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The hot big-bang model is the prevailing theory for the universe's evolution. It posits that the universe began 13.8 billion years ago from a state of extreme heat and density. This expansion caused a significant decrease in density and temperature, leading to the formation of hydrogen, helium, and lithium nuclei.1

Key assumptions of the model include the accuracy of Einstein's general theory of relativity and the cosmological principle, which states that the universe is uniform on large scales. About a million years after the big bang, atoms formed, allowing radiation to travel freely, creating the cosmic microwave background radiation detected today. While alternative theories have been proposed, the hot big-bang model remains dominant due to its ability to explain a wide range of cosmological observations.12

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