Evidence against solidification of a model neutron system

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Abstract
It is argued, on the basis of (a) recent ideas of Feenberg on the representation of the wave function of a solid together with (b) the accurate equation-of-state data calculated by Shen, Sim, and Woo, that a system of Boltzmann neutrons interacting via the soft repulsive core of the Reid S01 potential fails to crystallize at densities relevant to neutron stars.

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