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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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.