• Fulltext


        Click here to view fulltext PDF

      Permanent link:

    • Keywords


      Dense matter; Bose-Einstein condensation; neutron star; third family of compact stars

    • Abstract


      We investigate the role of Bose-Einstein condensation (BEC) of anti-kaons on the equation of state (EoS) and other properties of compact stars. In the framework of relativistic mean field model we determine the EoS for β-stable hyperon matter and compare it to the situation when anti-kaons condense in the system. We observe that anti-kaon condensates soften the EoS, thereby lowering the maximum mass of the stars. We also demonstrate that the presence of antikaon condensates in the high density core of compact stars may lead to a new mass sequence beyond white dwarf and neutron stars. The limiting mass of the new sequence stars is nearly equal to that of neutron star branch though they have distinctly different radii and compositions. They are called neutron star twins.

    • Author Affiliations


      Sarmistha Banik1 Debades Bandyopadhyay1

      1. Saha Institute of Nuclear Physics, 1/AF Bidhan Nagar, Kolkata - 700 064, India
    • Dates

  • Pramana – Journal of Physics | News

    • Editorial Note on Continuous Article Publication

      Posted on July 25, 2019

      Click here for Editorial Note on CAP Mode

© 2021-2022 Indian Academy of Sciences, Bengaluru.