Recent developments in cosmic ray physics
P. Blasi ((1) INAF/Arcetri, (2) INFN/GSSI)

TL;DR
This paper reviews recent developments and debates in cosmic ray physics, focusing on the origin, acceleration limits, and composition transition, highlighting conflicting experimental evidence and their implications for cosmic ray models.
Contribution
It provides a critical overview of current theories and experimental findings, clarifying what is well-established and what remains uncertain in cosmic ray origin research.
Findings
Recent data challenge the traditional knee interpretation.
Light component flux reduction observed at ~700 TeV.
Implications for supernova remnant models and Galactic-extragalactic transition.
Abstract
The search for a theory of the origin of cosmic rays that may be considered as a standard, agreeable model is still ongoing. On one hand, much circumstantial evidence exists of the fact that supernovae in our Galaxy play a crucial role in producing the bulk of cosmic rays observed on Earth. On the other hand, important questions about their ability to accelerate particles up to the knee remain unanswered. The common interpretation of the knee as a feature coinciding with the maximum energy of the light component of cosmic rays and a transition to a gradually heavier mass composition is mainly based on KASCADE results. Some recent data appear to question this finding: YAC1 - Tibet Array and ARGO-YBJ find a flux reduction in the light component at TeV, appreciably below the knee. Whether the maximum energy of light nuclei is as high as TeV or rather as low as a few…
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