Tracing the imprints of large-scale magnetized structure on γ rays from GRB 221009A

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250415890v1.pdf (3.42 MB)

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http://arxiv.org/abs/2504.15890

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https://doi.org/10.48550/arXiv.2504.15890
 http://hdl.handle.net/11603/38701

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UMBC Center for Space Sciences and Technology (CSST) / Center for Research and Exploration in Space Sciences & Technology II (CRSST II)
UMBC Faculty Collection

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https://orcid.org/0000-0002-7021-5838

Date

2025-04-22

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journal articles
preprints
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Citation of Original Publication

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Subjects

Astrophysics - High Energy Astrophysical Phenomena

Abstract

We search for possible GeV-TeV gamma-ray imprints of ultrahigh-energy (UHE; ≳ 0.1 EeV) cosmic ray (CR) acceleration in the large-scale structures surrounding the brightest gamma-ray burst (GRB) explosion, GRB 221009A. Using 1.25 years of post-event Fermi Large Area Telescope (LAT) data, we construct a 1 GeV – 1 TeV test-statistic (TS) map within 15 Mpc of the burst. We identify two peaks in the TS map with TS ≥ 9. The most significant peak, J1911.8+2044, exhibits gamma-ray emission in pre-burst LAT data. The other peak, J1913.2+1901, coincides with a 664.6 GeV photon recorded ∼ 191.9 days after the GRB trigger and located at about 0.75◦ from the GRB localization. The per-photon 95% containment angle for the LAT is about 0.25◦ in the 100 GeV – 1 TeV energy range. We explore two possible origins for the γ-ray emission: (1) UHECRs from GRB 221009A propagating through a magnetized cosmological volume in its vicinity, and (2) UHE or very high-energy (VHE; ≳ 100 GeV) γ-ray emission from GRB 221009A, propagating in the same volume. In both cases, electromagnetic cascade emission is induced in the structured region embedding the burst. If any TS features are related to large-scale imprints induced by cosmic rays, it might be further evidence that GRB 221009A accelerated UHECRs. However, our results show that alternative scenarios without invoking UHECRs cannot be ruled out, and the observed high-energy photon could be unrelated to GRB 221009A.