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If the neutron star's density is more than that of a neutron, the neutrons within the star are overlapping; if it is less, the neutrons are not...
If the neutron star's density is more than that of a neutron, the neutrons within the star are overlapping; if it is less, the neutrons are not overlapping. Which of these seems to be the case for average neutrons within the star? Which do you think is the case at the center of the neutron star, where densities are higher than average?