Role of injection parameters in jet propagation through realistic binary neutron star merger environments
Andrea Pavan, Riccardo Ciolfi, Emma Dreas, Jay V. Kalinani

TL;DR
This study uses 3D RMHD simulations to investigate how injection parameters and realistic merger environments influence jet propagation in binary neutron star mergers, highlighting environment impact on jet success.
Contribution
First comprehensive 3D RMHD simulation suite examining how injection parameters and realistic merger environments jointly affect jet evolution in BNS mergers.
Findings
Jet fate depends on environment properties even with identical injection parameters.
Realistic environments cause significant differences in jet breakout compared to simplified models.
Environment plays a central role in shaping jet evolution and success.
Abstract
After the first multi-messenger observation of a binary neutron star (BNS) merger powering a short-duration gamma-ray burst (GRB), GW170817-GRB 170817A, remarkable effort is ongoing to unravel the evolution of the collimated, relativistic outflow (or jet) that was launched during the merger and fed the GRB event, imprinting its angular structure onto the follow-up afterglow signal. Current theoretical models, based on relativistic magneto-hydrodynamic (RMHD) simulations, offer detailed insights into the launch and propagation processes that govern jet evolution. Notably, these simulations point out that jet injection parameters, such as luminosity, magnetization, power decay time scale, and launch time relative to merger, play a crucial role. However, the impact of these parameters is typically investigated within simplified jet propagation environments, lacking a direct connection with…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Pulsars and Gravitational Waves Research · Laser-Plasma Interactions and Diagnostics
