{
  "id": "1712.09760",
  "version": "v1",
  "published": "2017-12-28T05:47:56.000Z",
  "updated": "2017-12-28T05:47:56.000Z",
  "title": "Dense Matter in Neutron Star: Lessons from GW170817",
  "authors": [
    "Sarmistha Banik",
    "Debades Bandyopadhyay"
  ],
  "comment": "10 page, 4 figures; for the proceedings of 'FIAS International Symposion on Discoveries at the Frontiers of Science' held at FIAS, Germany",
  "categories": [
    "astro-ph.HE"
  ],
  "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.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2017-12-28T05:47:56.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "dense matter equation",
      "neutron star merger event gw170817",
      "density dependent hadron field theory",
      "star merger event gw170817 sets"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 10,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}