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Dense Matter in Neutron Star: Lessons from GW170817

  • Banik S
  • Bandyopadhyay D
DOI: 10.1007/978-3-030-34234-0_8
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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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Banik, S., & Bandyopadhyay, D. (2020). Dense Matter in Neutron Star: Lessons from GW170817 (pp. 85–94). https://doi.org/10.1007/978-3-030-34234-0_8

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