Hydrogen Enhancement

In this crucial stage of the early universe, approximately 380,000 years after the Big Bang, the universe had cooled enough for protons to capture electrons, forming the first hydrogen atoms. This marked the beginning of the atomic era in our cosmos, a pivotal moment in the Cosmogenesis theory.

As the temperature dropped below 3000 Kelvin, electrons could finally remain bound to protons, creating stable atoms. This process, known as recombination, allowed light to travel freely through space for the first time, releasing what we now observe as the cosmic microwave background radiation.