction is reported here using the arrival directions of cosmic rays recorded above the same energy threshold through 31 December 2009. The number of arrival directions has increased from 27 to 69, allowing a more precise measurement. The correlating…

AstronomyAstrophysicsUltra High Energy Cosmic ray01 natural scienceslaw.inventionObservatorylawAnisotropy010303 astronomy & astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]UHECRAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryGZKAnisotropíaGALAXIESNEUTRINOSGreisen–Zatsepin–Kuz’minComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaACTIVE GALACTIC NUCLEIHIPASS CATALOG[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Active galactic nucleusRadiación Cósmicamedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsTelescope0103 physical sciencesCosmic raysCiencias ExactasAstrophysics::Galaxy AstrophysicsPierre Auger ObservatorySPECTRUM010308 nuclear & particles physicsAstronomyFísicaAstronomy and AstrophysicsCosmic rayGalaxyCorrelation with astrophysical sourcesCosmic rays; UHECR; Anisotropy; Pierre Auger Observatory; Extra-galactic; GZKSkyExperimental High Energy PhysicsAnisotropyExtra-galactic
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Study of the leptonic decays of the Z0 boson

1990

Measurements are presented of the cross section ratios Rℓ = σℓ(e+e-→ℓ+ℓ -)/σhh(e+e-→hadrons) for ℓ = e, μ and τ using data taken from a scan around the Z0. The results are Re = (5.09±0.32±0.18)%, Rμ = (4.96±0.35±0.17)% and Rτ,=(4.72±0.38± 0.29)% where, for the ratio Re, the t-channel contribution has been subtracted. These results are consistent with the hypothesis of lepton universality and test this hypothesis at the energy scale s ∼ 8300 GeV2. The absolute cross sections σℓ(e+e-→ℓ +ℓ-) have also been measured. From the cross sections the leptonic partial widths Γe = (83.2±3.0±2.4) MeV, (ΓeΓμ) 1/2=(84.6±3.0±2.4) MeV and (ΓeΓτ) 1/2=(82.6±3.3±3.2) MeV have been extracted. Assuming lepton un…

PhysicsNuclear and High Energy PhysicsParticle physics[PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex]010308 nuclear & particles physicsElectron–positron annihilationHadronWidth ratio01 natural sciences7. Clean energyNuclear physics0103 physical sciencesPhysique des particules élémentaires[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino010306 general physicsParticle Physics - ExperimentLeptonBosonPhysics Letters B
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Measurement of the radiation energy in the radio signal of extensive air showers as a universal estimator of cosmic-ray energy

2016

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8±0.7(stat)±6.7(syst) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principles calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the d…

Ciencias FísicasAstronomyGeneral Physics and Astronomyultra-high energy cosmic raysAstrophysics01 natural sciencesHigh Energy Physics - Experiment//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)CODALEMAObservatory[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]GeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsRange (particle radiation)Radio detectorTUNKA-REXSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsRadio TechniqueFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsradio emissionCIENCIAS NATURALES Y EXACTASRadio wave[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsPhysics and Astronomy (all)0103 physical sciencesextensive air showersHigh Energy Physicsultra-high energy cosmic rays extensive air showers radio emission010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Cosmic raysPierre Auger Observatory010308 nuclear & particles physicsRadiant energyFísicaLOFAR//purl.org/becyt/ford/1.3 [https]LOFARASTROFÍSICASIMULATIONSComputational physicsAstronomíaCOREASExperimental High Energy PhysicsARRAYEMISSION SIMULATIONS LOFAR.EMISSION
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Search for scalar quarks in Z0 decays

1990

A search has been made for pairs of scalar quarks (squarks) produced in e+e- annihilations at LEP (√s≃MZ0), and decaying into a standard quark and a neutral, non-interacting, stable, massive particle (the lightest supersymmetric particle, LSP). The search has been conducted for differences in the mass of the squark and LSP of 2 GeV/c2 and above. Up squarks with masses below 42 GeV/c2 and down squarks below 43 GeV/c2 were excluded. Six squark flavours degenerate in mass were excluded below 45 GeV/c2.

PhysicsQuarkNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsElectron–positron annihilationHigh Energy Physics::LatticeScalar (mathematics)Degenerate energy levelsHigh Energy Physics::PhenomenologyMassive particle01 natural sciencesLightest Supersymmetric ParticleNuclear physics0103 physical sciencesPhysique des particules élémentairesHigh Energy Physics::Experiment010306 general physicsNuclear ExperimentParticle Physics - Experiment
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Multiplicity dependence of mean transverse momentum in $e^+e^-$ annihilations at LEP energies

1992

A strong increase of the mean transverse momentum [p(t)] with the number of charged particles n(ch) is observed in e+e- annihilations into hadrons at LEP energies, The effect resembles correlations observed in hadron-hadron interactions. In e+e- annihilations the [p(t)] and n(ch) correlations can be accounted for by gluon radiation.

Nuclear and High Energy PhysicsParticle physicsCOLLISIONSElectron–positron annihilationHadronNuclear TheoryISR ENERGIESANTI-PROTON COLLIDER; ISR ENERGIES; COLLISIONS; SPECTRA; EVENTS; MATTER; QCDRadiation01 natural sciencesANTI-PROTON COLLIDERNuclear physicsEVENTS0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SPECTRAMultiplicity (chemistry)010306 general physicsNuclear ExperimentPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyQCDCharged particleGluonTransverse momentumFísica nuclearHigh Energy Physics::ExperimentMATTERParticle Physics - Experiment
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Determination of 55-155-155-1in second order QCD from hadronic Z decays

1992

Distributions of event shape variables obtained from 120600 hadronic Z decays measured with the DELPHI detector are compared to the predictions of QCD based event generators. Values of the strong coupling constant αs are derived as a function of the renormalization scale from a quantitative analysis of eight hadronic distributions. The final result, αs(MZ), is based on second order perturbation theory and uses two hadronization corrections, one computed with a parton shower model and the other with a QCD matrix element model. © 1992 Springer-Verlag.

Quantum chromodynamicsPhysicsParticle physicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsElectron–positron annihilationHadronHigh Energy Physics::Phenomenology01 natural sciencesHadronizationRenormalization0103 physical sciencesHigh Energy Physics::ExperimentPerturbation theory (quantum mechanics)010306 general physicsParton showerEngineering (miscellaneous)Event (particle physics)Zeitschrift für Physik C Particles and Fields
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Measurement of the partial width of the decay of the Z0 into charm quark pairs

1990

A determination of the partial width Γc̄ of the Z0 boson into charm quark pairs is presented, based on a total sample of 36 900 Z0 hadronic decays measured with the DELPHI detector at the LEP collider. The production rate of cc events is derived from the inclusive analysis of charged pions coming from the decay of charmed meson D*+-→D0π+ and D*-→D̄0π- where the π± is constrained by kinematics to have a low pT with respect to the jet axis. The probability to procedure these π± from D*± decay in cc events is taken to be 0.31±0.05 as measured at √S = 10.55 GeV. The measured relative partial width Γ∞/Γh = 0.162± 0.030(stat.) ± 0.050(syst.) is in good agreement with the standard model value of 0…

Nuclear and High Energy PhysicsParticle physicsE+E ANNIHILATIONMesonLUND MONTE-CARLOElectron–positron annihilationHadron01 natural sciencesJET FRAGMENTATIONCharm quarkStandard Modellaw.inventionNuclear physicsPHYSICSENERGYPionLUND MONTE-CARLO; D-STAR-MESON; E+E ANNIHILATION; JET FRAGMENTATION; CROSS-SECTION; PHYSICS; ENERGYlaw0103 physical sciences010306 general physicsColliderD-STAR-MESONNuclear ExperimentBosonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyPhysique des particules élémentairesFísica nuclearHigh Energy Physics::ExperimentCROSS-SECTIONParticle Physics - Experiment
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A measurement of the photon structure function F-2(gamma) at an average Q(2) of 12 GeV2/c(4)

1995

The hadronic photon structure function F_{2}^{gamma} has been measured in the Q^{2} range from 4 to 30~GeV^2/c^{4} and down to x values of order 0.001, using data taken with the DELPHI detector at LEP between 1991 and 1993. A comparison is made with several F_{2}^{gamma} parameterizations with special emphasis on their low x behaviour. A result on the Q^{2} evolution of F_{2}^{gamma} is presented.

Particle physicsPhotonPhysics and Astronomy (miscellaneous)LEP; DELPHI; hadronic photon structureHadronMONTE-CARLO SIMULATIONStructure (category theory)01 natural sciencesC-4Partícules (Física nuclear)JET FRAGMENTATIONlaw.inventionQ2Nuclear physicsMONTE-CARLO SIMULATION; STRUCTURE-FUNCTION F2; JET FRAGMENTATION; E+E-PHYSICS; QCD; Q2; SCATTERING; ORDERlaw0103 physical sciencesRange (statistics)SCATTERINGhadronic photon structure010306 general physicsDELPHIQuantum chromodynamicsPhysicsE+E-PHYSICS010308 nuclear & particles physicsScatteringEmphasis (telecommunications)DetectorOrder (ring theory)ORDERLEPQCDLARGE ELECTRON POSITRON COLLIDERPhoton structure functionPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIMass spectrumPARTICLE PHYSICSFísica nuclearSTRUCTURE-FUNCTION F2
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Features of the Energy Spectrum of Cosmic Rays above 2.5×10$^{18}$ eV Using the Pierre Auger Observatory

2020

We report a measurement of the energy spectrum of cosmic rays above $2.5{\times} 10^{18}$ eV based on $215,030$ events. New results are presented: at about $1.3{\times} 10^{19}$ eV, the spectral index changes from $2.51 \pm 0.03 \textrm{ (stat.)} \pm 0.05 \textrm{ (sys.)}$ to $3.05 \pm 0.05 \textrm{ (stat.)}\pm 0.10\textrm{ (sys.)}$, evolving to $5.1\pm0.3\textrm{ (stat.)} \pm 0.1\textrm{ (sys.)}$ beyond $5{\times} 10^{19}$ eV, while no significant dependence of spectral features on the declination is seen in the accessible range. These features of the spectrum can be reproduced in models with energy-dependent mass composition. The energy density in cosmic rays above $5{\times} 10^{18}$ eV …

FOS: Physical sciencespower spectrumGravitation and Astrophysics7. Clean energy01 natural sciences530energy dependencemass spectrumcosmic ray; astroparticle detectors; cosmic ray spectracosmic ray spectraastroparticle detectors5/30103 physical sciencesddc:530energy: densityUHE Cosmic Rays010303 astronomy & astrophysicscosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)Ultra-high energy cosmic rays energy spectrum astrophysical implications Cherenkov detectorscosmic radiation: energy spectrum010308 nuclear & particles physicsPhysicsAugerobservatoryEnergy SpectrumspectralAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]energy spectrum [cosmic radiation]density [energy]
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Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei

2008

Data collected by the Pierre Auger Observatory provide evidence for anisotropy in the arrival directions of the cosmic rays with the ighest-energies, which are correlated with the positions of relatively nearby active galactic nuclei (AGN) [Pierre Auger Collaboration, Science 318 (2007) 938]. The correlation has maximum significance for cosmic rays with energy greater than ~6 x 1019 eV and AGN at a distance less than ~75 Mpc. We have confirmed the anisotropy at a confidence level of more than 99% through a test with parameters specified a priori, using an independent data set. The observed correlation is compatible with the hypothesis that cosmic rays with the highest-energies originate fro…

[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomyOsservatorio Pierre AugerAstrophysicsGALAXY CLUSTER SURVEYAstrophysicsauger01 natural sciencesHigh energy cosmic rayRaggi cosmiciAstrophysical jetGMFObservatoryUltra-high-energy cosmic ray010303 astronomy & astrophysicsPhysicsBL-LACERTAEGreisen–Zatsepin–Kuz’min effect[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]ORIGINUHECRAstrophysics (astro-ph)Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryGZKRadiación cósmicaAnisotropíaCATALOGobservatoryddc:540EGMFCUTOFFComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRELATIVISTIC JETSActive galactic nucleusAstrophysics::High Energy Astrophysical PhenomenaCosmic background radiationFOS: Physical sciencesCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsACCELERATION[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesextra-galacticPARTICLESAGNAstrophysics::Galaxy AstrophysicsCiencias ExactasPierre Auger ObservatoryANISOTROPYhigh energy cosmic raysSciami atmosferici010308 nuclear & particles physicsFísicaAstronomyAstronomy and AstrophysicsCENTAURUSGalaxyExperimental High Energy Physics
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