Hunting for heavy winos in the Galactic Center
Observing gamma rays using ground-based atmospheric Cherenkov telescopes provides one of the only probes of heavy weakly interacting dark matter. A canonical target is the thermal wino, for which the strongest limits come from searches for photon lines from annihilations in the Galactic Center. Irre...
| Main Authors: | , , , , , , , , |
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| מחברים אחרים: | |
| פורמט: | Article |
| שפה: | English |
| יצא לאור: |
American Physical Society
2018
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| גישה מקוונת: | http://hdl.handle.net/1721.1/119830 https://orcid.org/0000-0003-3472-7606 https://orcid.org/0000-0001-9699-9047 https://orcid.org/0000-0003-0248-0979 |