If it weren’t for the intricate rules of quantum physics, we wouldn’t have formed neutral atoms “only” ~380,000 years after the Big Bang.
In order for you to exist, a lot of things had to happen beforehand. Planet Earth needed to come into existence, complete with the organic ingredients from which life could arise. In order to have those ingredients, we need for many previous generations of stars to have lived-and-died, recycling the elements formed within them back into the interstellar medium. For those stars to live, large quantities of neutral, molecular gas had to collect in one place, collapsing under its own gravity to fragment and form stars in the first place. But in order to make those stars — even the very first stars — we first need the Universe to create stable, neutral atoms.
In a Universe that begins with a hot Big Bang, this isn’t necessarily so easy! A few minutes after the hot Big Bang, our Universe was filled with protons and a small but important population of more complex light atomic nuclei, an equal number of electrons to the total number of protons, a large number of neutrinos that don’t interact with any of them, and about 1.4 billion photons for every proton-or-neutron present. (There’s also dark matter…
