Abstract
The gluon condensation (GC) effect in cosmic proton-proton collisions at high energy is used to explain an excess in the positron spectrum observed by the Alpha Magnetic Spectrometer. We find that this excess may originate from the GC effect in Tycho's supernova remnant.
| Original language | English |
|---|---|
| Article number | 127 |
| Journal | Astrophysical Journal |
| Volume | 889 |
| Issue number | 2 |
| DOIs | |
| State | Published - 1 Feb 2020 |