Dark Matter Detection via Radio Waves
Dark matter clumps formed during the cosmic dark ages (100 million years post-Big Bang) seeded galaxies.
Radio antennas and the Square Kilometre Array (SKA) aim to detect faint emissions from dark matter clumps.
Lunar telescopes avoid atmospheric interference for dark matter observations.
Successful detection would test dark matter theories and reveal galaxy seeding structures.
Prof. Barkana leads an international team working on SKA and lunar telescope projects.
Recent JWST findings highlight opportunities for studying the early Universe.