Mass composition of ultra-high-energy cosmic rays at the Pierre Auger Observatory
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F25%3A00640394" target="_blank" >RIV/68378271:_____/25:00640394 - isvavai.cz</a>
Alternative codes found
RIV/61989592:15310/25:73634779
Result on the web
<a href="https://pos.sissa.it/484/041/pdf" target="_blank" >https://pos.sissa.it/484/041/pdf</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.484.0041" target="_blank" >10.22323/1.484.0041</a>
Alternative languages
Result language
angličtina
Original language name
Mass composition of ultra-high-energy cosmic rays at the Pierre Auger Observatory
Original language description
For the past 20 years, the Pierre Auger Observatory has collected the largest dataset of ultra-high- energy cosmic rays (UHECRs) ever achieved using a hybrid detector. The study of this dataset has led to numerous unexpected discoveries that enhance our understanding of the origins of UHECRs. One of the key points in this study is their mass composition. In this work, we will present the most recent results regarding the mass composition of UHECRs at the Pierre Auger Observatory. In particular, we will focus on the measurement of the depth of the maximum of air-shower profiles, denoted as Xmax . This determination has been achieved through both direct measurements from the Fluorescence Detector data and the application of machine learning for estimating Xmax on an event-by-event basis using the Surface Detector data. The latter has allowed us to extend the measurement to energies up to 100 EeV and indicates a correlation between changes in composition and three features of the energy spectrum (ankle, instep, steepening). Moreover, the results provide evidence of a heavy and nearly pure primary beam for energies greater than 50 EeV that is independent of the hadronic interaction model. The implications of these findings for astrophysics and for modelling hadronic interactions will be discussed.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10303 - Particles and field physics
Result continuities
Project
Result was created during the realization of more than one project. More information in the Projects tab.
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2025
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Proceedings of Science
ISBN
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ISSN
1824-8039
e-ISSN
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Number of pages
8
Pages from-to
041
Publisher name
Sissa Medilab srl
Place of publication
Trieste
Event location
Malargüe
Event date
Nov 17, 2024
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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