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The Structure and Dynamics of GRB Jets

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arxiv astro-ph/0610379 v1 pith:C4XZ7OKC submitted 2006-10-12 astro-ph

Jonathan Granot (KIPAC , Stanford) This is my paper
classification astro-ph
keywords structuredynamicsjetsgrbsaccelerationburstscollimatedcollimation
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There are several lines of evidence which suggest that the relativistic outflows in gamma-ray bursts (GRBs) are collimated into narrow jets. The jet structure has important implications for the true energy release and the event rate of GRBs, and can constrain the mechanism responsible for the acceleration and collimation of the jet. Nevertheless, the jet structure and its dynamics as it sweeps up the external medium and decelerates, are not well understood. In this review I discuss our current understanding of GRB jets, stressing their structure and dynamics.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 15 citations worldwide. Full citation record

  1. Compact Objects Merging with Stars as an Origin of Ultra-Long Gamma-Ray Bursts and Luminous Fast Blue Optical Transients

    astro-ph.HE 2026-07 conditional novelty 6.0 of 10

    SN 2011kl is broadly consistent with an LFBOT light-curve model and ULGRB hosts match LFBOT/LGRB environments, supporting a shared He-CO merger progenitor for a subset of both classes.

  2. Probing a new subclass of llGRB-SN transients: Insights from EP250304a and its associated supernova

    astro-ph.HE 2026-06 unverdicted novelty 5.0 of 10

    EP250304a/SN 2025fhm is presented as a member of an emerging subclass of shocked cocoon-dominated low-luminosity GRB-SNe based on spectral, photometric, and light-curve modeling comparisons to prior events.

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