Magnetars, a type of neutron star, can exist despite the high density of neutrons because neutron stars are not homogenous and contain significant amounts of protons and electrons, particularly in their crusts and cores. The crust of a neutron star is composed of polarized nuclei and free electrons, while the core contains a mix of neutrons, protons, and possibly exotic baryons. The dynamic environment of neutron stars allows for ongoing nuclear reactions, which can affect the composition and charge of their components. Resources for further understanding include detailed academic papers and books that explore the structure and magnetic fields of magnetars. The complexity of neutron stars and magnetars highlights the need for more accurate and detailed descriptions in astrophysics literature.