How did direct collapsing black holes form so early in the universe?

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SUMMARY

Direct collapsing black holes (DCBH) formed shortly after the Big Bang, potentially weighing millions of solar masses just 1 billion years post-event. Unlike traditional stellar black holes, which are limited by stellar evolution models, DCBHs are not mass constrained and can grow significantly through accretion and mergers. Their formation is influenced by the initial density fluctuations in the early universe, which were much greater than present conditions, allowing for the rapid accumulation of mass.

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How are thees black holes formed so early in the universe, weighing millions of suns after only 1 billion years after the big bang?
 
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It is much easier for black holes to grow to great sizes via accretion and mergers under the direct collapse scenario. A DCBH seed is not mass constrained the same way as a star - which cannot exceed a few hundref M-solar under any existing stellar evolution model. They are only limited by the size of initial density fluctuations in the early universe - which could be millions of solar masses. It also bypasses the entire stellar evolution phase giving them more time to bulk up compared to a stellar mass BH. Keep in mind the early universe was much denser than now, so this could be a significant factor.
 

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