👉 The origins fluid, also known as primordial fluid or protofluid, is a theoretical substance proposed to be the earliest form of matter in the universe before the formation of atoms and subatomic particles. It is thought to have existed during the extremely high-energy conditions of the Big Bang, where temperatures and densities were so extreme that all known forms of matter were in a state of ionization. As the universe expanded and cooled, these conditions allowed quarks and gluons to combine into protons and neutrons, marking the transition from the origins fluid to the first atomic nuclei. This primordial fluid eventually condensed into the first atoms, primarily hydrogen and helium, setting the stage for the formation of stars, galaxies, and ultimately, the complex structures we observe today.
