| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8133034 | Astroparticle Physics | 2013 | 6 Pages |
Abstract
⺠CTA will mean a significant increase of the potential for indirect dark matter detection. ⺠The annihilation rate for TeV WIMPs may be high, for a variety of reasons. ⺠A low energy threshold would be beneficial. ⺠A complement to CTA in the form of a high-altitude, low energy threshold dedicated dark matter array may be contemplated.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Lars Bergström,