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Lorentz invariance violation induced threshold anomaly versus very-high energy cosmic photon emission from GRB 221009A

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arxiv 2210.06338 v6 pith:SB6IFGFH submitted 2022-10-12 astro-ph.HE gr-qchep-ph

Lorentz invariance violation induced threshold anomaly versus very-high energy cosmic photon emission from GRB 221009A

classification astro-ph.HE gr-qchep-ph
keywords energyphotonshighanomalygammainducedinvariancelorentz
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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It has been reported that the Large High Altitude Air Shower Observatory (LHAASO) observed very high energy photons from GRB 221009A, with the highest energy reaching 18~TeV. We find that observation of such high energy photons is quite nontrivial since extragalactic background light could absorb these photons severely and the flux is too weak to be observed. Therefore we discuss a potential mechanism for us to observe these photons, and suggest that Lorentz invariance violation induced threshold anomaly of the process \(\gamma\gamma\to e^-e^+\) provides a candidate to explain this phenomenon.

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Cited by 1 Pith paper

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

  1. Is There New Physics Beyond 30 TeV in the BOAT?

    astro-ph.HE 2025-11 conditional novelty 5.0

    Under quadratic subluminal Lorentz invariance violation, GRB 221009A's spectrum should show a flux recovery above ~30 TeV; the paper motivates a targeted LHAASO search but performs no data analysis.