The characterization of the gamma-ray signal from the central Milky Way: A case for annihilating dark matter

The characterization of the gamma-ray signal from the central Milky Way: A case for annihilating dark matter

Past studies have identified a spatially extended excess of ~1-3 GeV gamma rays from the region surrounding the Galactic Center, consistent with the emission expected from annihilating dark matter. We revisit and scrutinize this signal with the intention of further constraining its characteristics a...

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Bibliographic Details
Main Authors: Daylan, Tansu, Finkbeiner, Douglas P., Hooper, Dan, Linden, Tim, Portillo, Stephen K.N., Rodd, Nicholas Llewellyn, Slatyer, Tracy Robyn
Other Authors: Massachusetts Institute of Technology. Center for Theoretical Physics
Format: Article
Published: Elsevier BV 2018
Online Access:http://hdl.handle.net/1721.1/116342
https://orcid.org/0000-0003-3472-7606
https://orcid.org/0000-0001-9699-9047

Internet

http://hdl.handle.net/1721.1/116342
https://orcid.org/0000-0003-3472-7606
https://orcid.org/0000-0001-9699-9047

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