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: | Rinchiuso, Lucia, Moult, Ian, Moulin, Emmanuel, Baumgart, Matthew, Cohen, Timothy, Vaidya, Varun, Rodd, Nicholas Llewellyn, Slatyer, Tracy Robyn, Stewart, Iain W |
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Other Authors: | Massachusetts Institute of Technology. Center for Theoretical Physics |
Format: | Article |
Language: | English |
Published: |
American Physical Society
2018
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Online Access: | 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 |
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