Abstract
Models of neutron stars with a quark core are calculated on the basis of an extensive set of equations of state for superdense matter. The possible existence of a new branch of stable layered neutron stars is revealed for some realistic equations of state of neutron matter.
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Harutyunyan, A.R. Neutron Stars With a Quark Core. Astrophysics 45, 248–251 (2002). https://doi.org/10.1023/A:1016029319324
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DOI: https://doi.org/10.1023/A:1016029319324