Isotropy of Cosmic Rays beyond 10^{20} eV Favors Their Heavy Mass Composition.
Journal
Physical review letters
ISSN: 1079-7114
Titre abrégé: Phys Rev Lett
Pays: United States
ID NLM: 0401141
Informations de publication
Date de publication:
26 Jul 2024
26 Jul 2024
Historique:
received:
24
03
2023
revised:
15
04
2024
accepted:
21
05
2024
medline:
9
8
2024
pubmed:
9
8
2024
entrez:
9
8
2024
Statut:
ppublish
Résumé
We report an estimation of the injected mass composition of ultrahigh energy cosmic rays (UHECRs) at energies higher than 10 EeV. The composition is inferred from an energy-dependent sky distribution of UHECR events observed by the Telescope Array surface detector by comparing it to the Large Scale Structure of the local Universe. In the case of negligible extragalactic magnetic fields (EGMFs), the results are consistent with a relatively heavy injected composition at E∼10 EeV that becomes lighter up to E∼100 EeV, while the composition at E>100 EeV is very heavy. The latter is true even in the presence of highest experimentally allowed extragalactic magnetic fields, while the composition at lower energies can be light if a strong EGMF is present. The effect of the uncertainty in the galactic magnetic field on these results is subdominant.
Identifiants
pubmed: 39121414
doi: 10.1103/PhysRevLett.133.041001
doi:
Types de publication
Journal Article
Langues
eng
Sous-ensembles de citation
IM