English

Indirect evidence of GeV Dark Matter

High Energy Astrophysical Phenomena 2015-06-23 v1

Abstract

Recently, an excess of GeV gamma ray near the Galactic Centre has beenvreported. The spectrum obtained can be best fitted with the annihilationvof 304030-40 GeV dark matter particles through bbˉb \bar{b} channel. In this letter, I show that this annihilation model can also solve the mysteries of heating source in x-ray plasma and the unexpected high gamma-ray luminosity. The cross section constrained by these observations give excellent agreements with both the predicted range by using Fermi-LAT data and the canonical thermal relic abundance cross section.

Keywords

Cite

@article{arxiv.1501.02043,
  title  = {Indirect evidence of GeV Dark Matter},
  author = {Man Ho Chan},
  journal= {arXiv preprint arXiv:1501.02043},
  year   = {2015}
}

Comments

Accepted by MNRAS Letters