Hiroyuki Tajima

Inside a neutron star, matter is compressed so intensely that atomic nuclei fuse into long strands and flat sheets. Astrophysicists call these structures nuclear pasta. At their surface, the density of matter plummets to nearly zero, like diving out of thick jelly into thin air. It's this sharp transition that creates the unusual effect.

Neutron stars are cosmic alchemical retorts: at supranuclear densities, hadrons melt into quark-gluon plasma (QGP), and at the very core where pressure peaks, a color superconductor (CS) is born.