Sarmistha Banik

A Third family of superdense stars in the presence of anti-kaon condensates

The formation of

Density dependent hadron field theory for neutron stars with antikaon condensates

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Antikaon condensation and the metastability of protoneutron stars

and

Massive Neutron Stars with Antikaon Condensates in a Density Dependent Hadron Field Theory

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Rotating compact stars with exotic matter

condensation in

Nuclear symmetry energy in the presence of hyperons in the non-relativistic Thomas-Fermi approximation

\beta

Neutron Star Physics in the Square Kilometre Array Era: An Indian Perspective

-equilibrated hyperonic matter is investigated within a relativistic mean field model. In this model, baryon-baryon and (anti)kaon-baryon interactions are mediated by the exchange of mesons. It is found that antikaon condensation is not only sensitive to the equation of state but also to antikaon optical potential depth. For large values of antikaon optical potential depth,

A Comparative study of hyperon equations of state in supernova simulations

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The “horn” in the kaon-to-pion ratio

condensation sets in before the appearance of negatively charged hyperons. We treat

Critical mass, moment of inertia and universal relations of rapidly rotating neutron stars with exotic matter

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