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arXiv · 1712.09760

Dense Matter in Neutron Star: Lessons from GW170817

Sarmistha Banik·Debades Bandyopadhyay
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Abstract

Neutron star merger event GW170817 sets an upper limit on the maximum mass of non-rotating neutron stars. Consequently, this event puts strong constraints on the dense matter equation of state (EoS). A comparative study of dense matter equations of state (EoSs) is presented here. It is found that the $\Lambda$ hyperon EoS BHB$\Lambda\phi$ (Banik, Hempel $\&$ Bandyopadhyay 2014) constructed within the framework of the density dependent hadron field theory is favoured.

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Sarmistha Banik, Debades Bandyopadhyay. 2017-12-28. Dense Matter in Neutron Star: Lessons from GW170817. https://arxiv.org/abs/1712.09760

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