The Fermi Galactic Center GeV Excess and Implications for Dark Matter
By M. Ackermann, M. Ajello, A. Albert, W. Atwood, L. Baldini, J. Ballet, G. Barbiellini, D. Bastieri, R. Bellazzini, E. Bissaldi and 122 more. 2017
176 citations recorded by the source corpus.
Subfields: Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/66c51bbac57fe6528194a8747c505b34c7e1785a
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In Nuclear and High Energy Physics
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- Anna Franckowiak
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- G. Zaharijas
- Igor V. Moskalenko
Citations in the corpus
- The Search for Spatial Extension in High-latitude Sources Detected by the Fermi Large Area Telescope (2018, methodology): “3+04.5 (Ackermann et al. 2016a), and M31(Ackermann et al. 2017a).”
- WIMP dark matter candidates and searches—current status and future prospects (2017, methodology): “ze out and then decay into EWIMPs. Note that in this case the resulting number density of DM is still determined at freeze-out. Alternatively, EWIMPs can be produced 5They are also called super-WIMPs [279] or FIMPs [78] (feebly interacting massive particles, although the name of frozen-in massive pa”