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Since all protons are in nuclei, the nucleus-nucleus interaction is simply (Equation presented) times the proton-proton one.
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While the condition for stability must also be satisfied below neutron drip density, the rate at which an instability could develop in such matter would be very long, since it would demand changes in the proton and/or neutron numbers of nuclei, processes which will proceed very slowly when there are no interstitial neutrons. If the (Equation presented) and (Equation presented) of the nuclei are fixed, the system behaves as a one-component system, and the stability condition is (Equation presented). In the absence of interstitial neutrons, it has been shown that matter consisting of a mixture of two different nuclei, e.g., (Equation presented) and (Equation presented), in an NaCl structure could have a lower energy than that of the pure phases [F.J. Dyson, Ann. Phys. (N.Y.) 63, 1 (1971)]. Such phases could be of interest in the outer crusts of accreting neutron stars, where locally matter can have more than a single species of nucleus. However, we know of no studies of the stability of such a structure. APNYA6 0003-4916 10.1016/0003-4916(71)90294-6
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