Search results for " ultra-high energy cosmic rays"

showing 2 items of 2 documents

Measurement of the cosmic ray energy spectrum using hybrid events of the Pierre Auger Observatory

2012

The energy spectrum of ultra-high energy cosmic rays above 10$^{18}$ eV is measured using the hybrid events collected by the Pierre Auger Observatory between November 2005 and September 2010. The large exposure of the Observatory allows the measurement of the main features of the energy spectrum with high statistics. Full Monte Carlo simulations of the extensive air showers (based on the CORSIKA code) and of the hybrid detector response are adopted here as an independent cross check of the standard analysis (Phys. Lett. B 685, 239 (2010)). The dependence on mass composition and other systematic uncertainties are discussed in detail and, in the full Monte Carlo approach, a region of confiden…

FLUORESCENCE DETECTORAstronomyAstrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodenergy spectrumFOS: Physical sciencesGeneral Physics and AstronomyFluxCosmic rayEXTENSIVE AIR-SHOWERSSURFACE DETECTOR01 natural sciencesCosmic RayAugerPierre Auger Observatory ; Monte Carlo simulations ; ultra-high energy cosmic raysHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Observatory0103 physical sciencesRECONSTRUCTIONFermilab010306 general physicsUHE Cosmic Rays Monte Carlo Energy SpectrumTRIGGERNuclear PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryPACS: 96.50.S 96.50.sb 96.50.sd 98.70.Sa010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Pierre Auger Observatory; Monte Carlo simulations; ultra-high energy cosmic raysPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryPROFILES[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph]Experimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGARRAYFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaRAIOS CÓSMICOS
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Direct measurement of the muonic content of extensive air showers between 2× 1017 and 2×1018 eV at the Pierre Auger Observatory

2020

The hybrid design of the Pierre Auger Observatory allows for the measurement of the properties of extensive air showers initiated by ultra-high energy cosmic rays with unprecedented precision. By using an array of prototype underground muon detectors, we have performed the first direct measurement, by the Auger Collaboration, of the muon content of air showers between 2 × 10 17 and 2 × 10 18 eV. We have studied the energy evolution of the attenuation-corrected muon density, and compared it to predictions from air shower simulations. The observed densities are found to be larger than those predicted by models. We quantify this discrepancy by combining the measurements from the muon detector …

Muon detector ultra-high energy cosmic raysmuonsUHE Cosmic Rays
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