- #36
Entropy
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- 0
within picoseconds of impact (and it would be in the form of neutrons)
Actually, the forces at the very surface of the neutron star are not strong enough to insue neutron degradation. The outer most surface of a neutron star is acutally composed of various atomic nuclei, mostly iron isotopes. Then as you barrow deeper neutrons will start to break free and form a neutron superfluid but still have protons and electrons mixed in with it. Then as you get even deeper it will eventually become entirely 100% neutrons. As for the core, it may just continue to be neutrons as well, but it might be that their is further degradation of neutrons into a type of quark matter.