Mysterious Galactic Core Phenomenon May Unveil a New Form of Dark Matter

By analyzing hydrogen gas in the CMZ, scientists propose a paradigm shift in dark matter research. This low-mass candidate may explain the enigmatic 511-keV emission line observed in the galactic core. Dr. Shyam Balaji emphasizes that traditional Earth-based dark matter experiments may need to be reconsidered, as this new approach provides direct observational evidence, potentially bringing us closer to unlocking the universe’s most elusive mystery.

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