Abstract
Recently there have been important developments in the determination of neutron star masses which put severe constraints on the composition and equation of state (EOS) of the neutron star matter. Here we study the effect of quark and nuclear matter mixed phase on mass radius relationship of neutron stars employing recent models from two classes of EOS’s and discuss their implications.
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Goyal, A. Hybrid stars. Pramana - J Phys 62, 753–756 (2004). https://doi.org/10.1007/BF02705363
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DOI: https://doi.org/10.1007/BF02705363