Propagation and Source Energy Spectra of Cosmic-Ray Nuclei at High Energies

TL;DR

This paper investigates the propagation and energy spectra of cosmic-ray nuclei at high energies, aiming to understand their origins and behavior in space.

Contribution

It introduces new analysis methods for cosmic-ray spectra and provides insights into their propagation mechanisms at high energies.

Findings

Cosmic-ray nuclei exhibit specific spectral features at high energies

Propagation models align with observed energy spectra

Source energy spectra suggest particular acceleration processes

Abstract

This paper has not yet been accepted for publication