Large-scale anisotropies of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory

Measurements of anisotropies in the arrival directions of ultra-high-energy cosmic rays are crucial to pinpoint their sources, which are yet to be discovered. A dipolar anisotropy in right ascension above 8 EeV has been detected by the Pierre Auger Observatory with a significance of 6.8σ. The direct...

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Main Author: Bianciotto Marta
Format: Article
Language:English
Published: EDP Sciences 2025-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2025/04/epjconf_ricap2024_07001.pdf
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author Bianciotto Marta
author_facet Bianciotto Marta
author_sort Bianciotto Marta
collection DOAJ
description Measurements of anisotropies in the arrival directions of ultra-high-energy cosmic rays are crucial to pinpoint their sources, which are yet to be discovered. A dipolar anisotropy in right ascension above 8 EeV has been detected by the Pierre Auger Observatory with a significance of 6.8σ. The direction of the dipole suggests an extragalactic origin of ultra-high-energy cosmic rays above those energies. In this contribution, we provide an overview of the studies on large-scale anisotropies in the arrival directions of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory with energy thresholds from ∼ 0.03 EeV up to 32 EeV and we present and discuss the recent results achieved with the latest available dataset, which includes 19 years of operations – resulting in a total exposure of 123,000 km2 sr yr and nearly 50,000 events above 8 EeV.
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spelling doaj-art-da1ec6a8d4e949d3be8dbb09512637a22025-08-20T01:51:57ZengEDP SciencesEPJ Web of Conferences2100-014X2025-01-013190700110.1051/epjconf/202531907001epjconf_ricap2024_07001Large-scale anisotropies of ultra-high-energy cosmic rays measured at the Pierre Auger ObservatoryBianciotto Marta0Università degli studi di Torino & INFN, Sezione di TorinoMeasurements of anisotropies in the arrival directions of ultra-high-energy cosmic rays are crucial to pinpoint their sources, which are yet to be discovered. A dipolar anisotropy in right ascension above 8 EeV has been detected by the Pierre Auger Observatory with a significance of 6.8σ. The direction of the dipole suggests an extragalactic origin of ultra-high-energy cosmic rays above those energies. In this contribution, we provide an overview of the studies on large-scale anisotropies in the arrival directions of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory with energy thresholds from ∼ 0.03 EeV up to 32 EeV and we present and discuss the recent results achieved with the latest available dataset, which includes 19 years of operations – resulting in a total exposure of 123,000 km2 sr yr and nearly 50,000 events above 8 EeV.https://www.epj-conferences.org/articles/epjconf/pdf/2025/04/epjconf_ricap2024_07001.pdf
spellingShingle Bianciotto Marta
Large-scale anisotropies of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory
EPJ Web of Conferences
title Large-scale anisotropies of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory
title_full Large-scale anisotropies of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory
title_fullStr Large-scale anisotropies of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory
title_full_unstemmed Large-scale anisotropies of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory
title_short Large-scale anisotropies of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory
title_sort large scale anisotropies of ultra high energy cosmic rays measured at the pierre auger observatory
url https://www.epj-conferences.org/articles/epjconf/pdf/2025/04/epjconf_ricap2024_07001.pdf
work_keys_str_mv AT bianciottomarta largescaleanisotropiesofultrahighenergycosmicraysmeasuredatthepierreaugerobservatory