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we are concerned with the latter case. OCR Output calculations [2,3] and in studying properties of dense matter in neutron stars [4,5] VVe find that Skyrme forces with 2:2 in this range provide very good parameterization of .7:2, which was neglected in spin-saturated systems, is in the range **5//1 < 232 §-1. consistent description of polarized neutron matter requires that the exchange parameter There is, however, no ground state and the system displays a singular behaviour. Physically of polarized neutron matter. This instability has a form ofthe ferromagnetic spin ordering.It is shown that Skyrme forces with a commonly used parameter tg < 0 lead to instability Abstract:

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