Advanced Multi-Messenger Evidence for WIMP Dark Matter Decay

This study presents robust multi-messenger indications of possible WIMP (Weakly Interacting Massive Particles) decay as a viable dark matter candidate. By integrating observational data from AMS-02 (positrons), Fermi-LAT (gamma rays), and IceCube (neutrinos), we identify overlapping energy signatures in the 6-10 GeV range, spatially localized near the Galactic Center. Theoretical predictions based on NFW and Einasto halo models show strong consistency with the observed distributions. Statistical analysis using Monte Carlo simulations reveals a significance exceeding 3o in 85% of the trials. These results underscore the power of coordinated multi-channel astrophysical detection in probing dark matter and exploring physics beyond the Standard Model.