Session: Cosmology and Relativistic Astrophysics
Name: Mr. Vasileios Mpisketzis (National & Kapodistrian Univ. of Athens)
Coauthors:
No coauthors were included.
Type: Oral
Title: Impact of inhomogeneous ejecta in jet dynamics and afterglow emission in binary neutron star mergers
Abstract:
Binary neutron star (BNS) systems are prime candidates as progenitors of
gamma-ray bursts (GRB). After the remnant of the BNS merger collapses to a black
hole, a jet is powered from the central engine that may break out of the merger
ejecta, a massive dense envelope that forms upon collision. This ejecta could
be anisotropic and inhomogeneous, which may affect the dynamical evolution of
the outflow from the merger, the emerging jet, and the resulting
electromagnetic counterparts. Here, we examine how an inhomogeneous ejecta
affects the properties of the jet-ejecta cocoon, the propagation of the jet,
and finally the afterglow radiated by the jet upon deceleration. We carry out
hydro-dynamical simulations of relativistic jets launched within ejectas with
prescribed inhomogeneous distributions of matter. Effects are mostly present in the
high-latitude regions of the jet, where we find that a significant reservoir of
energy can be present, depending on the ejecta structure. On the off-axis lines
of sight expected for afterglow counterparts of GW-triggered BNS mergers, the
early afterglow emission is particularly affected by the high-latitude
structure of the jet.