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Bose-Einstein condensation in dense matter and the third family of compact stars

Sarmistha Banik·Debades Bandyopadhyay
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Abstract

We investigate antikaon condensation in compact star matter using a relativistic mean field model. Antikaon condensates make the equation of state softer resulting in a smaller maximum mass star compared to the case without condensate. It is found that the equation of state including antikaon condensates gives rise to a stable sequence of compact stars called the third family beyond the neutron star branch.

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Sarmistha Banik, Debades Bandyopadhyay. 2002-01-26. Bose-Einstein condensation in dense matter and the third family of compact stars. https://doi.org/10.1088/0954-3899%2F28%2F7%2F351

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