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The Galactic Center GeV excess (GCE) has garnered great interest as a possible signal of either dark matter annihilation or some novel astrophysical phenomenon, such as a new population of gamma-ray emitting pulsars.
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Julio F. Navarro, Carlos S. Frenk, and Simon D. M. White, “The Structure of cold dark matter halos,” Astrophys. J. 462
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A. W. Strong and I. V. Moskalenko, “Propagation of cosmic-ray nucleons in the galaxy,” Astrophys. J. 509
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Andrew W. Strong, “Source population synthesis and the Galactic diffuse gamma-ray emission,” The Multi-Messenger Approach to High-Energy Gamma-Ray Sources: 3rd Workshop on the Nature of Unidentified High-Energy Sources, Barcelona, Spain, 4-7 Jul, 2006 , Astrophys. Space Sci. 309
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N. Mirabal, “Dark matter vs. Pulsars: Catching the impostor,” Mon. Not. Roy. Astron. Soc. 436
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Rebecca K. Leane and Tracy R. Slatyer, “Spurious point source signals in the galactic center excess,” Phys. Rev. Lett. 125
2020
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