Search results for "Ultra High Energy Cosmic ray"

showing 5 items of 25 documents

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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Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory

2017

We report a multi-resolution search for anisotropies in the arrival directions of cosmic rays detected at the Pierre Auger Observatory with local zenith angles up to $80^\circ$ and energies in excess of 4 EeV ($4 \times 10^{18}$ eV). This search is conducted by measuring the angular power spectrum and performing a needlet wavelet analysis in two independent energy ranges. Both analyses are complementary since the angular power spectrum achieves a better performance in identifying large-scale patterns while the needlet wavelet analysis, considering the parameters used in this work, presents a higher efficiency in detecting smaller-scale anisotropies, potentially providing directional informa…

moment: dipoleAstronomy[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic ray experiments; ultra high energy cosmic rays; Astronomy and AstrophysicsCosmic rayanisotropyultra high energy cosmic raysSURFACE DETECTOR01 natural sciencesLARGE-SCALE DISTRIBUTIONwaveletSEARCH0103 physical sciencesARRIVAL DIRECTIONSHigh Energy Physicscosmic radiation: UHEAnisotropy010303 astronomy & astrophysicsZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)Pierre Auger ObservatoryPhysicsSPECTRUM010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleSpectral densityAstronomy and AstrophysicsEEVASTROFÍSICAComputational physicsAugerCosmic ray experiments; ultra high energy cosmic raysobservatoryDipolecosmic ray experiments ultra high energy cosmic raysRESOLUTIONMoment (physics)Experimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGpower spectrum: angular dependenceARRAYcosmic ray experimentsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Measurement of the average shape of longitudinal profiles of cosmic-ray air showers at the Pierre Auger Observatory

2019

The profile of the longitudinal development of showers produced by ultra-high energy cosmic rays carries information related to the interaction properties of the primary particles with atmospheric nuclei. In this work, we present the first measurement of the average shower profile in traversed atmospheric depth at the Pierre Auger Observatory. The shapes of profiles are well reproduced by the Gaisser-Hillas parametrization within the range studied, for E>10 17.8 eV .A detailed analysis of the systematic uncertainties is performed using ten years of data and a full detector simulation. The average shape is quantified using two variables related to the width and asymmetry of the profile, and …

p: showersphoton: Cherenkovinteraction: modelAstronomyHadronpiastro-ph.HE; astro-ph.HE01 natural sciencesnitrogenironParametrization (atmospheric modeling)Monte Carlomedia_commonPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Range (particle radiation)photomultiplierSettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for AstrophysicsDETETOREScosmic rays detectors; ultra high energy cosmic rays; Astronomy and AstrophysicsAugerobservatorycosmic rays detectorscosmic rays detectors; ultra high energy cosmic raysgeometricalAstrophysics - High Energy Astrophysical PhenomenaasymmetrylongitudinalCherenkov counter: waterairmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayheliumultra high energy cosmic raysnucleus: atmosphereAsymmetry0103 physical sciencesHigh Energy Physicscosmic radiation: UHEcosmic rays detectorFLUORESCENCEAstrophysiquePierre Auger Observatoryelectron positronshowers: atmosphere010308 nuclear & particles physicsbackgrounddetector: surfaceshowers: spatial distributionparametrizationAstronomy and AstrophysicsAstronomieComputational physics13. Climate actiongamma rayExperimental High Energy Physics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)Journal of Cosmology and Astroparticle Physics
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Search for photons with energies above 1018 eV using the hybrid detector of the Pierre Auger Observatory

2017

A search for ultra-high energy photons with energies above 1 EeV is performed using nine years of data collected by the Pierre Auger Observatory in hybrid operation mode. An unprecedented separation power between photon and hadron primaries is achieved by combining measurements of the longitudinal air-shower development with the particle content at ground measured by the fluorescence and surface detectors, respectively. Only three photon candidates at energies 1-2 EeV are found, which is compatible with the expected hadron-induced background. Upper limits on the integral flux of ultra-high energy photons of 0.027, 0.009, 0.008, 0.008 and 0.007 km-2 sr-1 yr-1 are derived at 95% C.L. for ener…

ultra high energy cosmic rays cosmic ray experimentsPhoton[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyHadronFluxultra high energy cosmic rays; cosmic ray experiments7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)energy: thresholdCosmic ray experiments[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsphoton: productionconstraint: energyCOSMIC-RAYSAugerobservatoryContent (measure theory)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearfluorescenceAstrophysics - High Energy Astrophysical PhenomenalongitudinalAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic rayultra high energy cosmic raysdark matterUltra high energy cosmic rays Cosmic ray experiments Astronomy and Astrophysics.Nuclear physics[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]0103 physical sciencesultra high energy cosmic rays; cosmic ray experiments; Astronomy and Astrophysicscosmic radiation: UHEHigh Energy PhysicsCiencias ExactasPierre Auger ObservatorySPECTRUMhybridbackgrounddetector: surface010308 nuclear & particles physicsFísicaUltra high energy cosmic raysAstronomy and AstrophysicsASTROFÍSICAULTRA-HIGH ENERGYfluxExperimental High Energy PhysicsHigh Energy Physics::Experimentcosmic ray experimentshadron[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Energy (signal processing)
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Ultra-High Energy Neutrinos at the Pierre Auger Observatory

2013

The observation of ultrahigh energy neutrinos (UHE nu s) has become a priority in experimental astroparticle physics. UHE nu s can be detected with a variety of techniques. In particular, neutrinos can interact in the atmosphere (downward-going nu) or in the Earth crust (Earth-skimming nu), producing air showers that can be observed with arrays of detectors at the ground. With the surface detector array of the Pierre Auger Observatory we can detect these types of cascades. The distinguishing signature for neutrino events is the presence of very inclined showers produced close to the ground (i.e., after having traversed a large amount of atmosphere). In this work we review the procedure and …

ultra high energy neutrino[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Physics::Instrumentation and DetectorsCiencias FísicasAstronomyFluxAstrophysics7. Clean energy01 natural sciencesAltas energíasAuger//purl.org/becyt/ford/1 [https]surface [detector]ObservatoryneutriniCosmic-rayscosmic rayHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCascada atmosférica extensaOBSERVATÓRIOS[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsSettore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsneutrino; Augerlcsh:QC1-999AugercascadeUHE [neutrino]observatoryPhysics::Space PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearultra high energy neutrinosNeutrinoAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASsignatureTAU-NEUTRINOSatmosphere [showers]FLUXNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Article SubjectairAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayFísica de Partículas y CamposLIMITPartícules (Física nuclear)Ultra high energy cosmic rayAtmosphere[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Air-showersSEARCHNeutrino0103 physical sciencesddc:530010306 general physicsAstrophysiqueCiencias ExactasPierre Auger ObservatoryAstroparticle physicsSPECTRUM010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaUltra high energy cosmic raystelescopes//purl.org/becyt/ford/1.3 [https]Ultrahigh Energyflux13. Climate actionenergy [neutrino]Pierre AugerExperimental High Energy PhysicsARRAYHigh Energy Physics::ExperimentAstroparticle physicslcsh:Physics
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