Search results for "Particle detectors."

showing 10 items of 22 documents

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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The DAMPE silicon–tungsten tracker

2016

Abstract The DArk Matter Particle Explorer (DAMPE) is a spaceborne astroparticle physics experiment, launched on 17 December 2015. DAMPE will identify possible dark matter signatures by detecting electrons and photons in the 5 GeV–10 TeV energy range. It will also measure the flux of nuclei up to 100 TeV, for the study of the high energy cosmic ray origin and propagation mechanisms. DAMPE is composed of four sub-detectors: a plastic strip scintillator, a silicon–tungsten tracker–converter (STK), a BGO imaging calorimeter and a neutron detector. The STK is composed of six tracking planes of 2 orthogonal layers of single-sided micro-strip detectors, for a total detector surface of ca. 7 m2. T…

Nuclear and High Energy PhysicsCosmic rays; Dark matter; Silicon tracker; Spaceborne experiment; Nuclear and High Energy Physics; InstrumentationPhysics::Instrumentation and DetectorsCosmic rayParticle detectorsTracking (particle physics)01 natural sciencesParticle detectorOpticscosmic rays0103 physical sciencesDark matterNeutron detection010303 astronomy & astrophysicsInstrumentationAstroparticle physicsPhysicsLarge Hadron ColliderCalorimeter (particle physics)010308 nuclear & particles physicsbusiness.industryDetectorSettore FIS/01 - Fisica SperimentaleParticle detectors cosmic raysSpaceborne experimentSilicon trackerHigh Energy Physics::Experimentbusiness
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Silicon detectors for the sLHC

2011

In current particle physics experiments, silicon strip detectors are widely used as part of the inner tracking layers. A foreseeable large-scale application for such detectors consists of the luminosity upgrade of the Large Hadron Collider (LHC), the super-LHC or sLHC, where silicon detectors with extreme radiation hardness are required. The mission statement of the CERN RD50 Collaboration is the development of radiation-hard semiconductor devices for very high luminosity colliders. As a consequence, the aim of the RandD programme presented in this article is to develop silicon particle detectors able to operate at sLHC conditions. Research has progressed in different areas, such as defect …

Nuclear and High Energy PhysicsSiliconPhysics::Instrumentation and DetectorsLHC; High luminosity collider; radiation damageCharge collection efficiencychemistry.chemical_elementHigh luminosity colliderTracking (particle physics)Nuclear physicsRadiation damageSilicon particle detectors; Radiation damage; Irradiation; Charge collection efficiencyInstrumentationRadiation hardeningPhysicsLuminosity (scattering theory)Large Hadron ColliderDetectorSemiconductor deviceEngineering physicsSilicon particle detectorschemistryHigh Energy Physics::ExperimentIrradiationLHCParticle physics experiments
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Radiation-hard semiconductor detectors for SuperLHC

2005

An option of increasing the luminosity of the Large Hadron Collider (LHC) at CERN to 10^35 cm^(- 2) s(- 1) has been envisaged to extend the physics reach of the machine. An efficient tracking down to a few centimetres from the interaction point will be required to exploit the physics potential of the upgraded LHC. As a consequence, the semiconductor detectors close to the interaction region will receive severe doses of fast hadron irradiation and the inner tracker detectors will need to survive fast hadron fluences of up to above 1016 cm 2. The CERN-RD50 project ''Development of Radiation Hard Semiconductor Devices for Very High Luminosity Colliders'' has been established in 2002 to explore…

Nuclear and High Energy Physicsradiation hard semiconductorsPhysics::Instrumentation and DetectorsSemiconductor detectorsRadiation Detector; LHCradiation hardness01 natural sciencesDefect engineeringSuper-LHCRadiation damageradiation detectorssilicon detectors0103 physical sciencesRadiation damageSuperLHCSilicon detectors; LHC; RD50 collaboration; radiation hardnessInstrumentationRadiation hardeningRadiation hardness010302 applied physicsPhysicsRadiation damage; Semiconductor detectors; Silicon particle detectors; Defect engineering; SLHC; Super-LHCLuminosity (scattering theory)Large Hadron ColliderRadiation DetectorInteraction pointRD50 collaboration010308 nuclear & particles physicsbusiness.industrySLHCDetectorRadiation hardness; silicon detectorsSemiconductor deviceSemiconductor detectorSilicon particle detectorsOptoelectronicsSilicon detectorsHigh Energy Physics::ExperimentLHCbusiness
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Expansion cone for the 3-inch PMTs of the KM3NeT optical modules

2013

[EN] Detection of high-energy neutrinos from distant astrophysical sources will open a new window on the Universe. The detection principle exploits the measurement of Cherenkov light emitted by charged particles resulting from neutrino interactions in the matter containing the telescope. A novel multi-PMT digital optical module (DOM) was developed to contain 31 3-inch photomultiplier tubes (PMTs). In order to maximize the detector sensitivity, each PMT will be surrounded by an expansion cone which collects photons that would otherwise miss the photocathode. Results for various angles of incidence with respect to the PMT surface indicate an increase in collection efficiency by 30% on average…

Optical detector readout concepts; Instrument optimisation; Cherenkov detectorsPhotomultiplier[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]Instrument optimisationCherenkov detectorPhysics::Instrumentation and Detectors01 natural scienceslarge detector systems for particle and astroparticle physics; optical detector readout concepts; cherenkov detectors; instrument optimization.Photocathodelaw.inventionTelescopeOpticslaw0103 physical sciencesOptical detector readout conceptsNEUTRINO TELESCOPE010306 general physicsInstrumentationMathematical PhysicsCherenkov radiationPhysics010308 nuclear & particles physicsbusiness.industryLarge detector systems for particle and astroparticle physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]DetectorCherenkov detectorsAstrophysics::Instrumentation and Methods for AstrophysicsInstrument optimizationINGENIERIA TELEMATICAOptical detector readout concept[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]KM3NeTLarge detector systems for particle and astroparticle physicNeutrinobusinessPROJECTCherenkov detector85.60.Ha Photomultipliers ; phototubes and photocathodes ; 42.15.Dp Wave fronts and ray tracing ; 98.80.-k Cosmology ; 95.55.Vj Neutrino muon pion and other elementary particle detectors; cosmic ray detectors ; 29.40.Ka Cherenkov detectors
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Measurement of the Inclusive Electron Neutrino Charged Current Cross Section on Carbon with the T2K Near Detector

2014

The T2K off-axis near detector, ND280, is used to make the first differential cross-section measurements of electron neutrino charged current interactions at energies ~1 GeV as a function of electron momentum, electron scattering angle and four-momentum transfer of the interaction. The total flux-averaged $\nu_e$ charged current cross-section on carbon is measured to be $1.11\pm0.09~(stat)\pm0.18~(syst)\times10^{-38} cm^2/nucleon$. The differential and total cross-section measurements agree with the predictions of two leading neutrino interaction generators, NEUT and GENIE. The NEUT prediction is $1.23\times10^{-38} cm^2/nucleon$ and the GENIE prediction is $1.08\times10^{-38} cm^2/nucleon$…

Particle physicsPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesParticle detectorsElectronCarbon Electron scattering Electrons Neutrons Testbed7. Clean energyHigh Energy Physics - ExperimentNuclear physicsCross section (physics)Physics and Astronomy (all)High Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentCharged currentPhysicsCharged current Differential cross section Electron momentum Electron neutrino Neutrino interactions Off-axis Total cross section Total fluxFísicaGargamelleHigh Energy Physics::ExperimentNeutrinoNucleonElectron neutrinoElectron scatteringPhysical Review Letters
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MALTA: a CMOS pixel sensor with asynchronous readout for the ATLAS High-Luminosity upgrade

2018

Radiation hard silicon sensors are required for the upgrade of the ATLAS tracking detector for the High- Luminosity Large Hadron Collider (HL-LHC) at CERN. A process modification in a standard 0.18 μm CMOS imaging technology combines small, low-capacitance electrodes (∼2 fF for the sensor) with a fully depleted active sensor volume. This results in a radiation hardness promising to meet the requirements of the ATLAS ITk outer pixel layers (1.5 × 1015 neq /cm2 ), and allows to achieve a high signal-to-noise ratio and fast signal response, as required by the HL-LHC 25 ns bunch crossing structure. The radiation hardness of the charge collection to Non-Ionizing Energy Loss (NIEL) has been previ…

PhysicsActive pixel sensors ; CMOS integrated circuits ; position sensitive particle detectors ; radiation effects ; radiation hardening (electronics) ; semiconductor detectors ; solid state circuit designPixelPhysics::Instrumentation and Detectors010308 nuclear & particles physicsbusiness.industryDetectorHigh Luminosity Large Hadron Collider01 natural sciencesCapacitance030218 nuclear medicine & medical imagingSemiconductor detector03 medical and health sciences0302 clinical medicineCMOSNuclear electronics0103 physical sciencesbusinessRadiation hardeningComputer hardware
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ALEPH: a Detector for Electron-Positron Annihilations at LEP

1990

Process-centred Software Engineering Environments (PSEE) are the most recent generation of environments supporting software development activities. Most of PSEE are based on mechanisms promoting enforcement and automation of process activities. In this kind of mechanisms the process models are prescribed in a detailed and complete way. But the experience shows that supporting processes is more concerned with the flexibility of guidance offered during the process performance than with enforcement of a collection of predefined process models. In this paper, we present a solution to support strategic processes in a PSEE by providing a flexible guidance during process enactment.

PhysicsFlexibility (engineering)Nuclear and High Energy PhysicsAlephhigh-energy physicsProcess modelingProcess (engineering)business.industrySoftware developmentLEPAutomationparticle detectorsData acquisitionDetectors and Experimental TechniquesLEP; particle detectors; high-energy physicsSoftware engineeringbusinessEnforcementInstrumentationparticle detector
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Coexisting structures in 115Sn and 116Sn

1998

Abstract Excited states up to I ≈ 20 in 115 Sn and 116 Sn, populated via the ( 18 O, αxn) reactions, have been studied using the DORIS Ge detector array in conjunction with charged particle detectors. In both nuclei, spherical as well as regular, deformed level structures were found. The spherical states are interpreted to arise from pure neutron configurations, while the deformed, intruder bands obviously involve proton 2p-2h excitations across the Z = 50 shell gap.

PhysicsNuclear and High Energy PhysicsCharged particle detectorsProtonConjunction (astronomy)Excited stateShell (structure)NeutronDetector arrayAtomic physicsNuclear Physics A
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Search for ultrahigh energy neutrinos in highly inclined events at the Pierre Auger Observatory

2011

Erratum: Phys. Rev. D 85, 029902(E) (2012) [http://dx.doi.org/10.1103/PhysRevD.85.029902]

Physics::Instrumentation and DetectorsSolar neutrinoAstrophysicsUPPER LIMITPHOTON FRACTION01 natural sciences7. Clean energyneutrinoObservatoryHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsORIGINPhysics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]pionAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryCOSMIC-RAYScosmic ray detectorsand other elementary particle detectorsCosmic neutrino backgroundNEUTRINOSFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaFLUXFERMI-LATNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]TELESCOPEAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayEXTENSIVE AIR-SHOWERSSURFACE DETECTORCosmic RayPionmuon0103 physical sciencesNeutrino010306 general physicsCosmic raysPierre Auger ObservatoryMuon010308 nuclear & particles physicsFísicaand other elementary particlesUltra-high energy cosmic raysPERFORMANCECosmic rayneutrino flavor; air showers; surface detector; observatory; atmosphere; Auger; cosmic radiation; energy spectrum13. Climate actionHigh Energy Physics::Experiment
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