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Summary: The paper investigates the origin of supermassive black holes (SMBHs), proposing that primordial black holes (PBHs) may have served as their seeds. These hypothetical PBHs, thought to have formed in the universe’s earliest moments, could have clustered in high-density regions, becoming galaxy centers. As these clusters collapsed, PBHs merged rapidly due to gas friction, forming massive black hole seeds. This theory offers a solution to how SMBHs grew so large so early, as PBHs would have started with significant mass, avoiding unrealistic growth rates. Predictions align with early SMBH observations by the JWST, and future gravitational wave detections could support the theory. While further testing is needed, this work opens new paths in black hole and cosmology research. Link to paper: https://arxiv.org/abs/2411.03448 The Audio is AI generated and made with: https://notebooklm.google.com/