The multimessenger event of August 17, 2017, demonstrated that binary neutron star (BNS) systems can merge and power collimated relativistic outflows (jets) that are compatible with the prompt and afterglow emission of short gamma-ray bursts (GRBs). However, many open questions remain about the physical mechanisms behind this connection, calling for advanced numerical modeling of the merger and jet propagation stages up to the formation of electromagnetic signals. In this talk, I will present results of three-dimensional relativistic (magneto)hydrodynamic short GRB jet simulations that we carried out by employing, for the first time, self-consistent initial conditions for the jet propagation environment directly imported from the outcome of general-relativistic BNS merger simulations, also carried out by our group. The results presented will soon allow us to make direct and more solid comparisons with the afterglow data of 170817, establishing a powerful new approach for the interpretation of similar events in the future.
Link alla videochiamata: https://meet.google.com/vap-tnxs-soq
Oppure digita: (IT) +39 02 3046 1455 PIN: 634 762 978#
Riccardo Ciolfi