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

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dc.creatorBanik, Sarmistha
dc.creatorBandyopadhyay, Debades
dc.date2002-01-26
dc.date.accessioned2026-07-07T10:47:22Z
dc.date.available2026-07-07T10:47:22Z
dc.descriptionWe 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.
dc.description4 pages, 2 figures; presented in "Strange Quarks in Matter 2001" conference, Frankfurt am Main, Germany, 25-29 September, 2001 and to be published in J. Phys. G
dc.identifierhttps://arxiv.org/abs/astro-ph/0201433
dc.identifierhttp://arxiv.org/abs/astro-ph/0201433
dc.identifierJ.Phys.G28:1949-1952,2002
dc.identifierdoi:10.1088/0954-3899/28/7/351
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/183511
dc.subjectAstrophysics
dc.titleBose-Einstein condensation in dense matter and the third family of compact stars
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