It's about nuclear density. Neutron stars are held up by neutron degeneracy pressure.
Another fun fact is that the magnetic field energy density alone near the surface of a pulsar (1e12 gauss and up) is about that of lead. (~40 g/cm^3).
Another fun fact is that the magnetic field energy density alone near the surface of a pulsar (1e12 gauss and up) is about that of lead. (~40 g/cm^3).