Connecting GRBs from Binary Neutron Star Mergers to Nuclear Properties of Neutron Stars

Rosalba Perna, Ore Gottlieb, Estuti Shukla +1

The fate of the binary neutron star (NS) merger remnants hinges sensitively upon the NS equation of state and the threshold mass, $M_{\mathrm{ls}}$, that separates a long-lived from a s…