Summary:
- The article discusses a new study that has identified a key mechanism underlying the formation of supermassive black holes in the early universe.
- Researchers used computer simulations to show that the rapid growth of these black holes was driven by the efficient accretion of gas from their surrounding environments, enabled by the collapse of massive, rotating gas clouds.
- The findings provide important insights into the origins of the first supermassive black holes, which are believed to have played a crucial role in the formation and evolution of the earliest galaxies in the universe.