Abstract
Recently it was shown that the excess of diffuse Galactic gamma rays above 1 GeV traces the Dark Matter halo, as proven by reconstructing the peculiar shape of the rotation curve of our Galaxy from the gamma ray excess. This can be interpreted as a Dark Matter annihilation signal. In this talk we show that this interpretation is consistent with Supersymmetry. It is found that the EGRET excess combined with all electroweak constraints and WMAP CMB data is fully consistent with the minimal mSUGRA model with the neutralino mass around 60 GeV. It leads to the SUSY mass spectrum in the TeV range for scalars and gauginos below 500 GeV. The corresponding cross‐sections for SUSY production are within the reach of the LHC.
Sign-in/Register to access full text options 
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
