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Hadrons in compact stars

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Abstract

We discuss β-equilibrated and charge neutral matter involving hyperons and {ie817-1} condensates within relativistic models. It is observed that populations of baryons are strongly affected by the presence of antikaon condensates. Also, the equation of state including {ie817-2} condensates becomes softer resulting in a smaller maximum mass neutron star

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  1. Saha Institute of Nuclear Physics, 1/AF Bidhan Nagar, 700 064, Kolkata, India

    Debades Bandyopadhyay

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  1. Debades Bandyopadhyay
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Bandyopadhyay, D. Hadrons in compact stars. Pramana - J Phys 66, 817–825 (2006). https://doi.org/10.1007/BF02704780

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