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

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

2002-01-26

arxiv.org/abs/astro-ph/0201433v1

J.Phys.G28:1949-1952,2002

Astronomy and Astrophysics

Astrophysics

4 pages, 2 figures; presented in "Strange Quarks in Matter 2001" conference, Frankfurt am Main, Germany, 25-29 September, 2001

Scientific paper

10.1088/0954-3899/28/7/351

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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