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When a star reaches the end of its life, it enters a process that leads to a phenomenon called a supernova. The inner part of the star collapses while the outer parts are released in an extremely energetic explosion. This phenomenon occurs in stars much more massive than the Sun and at the end of the process, a stellar remnant appears that can be a neutron star or a black hole.
Despite the fame of black holes, neutron stars are also extreme objects and have somewhat peculiar characteristics. These stars are composed mainly of neutrons and have a very high density. This is caused by gravitational pressure. In some cases, the pressure can be so intense that neutrons decay into quarks.
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