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Galaxies 2018, 6(4), 119;

Binary Neutron Star and Short Gamma-Ray Burst Simulations in Light of GW170817

Institut für Theoretische Physik, Goethe Universität Frankfurt, Max-von-Laue-Str.1, 60438 Frankfurt am Main, Germany
Received: 16 August 2018 / Revised: 9 November 2018 / Accepted: 13 November 2018 / Published: 19 November 2018
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In the dawn of the multi-messenger era of gravitational wave astronomy, which was marked by the first ever coincident detection of gravitational waves and electromagnetic radiation, it is important to take a step back and consider our current established knowledge. Numerical simulations of binary neutron star mergers and simulations of short GRB jets must combine efforts to understand such complicated and phenomenologically rich explosions. We review the status of numerical relativity simulations with respect to any jet or magnetized outflow produced after merger. We compare what is known from such simulations with what is used and obtained from short GRB jet simulations propagating through the BNS ejecta. We then review the established facts on this topic, as well as discuss things that need to be revised and further clarified. View Full-Text
Keywords: binary neutron stars; short gamma-ray bursts; GW170817 binary neutron stars; short gamma-ray bursts; GW170817

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Nathanail, A. Binary Neutron Star and Short Gamma-Ray Burst Simulations in Light of GW170817. Galaxies 2018, 6, 119.

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