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Abstract: We calculate several neutron star properties, for static and-or rotatingstars, using equations of state based on different microscopic models. Theseinclude our Dirac-Brueckner-Hartree-Fock model and others derived from thenon-relativistic Brueckner-Hartree-Fock approach implemented with microscopicthree-body forces. The model dependence is discussed.



Author: F. Sammarruca, Pei Liu

Source: https://arxiv.org/



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