Abstract
The anomalies in positron fraction observed in PAMELA and total flux of electrons and positron reported by Fermi can be explained by a decaying dark matter. The agreement between astrophysical background and observed data in anti-proton indicates a lep-tophilic dark matter and constrains the hadronic decay branching ratios. In this work, we study the constrains on decaying rates of a dark matter to various 2-body final states using the Fermi and HESS gamma-ray data. We find that μ+μ- or τ+τ- final state is preferred to simultaneously explain the excesses and meet the gamma-ray constrains.
| Original language | English |
|---|---|
| Pages (from-to) | 969-975 |
| Number of pages | 7 |
| Journal | Modern Physics Letters A |
| Volume | 25 |
| Issue number | 11-12 |
| DOIs | |
| Publication status | Published - 2010 Apr 20 |
| Externally published | Yes |
Keywords
- Cosmic-ray
- Dark matter
ASJC Scopus subject areas
- Nuclear and High Energy Physics
- Astronomy and Astrophysics
- General Physics and Astronomy
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