• Hybrid stars

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    • Keywords


      Neutron stars; phase transition

    • 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.

    • Author Affiliations


      Ashok Goyal1

      1. Department of Physics and Astrophysics, University of Delhi, Delhi - 110 007, India
    • Dates

  • Pramana – Journal of Physics | News

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      Posted on July 25, 2019

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