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Features of the energy spectrum of cosmic rays above 2.5×1018 eV using the pierre auger observatory

  • (The Pierre Auger Collaboration)
  • Radboud University Nijmegen
  • Instituto Superior Tecnico
  • INAF-IAPS
  • Sezione di Torino
  • University of Adelaide
  • CNEA-UNCuyo-CONICET
  • Instituto de Tecnologías en Detección y Astropartículas (CNEA CONICET UNSAM)
  • Universidad Tecnológica Nacional
  • Universidad Nacional Autonoma de Mexico
  • Universidad de Santiago de Compostela
  • Università di Torino and Sezione INFN
  • Lehman College
  • Sezione di Napoli
  • RWTH Aachen University
  • Observatorio Pierre Auger and Comisión Nacional de Energía Atómica
  • University Politehnica of Bucharest
  • Institute of Physics of the Czech Academy of Sciences
  • 'Horia Hulubei' National Institute for Physics and Nuclear Engineering
  • Università di Napoli 'Federico II' and Sezione INFN
  • Bergische Universität Wuppertal
  • UJF-Grenoble 1/CNRS-INSU
  • Max-Planck-Institut für Radioastronomie
  • Université Paris 11
  • Dipartimento di Scienze Fisiche e Chimiche
  • Laboratori Nazionali del Gran Sasso
  • Universidade Federal do Rio de Janeiro
  • University of São Paulo
  • Institute of Nuclear Physics PAN
  • Colorado State University
  • Universität Siegen
  • Universidad de Granada
  • Vrije Universiteit Brussel
  • Università di Catania and Sezione INFN
  • Sezione di Catania
  • Universidad Autónoma de Chiapas
  • Università degli Studi di Milano
  • Sezione di Milano

Research output: Contribution to journalArticlepeer-review

173 Scopus citations

Abstract

We report a measurement of the energy spectrum of cosmic rays above 2.5×1018 eV based on 215 030 events. New results are presented: at about 1.3×1019 eV, the spectral index changes from 2.51±0.03(stat)±0.05(syst) to 3.05±0.05(stat)±0.10(syst), evolving to 5.1±0.3(stat)±0.1(syst) beyond 5×1019 eV, while no significant dependence of spectral features on the declination is seen in the accessible range. These features of the spectrum can be reproduced in models with energy-dependent mass composition. The energy density in cosmic rays above 5×1018 eV is [5.66±0.03(stat)±1.40(syst)]×1053 erg Mpc-3.

Original languageBritish English
Article number121106
JournalPhysical Review Letters
Volume125
Issue number12
DOIs
StatePublished - Sep 2020

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