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.
Title resolution pending
5 Pith papers cite this work. Polarity classification is still indexing.
5
Pith papers citing it
fields
astro-ph.HE 5verdicts
UNVERDICTED 5representative citing papers
Flux eruptions in MADs enhance non-axisymmetry near the black hole via m=1 and m=2 modes driven by vertical magnetic flux bundles formed through reconnection and expelled by buoyancy.
Spectral index maps of the limb-brightened jet in 3C 84 show significant evolution across three epochs, indicating dynamic filamentary structures, evolving magnetic fields, and interaction with the ambient medium.
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.
EP250416a is an X-ray-rich long GRB at z=0.963 showing a late jet break at 1.5e6 s and optical darkness explained by A_V^host = 5.5 mag extinction.
citing papers explorer
-
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.
-
The azimuthal structure of magnetically arrested disks during flux eruption events
Flux eruptions in MADs enhance non-axisymmetry near the black hole via m=1 and m=2 modes driven by vertical magnetic flux bundles formed through reconnection and expelled by buoyancy.
-
Spectral index evolution of the limb-brightened jet in 3C 84
Spectral index maps of the limb-brightened jet in 3C 84 show significant evolution across three epochs, indicating dynamic filamentary structures, evolving magnetic fields, and interaction with the ambient medium.
-
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.
-
Multi-wavelength study of EP250416a / GRB 250416C: An Optically Dark Long GRB with a Late Jet Break
EP250416a is an X-ray-rich long GRB at z=0.963 showing a late jet break at 1.5e6 s and optical darkness explained by A_V^host = 5.5 mag extinction.