A Collaborative Explanation of Cosmic Ray Spectrum Based on the Gluon Condensation Model

TL;DR

This paper uses the Gluon Condensation model to explain the relationship between cosmic ray electrons, gamma rays, and neutrinos, suggesting a common origin and linking gamma-ray observations to electron excesses.

Contribution

It introduces a unified explanation for cosmic ray particle spectra based on the Gluon Condensation model, connecting multiple particle types and observational data.

Findings

Particles share the same GC threshold and parameter β_p

Gamma-ray data suggests LHAASO J2108+5157 source contributes to electron excess

The model links electron, gamma-ray, and neutrino spectra through GC

Abstract

Based on the Gluon Condensation (GC) model, the relationship between the spectra of electrons, $\gamma$ rays, and neutrinos in cosmic rays can be deduced. It has been found that these particles share the same parameter, $\beta_p$, and have an identical GC threshold values. This paper explores the connection between the second excess spectra of electron and the spectra of gamma rays and neutrinos. According to the observed gamma-ray data, it is suggested that the source LHAASO J2108+5157 might contribute to the second excess of electron.