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A structured jet explains the extreme GRB 221009A

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arxiv 2302.07906 v1 pith:VZ4PO36R submitted 2023-02-15 astro-ph.HE

classification astro-ph.HE
keywords approxenergyexplosionsextremegrbsobservedstructuredafterglow
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

Long duration gamma-ray bursts (GRBs) are powerful cosmic explosions, signaling the death of massive stars. Among them, GRB 221009A is by far the brightest burst ever observed. Due to its enormous energy ($E_\textrm{iso}\!\approx$10$^{55}$ erg) and proximity ($z\!\approx$0.15), GRB 221009A is an exceptionally rare event that pushes the limits of our theories. We present multi-wavelength observations covering the first three months of its afterglow evolution. The X-ray brightness decays as a power-law with slope $\approx\!t^{-1.66}$, which is not consistent with standard predictions for jetted emission. We attribute this behavior to a shallow energy profile of the relativistic jet. A similar trend is observed in other energetic GRBs, suggesting that the most extreme explosions may be powered by structured jets launched by a common central engine.

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Forward citations

Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Polarization of impulsive relativistic jets propagating in a stratified medium

    astro-ph.HE 2026-07 conditional novelty 5.0 of 10

    Stratified external media reduce and slow the temporal evolution of afterglow polarization in impulsive jets, with the polarization peak near the geometrical light-curve break.

  2. EuraGovExam: A Multilingual Multimodal Benchmark from Real-World Civil Service Exams

    cs.CV 2026-03 unverdicted novelty 5.0 of 10

    EuraGovExam is a real-exam, image-only multilingual multimodal benchmark on which state-of-the-art VLMs reach only ~86% accuracy.

  3. On the Duration of Gamma-Ray Bursts

    astro-ph.HE 2024-12 conditional novelty 4.0 of 10

    GRB duration is shaped by the progenitor, the central engine, the emitter, and geometry, so short versus long duration is not a reliable direct indicator of what exploded or merged.

  4. Gamma-ray bursts: what do we know today that we did not know 10 years ago?

    astro-ph.HE 2024-12 unverdicted

    A review of the past decade of gamma-ray burst research, highlighting structured jets, GR-MHD simulations, TeV detections, and the contested idea that many GRBs have moderate Lorentz factors.

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