During this brief period, the universe was incredibly hot and dense, allowing protons and neutrons to collide and fuse into the first light nuclei, primarily hydrogen (¹H) and helium (⁴He). Trace amounts of deuterium (²H), tritium (³H), and lithium (⁷Li) were also created.
This event is crucial because it laid the foundation for the formation of stars, galaxies, and eventually, all the elements we see today.