What happens to matter when gravity crushes it beyond the breaking point? Inside a neutron star, atoms are destroyed. Electrons are forced into protons. Nuclei dissolve into a sea of neutrons. And at the very center, even neutrons themselves may break apart into quarks — forming exotic states of matter that physicists still can’t fully explain.
In this video, we go inside a neutron star layer by layer. From the crystalline outer crust where neutron-rich nuclei sit in a lattice denser than anything on Earth, through the bizarre nuclear pasta phases where matter forms sheets, tubes, and bubbles of nuclear material, into the superfluid outer core where neutrons flow without friction and protons conduct without resistance, and finally into the mysterious inner core where densities reach five to ten times that of an atomic nucleus and the very concept of a \.






