Abnormal neutron star matter at ultrahigh densities |
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| Authors: | S.A. Moszkowski C.G. Källman |
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| Affiliation: | University of California, Los Angeles, California 90024, USA;Åbo, Akademi, Åbo, Finland |
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| Abstract: | We consider three models, based on the mean field and sigma models, all of which fit the saturation properties and the symmetry energy of nuclear matter. None of the models yields an abnormal state of neutron star matter at supemuclear density even when pion condensation is taken into account. |
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