High-resolution calculations of merging neutron stars - II. Neutrino emission
High-resolution calculations of merging neutron stars - II. Neutrino emission
The remnant resulting from the merger of two neutron stars produces neutrinos in copious amounts. In this paper we present the neutrino emission results obtained via Newtonian, high-resolution simulations of the coalescence event. These simulations use three-dimensional smoothed particle hydrodynamics together with a nuclear, temperature dependent equation of state and …