Search results for "Shower"

showing 10 items of 151 documents

Measurement of pion and proton response and longitudinal shower profiles up to 20 nuclear interaction lengths with the ATLAS Tile calorimeter

2010

The response of pions and protons in the energy range of 20–180 GeV, produced at CERN's SPS H8 test-beam line in the ATLAS iron–scintillator Tile hadron calorimeter, has been measured. The test-beam configuration allowed the measurement of the longitudinal shower development for pions and protons up to 20 nuclear interaction lengths. It was found that pions penetrate deeper in the calorimeter than protons. However, protons induce showers that are wider laterally to the direction of the impinging particle. Including the measured total energy response, the pion-to-proton energy ratio and the resolution, all observations are consistent with a higher electromagnetic energy fraction in pion-indu…

Nuclear and High Energy PhysicsProtonTest-beamPion–proton responsePhysics::Instrumentation and DetectorsHadronMonte Carlo methodNuclear TheoryHadronic shower development01 natural sciencesElectromagnetic radiationPartícules (Física nuclear)Nuclear physicsPion0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Detectors and Experimental Techniques010306 general physicsNuclear ExperimentInstrumentationMonte Carlo simulationGEANT4Detectors de radiacióPhysicsCalorimeterLarge Hadron Collider010308 nuclear & particles physicsATLASLongitudinal shower profile for hadronsScintillation counterPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentParametrization
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Search for Galactic PeV gamma rays with the IceCube Neutrino Observatory

2013

Gamma-ray induced air showers are notable for their lack of muons, compared to hadronic showers. Hence, air shower arrays with large underground muon detectors can select a sample greatly enriched in photon showers by rejecting showers containing muons. IceCube is sensitive to muons with energies above ~500 GeV at the surface, which provides an efficient veto system for hadronic air showers with energies above 1 PeV. One year of data from the 40-string IceCube configuration was used to perform a search for point sources and a Galactic diffuse signal. No sources were found, resulting in a 90% C.L. upper limit on the ratio of gamma rays to cosmic rays of 1.2 x 10^(-3)for the flux coming from …

Nuclear and High Energy PhysicsTELESCOPEPoint sourcePhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsddc:500.201 natural sciences7. Clean energyIceCube Neutrino ObservatoryIceCubeHESS0103 physical sciencesddc:530MILAGRO010306 general physics010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsMuonGamma rayAstrophysics::Instrumentation and Methods for AstrophysicsPLANEGalactic planeAir showerPhysics and Astronomy13. Climate actionDISCOVERYMilagroMOLECULAR CLOUDSTEVRADIATIONHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical PhenomenaEMISSION
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Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory

2010

We report a measurement of the flux of cosmic rays with unprecedented precision and Statistics using the Pierre Auger Observatory Based on fluorescence observations in coincidence with at least one Surface detector we derive a spectrum for energies above 10(18) eV We also update the previously published energy spectrum obtained with the surface detector array The two spectra are combined addressing the systematic uncertainties and, in particular. the influence of the energy resolution on the spectral shape The spectrum can be described by a broken power law E-gamma with index gamma = 3 3 below the ankle which is measured at log(10)(E-ankle/eV) = 18 6 Above the ankle the spectrum is describe…

Nuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Radiación CósmicaAstronomyAstrophysics::High Energy Astrophysical Phenomenaenergy spectrumFluxFOS: Physical sciencesCosmic rayAstrophysicsElectronSURFACE DETECTORUPPER LIMITENERGIAPHOTON FRACTION01 natural sciencesSpectral lineAugerNuclear physicscosmic raysObservatorySHOWERS0103 physical sciencesHigh-Energy Cosmic Ray010306 general physicsCosmic raysCiencias ExactasPhysicsPierre Auger ObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Spectral densityFísicaPierre Auger ObservatoryCosmic rayELECTRONS3. Good healthPierre Auger Observatory; Cosmic rays; Energy spectrumSIMULATIONExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFluorescenciaARRAYFísica nuclearEnergy spectrumAstrophysics - High Energy Astrophysical PhenomenaSYSTEM
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AMADEUS-The acoustic neutrino detection test system of the ANTARES deep-sea neutrino telescope

2011

The AMADEUS (ANTARES Modules for the Acoustic Detection Under the Sea) system which is described in this article aims at the investigation of techniques for acoustic detection of neutrinos in the deep sea. It is integrated into the ANTARES neutrino telescope in the Mediterranean Sea. Its acoustic sensors, installed at water depths between 2050 and 2300 m, employ piezo-electric elements for the broad-band recording of signals with frequencies ranging up to 125 kHz. The typical sensitivity of the sensors is around - 145 dB re 1 V/mu Pa (including preamplifier). Completed in May 2008, AMADEUS consists of six "acoustic clusters", each comprising six acoustic sensors that are arranged at distanc…

Optical telescopesNuclear and High Energy PhysicsAcoustic devicesNeutrino detectionPreamplifierAmbient noise levelFOS: Physical sciencesLINENeutrino telescope01 natural sciencesOptical telescopeThermo-acoustic modelData acquisition0103 physical sciencesSHOWERSWATERPARTICLE-DETECTION14. Life underwater010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)InstrumentationRemote sensingPhysicsANTARES010308 nuclear & particles physicsSensorsDetectorAstronomyElementary particlesAcoustic waveAMADEUSAcoustic neutrino detectionAcoustic wavesNeutrino detectorAcoustic variables measurementthermo-acoustic model; amadeus; neutrino telescope; acoustic neutrino detection; antaresFISICA APLICADAFísica nuclearNeutrinoNeutrino telescopesComputer hardware description languagesAstrophysics - Instrumentation and Methods for AstrophysicsSignal detection
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Calibration of the RPC charge readout in the ARGO-YBJ experiment

2012

""The charge readout of Resistive Plate Chambers (RPCs) is implemented in the ARGO-YBJ experiment to measure the charged particle density of the shower front up to 10^4\\\/m^2, enabling the study of the primary cosmic rays with energies in the ''knee'' region. As the first time for RPCs being used this way, a telescope with RPCs and scintillation detectors is setup to calibrate the number of charged particles hitting a RPC versus its charge readout. Air shower particles are taken as the calibration beam. The telescope was tested at sea level and then moved to the ARGO-YBJ site for coincident operation with the ARGO-YBJ experiment. The charge readout shows good linearity with the particle de…

Optical telescopesNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsCamere a Piastre Resistive (RPC)Resistive plate chamberAstrophysics::High Energy Astrophysical PhenomenaCosmic raylaw.inventionTelescopeSettore FIS/05 - Astronomia E AstrofisicaOpticslawCoincidentAir showersCalibrationSea levelInstrumentationParticle densitiesCosmic raysResistive Plate Chambers Charge read-out Extended Air ShowersPhysicsAir showers Charge readout Dynamic range Knee regions Particle densities Resistive plate chambers; Calibration Charged particles Cosmic rays Experiments Optical telescopes Sea level Telescopes; Particle spectrometersResistive touchscreenScintillationDynamic rangeCharge readoutParticle spectrometersbusiness.industryCharged particlesSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsCharged particleAir showerCalibrazione della Risposta Analogica di RPCKnee regionsLettura Analogica di RPCCalibrationResistive plate chambersbusinessExperimentsTelescopes
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PenRed: An extensible and parallel Monte-Carlo framework for radiation transport based on PENELOPE

2021

Monte Carlo methods provide detailed and accurate results for radiation transport simulations. Unfortunately, the high computational cost of these methods limits its usage in real-time applications. Moreover, existing computer codes do not provide a methodology for adapting these kind of simulations to specific problems without advanced knowledge of the corresponding code system, and this restricts their applicability. To help solve these current limitations, we present PenRed, a general-purpose, stand-alone, extensible and modular framework code based on PENELOPE for parallel Monte Carlo simulations of electron-photon transport through matter. It has been implemented in C++ programming lan…

Parallel computingPhysics - Instrumentation and DetectorsAtomic Physics (physics.atom-ph)FortranRadiation transportFOS: Physical sciencesGeneral Physics and AstronomyParallel computingcomputer.software_genre01 natural sciencesPhysics - Atomic Physics010305 fluids & plasmasElectron-photon showers0103 physical sciencesCIENCIAS DE LA COMPUTACION E INTELIGENCIA ARTIFICIAL010306 general physicsMonte Carlo simulationcomputer.programming_languageMPICHbusiness.industryInstrumentation and Detectors (physics.ins-det)Construct (python library)Computational Physics (physics.comp-ph)Modular designPhysics - Medical PhysicsShared memoryHardware and ArchitectureProgramming paradigmDistributed memoryMPIMedical Physics (physics.med-ph)CompilerMedical physicsbusinessPhysics - Computational Physicscomputer
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PRODUCTION CHARACTERISTICS OF K-0 AND LIGHT MESON RESONANCES IN HADRONIC DECAYS OF THE Z(0)

1995

An analysis of inclusive production of K0and the meson resonances K*±(892), ρ0(770), f0(975) and f2(1270) in hadronic decays of the Z0is presented, based on about 973,000 multihadronic events collected by the DELPHI detector at LEP during 1991 and 1992. Overall multiplicities have been determined as 1.962±0.060 K0mesons, 0.712±0.067 K*±(892) and 1.21±0.15ρ0(770) per hadronic Z0decay. The average multiplicities of f0(975) for scaled momentum, xp, in the range 0.05≤xp≤0.6 and of f2(1270) for 0.05≤xp≤1.0 are 0.098±0.016 and 0.170±0.043 respectively. The f0(975) and ρ0(770)xp-spectra have similar shapes. The f2(1270)/ρ0(770) ratio increases with xp. The average multiplicities…

Particle physicsMesonPhysics and Astronomy (miscellaneous)LUND MONTE-CARLOElectron–positron annihilationHadron01 natural sciencesJET FRAGMENTATION250 GEV/CPartícules (Física nuclear)Nuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]multiplicityENERGY REGION010306 general physicsParton showerEngineering (miscellaneous)Detectors de radiacióDELPHI. inclusive production; K0 meson; multiplicity; MontecarloPhysicsRange (particle radiation)Momentum (technical analysis)010308 nuclear & particles physicsMultiplicity (mathematics)E+E-ANNIHILATIONINCLUSIVE PRODUCTIONZ0 DECAYSMontecarloParticle accelerationLUND MONTE-CARLO; E+E-ANNIHILATION; INCLUSIVE PRODUCTION; JET FRAGMENTATION; Z0 DECAYS; P INTERACTIONS; VECTOR-MESONS; ENERGY REGION; 250 GEV/C; 360 GEV/C360 GEV/CP INTERACTIONSK0 mesonDELPHI. inclusive productionVECTOR-MESONSParticle Physics - Experiment
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Electroweak Higgs production with HiggsPO at NLO QCD

2017

We present the HiggsPO UFO model for Monte Carlo event generation of electroweak $VH$ and VBF Higgs production processes at NLO in QCD in the formalism of Higgs pseudo-observables (PO). We illustrate the use of this tool by studying the QCD corrections, matched to a parton shower, for several benchmark points in the Higgs PO parameter space. We find that, while being sizable and thus important to be considered in realistic experimental analyses, the QCD higher-order corrections largely factorize. As an additional finding, based on the NLO results, we advocate to consider 2D distributions of the two-jet azimuthal-angle difference and the leading jet $p_T$ for new physics searches in VBF Higg…

Particle physicsPhysics and Astronomy (miscellaneous)530 PhysicsPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::LatticeMonte Carlo methodFOS: Physical scienceslcsh:Astrophysics10192 Physics InstituteParameter space01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Factorization0103 physical scienceslcsh:QB460-466lcsh:Nuclear and particle physics. Atomic energy. Radioactivity3101 Physics and Astronomy (miscellaneous)010306 general physicsParton showerEngineering (miscellaneous)PhysicsQuantum chromodynamics010308 nuclear & particles physicsElectroweak interactionHigh Energy Physics::PhenomenologyHigh Energy Physics - PhenomenologyHiggs bosonlcsh:QC770-798High Energy Physics::Experiment2201 Engineering (miscellaneous)
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Test of Colour Reconnection Models using Three-Jet Events in Hadronic Z Decays

2006

Hadronic Z decays into three jets are used to test QCD models of colour reconnection (CR). A sensitive quantity is the rate of gluon jets with a gap in the particle rapidity distribution and zero jet charge. Gluon jets are identified by either energy-ordering or by tagging two b-jets. The rates predicted by two string-based tunable CR models, one implemented in JETSET (the GAL model), the other in ARIADNE, are too high and disfavoured by the data, whereas the rates from the corresponding non-CR standard versions of these generators are too low. The data can be described by the GAL model assuming a small value for the R_0 parameter in the range 0.01-0.02.

Particle physicsPhysics and Astronomy (miscellaneous)Electron–positron annihilationAstrophysics::High Energy Astrophysical PhenomenaANNIHILATIONSW-BOSONFOS: Physical sciencesElementary particleJet (particle physics)MASS01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Particle decaySEARCH0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Rapidity010306 general physicsParton showerEngineering (miscellaneous)PhysicsQuantum chromodynamics010308 nuclear & particles physicsLEPQCDGLUON JETSGluonQUARK JETSHigh Energy Physics::ExperimentFRAGMENTATIONParticle Physics - ExperimentGENERATION
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Tuning and test of fragmentation models based on identified particles and precision event shape data

1996

Event shape and charged particle inclusive distributions are measured using 750000 decays of the $Z$ to hadrons from the DELPHI detector at LEP. These precise data allow a decisive confrontation with models of the hadronization process. Improved tunings of the JETSET ARIADNE and HERWIG parton shower models and the JETSET matrix element model are obtained by fitting the models to these DELPHI data as well as to identified particle distributions from all LEP experiments. The description of the data distributions by the models is critically reviewed with special importance attributed to identified particles.

Particle physicsPhysics and Astronomy (miscellaneous)Electron–positron annihilationHadron01 natural sciencesPartícules (Física nuclear)CROSS-SECTIONSNuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]BARYON PRODUCTIONMatrix element010306 general physicsParton showerPRODUCTION-RATESDELPHIELECTRON-POSITRON ANNIHILATIONQuantum chromodynamicsPhysicsQUANTUM CHROMODYNAMICS010308 nuclear & particles physicsDetectorHigh Energy Physics::PhenomenologyE+E-ANNIHILATIONLARGE ELECTRON POSITRON COLLIDERCharged particleFREE PERTURBATION-THEORYHadronizationELECTRON-POSITRON ANNIHILATION; FREE PERTURBATION-THEORY; HADRONIC Z(0) DECAYS; E+E-ANNIHILATION; QUANTUM CHROMODYNAMICS; ENERGY CORRELATIONS; BARYON PRODUCTION; PRODUCTION-RATES; CROSS-SECTIONS; NEUTRAL KAONSHADRONIC Z(0) DECAYSENERGY CORRELATIONSPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSFísica nuclearHigh Energy Physics::ExperimentNEUTRAL KAONSParticle Physics - Experiment
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