Hunting for heavy winos in the Galactic Center

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...

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Detaylı Bibliyografya
Asıl Yazarlar: Rinchiuso, Lucia, Moult, Ian, Moulin, Emmanuel, Baumgart, Matthew, Cohen, Timothy, Vaidya, Varun, Rodd, Nicholas Llewellyn, Slatyer, Tracy Robyn, Stewart, Iain W
Diğer Yazarlar: Massachusetts Institute of Technology. Center for Theoretical Physics
Materyal Türü: Makale
Dil:English
Baskı/Yayın Bilgisi: American Physical Society 2018
Online Erişim: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

Internet

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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