Making a GRB Jet

Physics

Scientific paper

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Scientific paper

I review recent results from numerical simulations of a magnetized flow inthe vicinity of a black hole in the context of the collapsar model forGRBs.The simulations show that after an initial transient, the flow settles intoa complex convolution of several distinct flow components. I discuss thenature and connection between these components, in particular between theinflows and related outflows. I also discuss how and under what conditionsthe collapsing stellar envelope can trigger a very strong and fast outflowthat can become a super-relativistic jet.

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