Videos

The full evolution of the system in GW170817

A full short GRB simulation from the jet launch to the afterglow phase
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First full GRMHD simulation of the Collapsar model-launching to breakout

Color map is logarithmic mass density; magnetic field lines in black
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Farthest GRMHD jet propagation in BNS ejecta

A 3D animation. Color contours correspond to logarithmic mass density.
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A successful long GRB jet emerging from a star

A 3D animation. Color contours correspond to terminal four-velocities of elements.
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Choked jet in a GW compact binary merger's ejecta

The energy density and the 4-velocity in a jet choked by GW compact binary merger's ejecta
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A successful SGRB jet

The energy density and the four velocity in a successful SGRB
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A successful LGRB

The 3D mass density in a LGRB system
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Evolution of a successful LGRB

The 3D mass density in a LGRB system
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A successful LGRB

The 3D energy density and the four velocity in a LGRB system
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A successful 3D SGRB

The 3D energy density in a SGRB system
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A successful 2D SGRB

A 2D simulation which evolves differently from the 3D
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A choked GRB jet in a star

The 2D mass density in a FGRB system
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