At the moment of the Big Bang, a large amount of energy and matter burst out and expanded outward at an alarming rate.
During the explosion, a lot of energy and matter are ejected from the singularity. After the "expanding" universe cooled rapidly, particles in space began to synthesize. First quarks condense into protons and neutrons, and then protons and neutrons gather together to form nuclei. The earliest nuclei in the universe are hydrogen nuclei and helium nuclei. The universe in this period is a high-temperature chaotic state full of energy and particles.
Quarks synthesize protons and neutrons.
Hydrogen nucleus and helium nucleus
After 380,000 years, electrons joined them to form atoms, which are still mainly hydrogen and helium. During this period, the universe gradually cooled down and began to become orderly.
= hydrogen atom and helium atom with electrons
After 400 million years, under the action of gravity, hydrogen began to gather together, forming primitive stars and galaxies. The universe in this period can be said to be the embryonic form of the modern universe.
A nectar-like protogalaxy
Later, after a long evolution of1300 million years, the universe became what it is now. If you use a picture to represent this process, as shown below:
To sum up, the evolution of the universe is roughly as follows: singularity explosion-high temperature inflation-high temperature chaos-orderly cooling-primitive galaxies-modern universe.
-The above content is taken from Millay's children's book A Brief History of Life.