UHECR2024
17-21 November 2024
Malargüe, Mendoza, Argentina
Malargüe, Mendoza, Argentina
The 7th International Symposium on Ultra-High-Energy Cosmic Rays (UHECR 2024), held from November 17 to 21, 2024, in Malargüe, Argentina, was a new edition of a series of meetings that bring together the UHECR community and that were previously held in Nagoya (2010), CERN (2012), Springdale, Utah (2014), Kyoto (2016), Paris (2018), and L'Aquila (2022).
The latest results from UHECR observations, theoretical developments, and future plans in the field were discussed. The symposium focused on the highest energy cosmic rays, as well as on cosmic rays with energies above 1 PeV. The agenda included invited reviews, contributed talks, and reports from inter-collaborative working groups, all in plenary sessions. Poster contributions were also presented. Both oral and poster presentations are included in the proceedings.
| Sessions |
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| session Monday |
| session Tuesday |
| session Wednesday |
| Session Thursday |
| session Posters |
| session Monday |
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Source Models of UHECRs
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Magnetic field effects on UHECR propagation
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The Galactic Magnetic Field and UHECR Deflections
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The flux of UHECRs along the supergalactic plane using Pierre Auger Observatory data
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Large-scale cosmic-ray anisotropies measured at the Pierre Auger Observatory
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Update on full-sky searches for large- and medium-scale anisotropies in the UHECR flux using the Pierre Auger Observatory and the Telescope Array
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Are Star-forming and Starburst Galaxies actually Cosmic-rays calorimeters? Insights from 15 years of Fermi-LAT Data and implications for UHECRs
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Astrophysical models to interpret the Pierre Auger Observatory data
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Approaching UHECR astronomy using mass-sensitive data from the Pierre Auger Observatory and the Telescope Array Project
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| session Tuesday |
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The Pierre Auger Observatory and Physics Beyond the Standard Model
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Searches for ultra-high-energy photons with the Pierre Auger Observatory
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Searches for UHE neutrinos and upward-going showers at the Pierre Auger Observatory
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Development of an analysis method for neutrino-induced air showers with the Telescope Array surface detectors
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A new view of UHECRs with the Pierre Auger Observatory
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Multi-Messenger Insights into Ultra-High-Energy Cosmic Rays from FR0 Radio Galaxies: Emission Spectrum, Composition, and Secondary Photons and Neutrinos
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Various constraints on BSM physics from extensive air showers and from UHE gamma-ray and neutrino searches
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| session Wednesday |
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Hadronic interaction at LHC: review for the LHCf and air shower related measurements
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Overview of hadronic interaction studies at the Pierre Auger Observatory
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Muons in air showers with IceCube: muon density at ground and high-energy muon multiplicity
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Measuring the Proton-Proton Interaction Cross-Section with Hybrid Data of the Pierre Auger Observatory
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Energy Spectrum Measured by the Telescope Array Surface Detectors
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Testing the declination dependency of the spectrum measured by the Pierre Auger Observatory
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Measurement of cosmic-ray energy spectrum with the TALE detector in hybrid mode
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Evaluation of the Telescope Array surface detector's energy reconstruction performance using a deep neural network and hybrid data
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Mass composition of ultra-high-energy cosmic rays at the Pierre Auger Observatory
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Cosmic Ray Composition Measurement between 3 PeV to 30 PeV with the TALE Hybrid Detector
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CORSIKA 8: A modern and universal framework for particle cascade simulations
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Modified Hadronic Interactions and the future of UHECR observations
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| Session Thursday |
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The Venusian Chronicles
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Highlights from the Auger Engineering Radio Array
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Subluminal Pulses in the Surface-Scintillator Detectors of AugerPrime
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Latest updates and results from the Fluorescence detector Array of Single-pixel Telescopes (FAST)
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Progress in the development of the observation system for the CRAFFT project
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Science Potential and Technical Design of the IceCube-Gen2 Surface Array
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The Strawman Design of the Global Cosmic Ray Observatory
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GRAND: status and perspectives
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The Mini-EUSO telescope on board the International Space Station: mission results in view of UHECR measurements from space
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Overview of the JEM-EUSO Program
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POEMMA-Balloon with Radio, towards a space-based Multi-Messenger Observatory
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| session Posters |
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Rescaling of the muon content of simulated air showers in the context of the Muon Puzzle
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The connection between Cosmic-rays, Neutrinos and X-ray: the Case of Seyfert Galaxies
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Light Dark Matter vs Starburst Nuclei
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Towards the implementation of the photodisintegration interaction in SimProp Sirente
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Amplifying UHECR arrival direction information using mass estimators at the Pierre Auger Observatory
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Arrival directions of ultra-high-energy cosmic rays assuming heavy mass-composition
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Prospects for constraining transient sources of UHECRs with arrival-direction data
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Beyond the Local Void: A comprehensive view on the origins of the Amaterasu particle.
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Magnetic Monopoles: Theoretical Insights into the Cosmic Ray Conundrum
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$\nu$SpaceSim: An end-to-end simulation package to model the sensitivity of UHECR experiments to upward-moving extensive air showers sourced by cosmic neutrinos interacting in the Earth
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GRAND@Auger: status and first results
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Improved Calibration Methods and Reconstruction of the Underground Muon Detector of the Pierre Auger Observatory
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Data-driven method to quantify and correct the corner-clipping effect in segmented muon counters
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On gamma rays as predictors of UHECR flux in AGNs
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Impact of the Galactic magnetic field modelling on studies of the UHECRs arrival direction
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Investigations of CORSIKA Thinning Levels Suitable for Studies of Photon-Hadron Discrimination at Ultra-High Energies
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ANDESPix: A Digital SiPM for Muon Detectors
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Calibration of the Scintillator Surface Detector of AugerPrime
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Layered Water Cherenkov Detectors for Next Generation Air-Shower Arrays
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Global Spline Fit (GSF) 2024
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Communicating astroparticle physics with the public: the Pierre Auger Observatory experience
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CORSIKA 8 with Pythia 8/Angantyr: Simulating Inclined Proton Showers
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Machine learning-based analyses using surface detector data of the Pierre Auger Observatory
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Correlation studies on UHECR arrival direction and source candidates, with a convolution of magnetic field and mass composition
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The Radio Detector of the Pierre Auger Observatory
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Oscillations of hypothetical strange stars as an efficient source ultra-high-energy particles.
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Measurement of cosmic rays with energies down to the PeV region using the TALE-infill SD array
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Telescope Array Surface Detector Medium-scale Anisotropy Analyses
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The fractional analysis of mass composition measured by the Telescope Array FADC fluorescence detectors in hybrid mode
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Analysis of Inclined Air Shower Events Observed by the TAx4 SD
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Mapping distributions of production variables of UHECR-air interactions onto the ($N_\mu$, $X_{\max}$) space
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Prospects of a composition-enhanced search for large-scale anisotropy with the Pierre Auger Observatory
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Search for neutrons from Galactic sources with the Pierre Auger Observatory
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Impact of Lorentz Invariance Violation on the Propagation of Ultra-High-Energy Photons
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Active Galactic Nuclei Metallicity Enrichment and UHECR Composition
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Improved method of searching for flares of neutral particles from point sources
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Does the Local Bubble bias Galactic magnetic field models used to backtrack UHECRs?
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Estimation of Muons on the Surface and Correlation with the Muonic Signal of AugerPrime
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Stochastic description of UHECR interactions
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Neural Networks for Photon Searches with AugerPrime
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ALPACA project to observe sub-PeV gamma-ray sky in the southern hemisphere
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The core software and simulation activities for data analysis at the Pierre Auger Observatory
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The Pierre Auger Observatory Open Data
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Neural network identification of highly inclined muons in water-Cherenkov particle detectors
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Effect of the knock-on electrons in the calorimetric mode of an underground muon detector
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Reconstructing Air-Shower Observables using a Universality-Based Model
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Ultra-high-energy cosmic rays from accretion shocks in galaxy clusters
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Calibration of the TA Fluorescence Detectors and Systematic Uncertainties in UHECR Analysis
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Evaluating the purity of cosmic ray composition via depth of the shower maximum and muon density-based parameter correlation
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Plans for a new array of radio antennas for the detection of air showers at the 433m surface-detector array of the Pierre Auger Observatory
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Consequences of a Heavy-Metal Scenario for Ultra-High-Energy Cosmic Rays
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When the link to the pdf file is not available, the contribution in question has not yet been accepted for publication.