Anomalous coupling in radiation mediated shocks

We summarize recent attempts to unravel the role of plasma kinetic effects in radiation mediated shocks. Such shocks form in all strong stellar explosions and are responsible for the early electromagnetic emission released from these events. A key issue that has been overlooked in all previous works is the nature of the coupling between the charged leptons, that mediate the radiation force, and the ions, which are the dominant carriers of the shock energy. Our preliminary investigation indicates that in the case of relativistic shocks, as well as Newtonian shocks in multi-ion plasma, this coupling is driven by either, transverse magnetic fields of a sufficiently magnetized upstream medium, or plasma microturbulence if strong enough magnetic fields are absent. We discuss the implications for the shock breakout signal, as well as abundance evolution and kilonova emission in binary neutron star mergers.

Automated summary

We summarize recent attempts to understand the role of plasma kinetic effects in radiation mediated shocks. Our research indicates that the coupling between charged leptons and ions in relativistic and multi-ion plasma shocks is driven by transverse magnetic fields or plasma microturbulence. We discuss the implications for shock breakout signals, abundance evolution, and kilonova emission in binary neutron star mergers.