A possible evidence of the gluon condensation effect in cosmic positron and gamma-ray spectra

Abstract

The gluon condensation effect in cosmic proton-proton collisions at high energy is used to explain an excess in the positron spectrum observed by AMS. We find that this excess may originate from the GC-effect in Tycho's supernova remnant.

4 pages, 4 figures, Accepted for publication in the ApJ

References in corpus (3)

• Cosmic ray production in supernovae
• The gluon condensation at high energy hadron collisions
• Can a chaotic solution in the QCD evolution equation restrain high-energy collider physics?

Cited by in corpus (7)

• The gluon condensation in hadron collisions
• Looking for the possible gluon condensation signature in sub-TeV gamma-ray spectra: from active galactic nuclei to gamma ray bursts
• Exploring the possible gluon condensation signature in gamma-ray emission from pulsars
• Gluon Condensation Signature in the GeV Gamma-Ray Spectra of Pulsars
• Warning: The mini gamma-ray-bursts in planning hadron colliders beyond the LHC energies
• The current recorded signals of ultrahigh-energy $\gamma$-rays may come from EeVatrons in the galaxy
• The gluon condensation effect in the cosmic hadron spectra