0000000000460163

AUTHOR

M. D. Rodriguez-frias

showing 2 related works from this author

Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory

2016

Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accelerators. Here we introduce a new method to test hadronic interaction models without relying on the absolute energy calibration, and apply it to events with primary energy 6-16 EeV (ECM=110-170 TeV), whose longitudinal development and lateral distribution were simultaneously measured by the Pierre Auger Observatory. The average hadronic shower is 1.33±0.16 (1.61±0.21) times larger than predicted using the leading LHC-tuned models EPOS-LHC (QGSJetII-04), with a corresponding excess of muons.

Hadronic interaction[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Particle physicsCOLLISIONSAstronomyAstrophysics::High Energy Astrophysical PhenomenaHadronFOS: Physical sciencesGeneral Physics and AstronomyCosmic ray01 natural sciences7. Clean energyHigh Energy Physics - ExperimentAugerHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)High Energy Physics - Phenomenology (hep-ph)Observatory0103 physical sciencesCalibrationHigh Energy PhysicsUHE Cosmic Rays010306 general physicsParticle PhysicsCosmic raysGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryEnergyMuon010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for AstrophysicsFísicaInteraction modelASTROFÍSICAHigh Energy Physics - Phenomenology13. Climate actionExperimental High Energy PhysicsHigh Energy Physics::ExperimentAstrophysics - High Energy Astrophysical Phenomena
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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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