Self-gravity in collapsar models produces temporary jet quenching, narrower jets, and modified timescales compared to non-self-gravitating cases, potentially explaining GRB variability and failed bursts.
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GRMHD simulations of GRB 090510 predict energetics and jet opening angles consistent with observations within 1 sigma when jet angles evolve with redshift, while dynamical ejecta influence collimation and a suite of models explores broader GRB properties.
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Three-dimensional GRMHD simulations of jet formation and propagation in self-gravitating collapsing stars
Self-gravity in collapsar models produces temporary jet quenching, narrower jets, and modified timescales compared to non-self-gravitating cases, potentially explaining GRB variability and failed bursts.
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Exploring Jet Structure and Dynamics in Short Gamma Ray Bursts: A Case Study on GRB 090510
GRMHD simulations of GRB 090510 predict energetics and jet opening angles consistent with observations within 1 sigma when jet angles evolve with redshift, while dynamical ejecta influence collimation and a suite of models explores broader GRB properties.