  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.
