Abstract
Mass, radius and moment of inertia are direct probes of compositions and Equation of State (EoS) of dense matter in neutron star interior. These are computed for novel phases of dense matter involving hyperons and antikaon condensate and their observable consequences are discussed in this article. Furthermore, the relationship between moment of inertia and quadrupole moment is also explored.
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The second author, DB acknowledges fruitful discussions with Debarati Chatterjee.
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Bhat, S.A., Bandyopadhyay, D. Dense matter in strong gravitational field of neutron star. J Astrophys Astron 39, 18 (2018). https://doi.org/10.1007/s12036-017-9495-0
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DOI: https://doi.org/10.1007/s12036-017-9495-0