Cosmic-ray Spectrum and Composition with the IceCube Observatory
Alessio Tamburro (for the IceCube Collaboration)

TL;DR
This paper presents recent measurements of the energy spectrum and nuclear composition of galactic cosmic rays using the IceCube Observatory, covering energies from 300 TeV to 1 EeV.
Contribution
It provides new observational data on cosmic-ray spectrum and composition in a high-energy range using IceCube, enhancing understanding of cosmic-ray origins.
Findings
Detailed cosmic-ray energy spectrum between 300 TeV and 1 EeV.
Insights into the nuclear composition of galactic cosmic rays.
Improved constraints on cosmic-ray source models.
Abstract
This paper reports on recent results from measurements of energy spectrum and nuclear composition of galactic cosmic rays performed with the IceCube Observatory at the South Pole in the energy range between about 300 TeV and 1 EeV.
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