Feb 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006sgrb.confe..51p&link_type=abstract
Presented at the KITP Conference: Supernova and Gamma-Ray Burst Remnants, Feb 6, 2006, Kavli Institute for Theoretical Physics,
Physics
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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