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Analyzing Fermi data, along with the results of an ISS experiment and gamma ray observations from dwarf galaxies that are not too far away, led researcher Mattia Di Mauro to believe that this light probably has a dark origin. This has never been hypothesized before. She was also able to figure out the shape of this gamma ray glow and how its is positioned in space, along with how much energy it emits, and published those findings in Physical Review D. “This excess of gamma rays cannot be explained with the known processes and components,” Di Mauro, who more recently coauthored a second study with colleague Martin Wolfgang Winkler, told SYFY WIRE. “A signal of dark matter particles annihilating in the center of the Galaxy is compatible with all the characteristics of the excess, including the flux, spatial distribution, and position. ....
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