Pith. sign in

REVIEW 4 cited by

On ALP scenarios and GRB 221009A

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2211.02010 v2 pith:3E2TFSNS submitted 2022-11-03 astro-ph.HE hep-ph

classification astro-ph.HEhep-ph
keywords accountbackgroundeventeventsobservationsphotonscenarioabsorbed
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
read the original abstract

The extraordinarily bright gamma-ray burst GRB 221009A was observed by a large number of observatories, from radio frequencies to gamma-rays. Of particular interest are the reported observations of photon-like air showers of very high energy: an 18 TeV event in LHAASO and a 251 TeV event at Carpet-2. Gamma rays at these energies are expected to be absorbed by pair-production events on background photons when travelling intergalactic distances. Several works have sought to explain the observations of these events, assuming they originate from GRB 221009A, by invoking axion-like particles (ALPs). We reconsider this scenario and account for astrophysical uncertainties due to poorly known magnetic fields and background photon densities. We find that, robustly, the ALP scenario cannot simultaneously account for an 18 TeV and a 251 TeV photon from GRB 221009A.

Discussion (0). Continue with ORCID to comment.

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. Search for Axions in Magnetic White Dwarf Polarization at Lick and Keck Observatories

    hep-ph 2025-04 accept novelty 6.0 of 10

    Dedicated Lick and Keck spectropolarimetry of magnetic white dwarfs finds no axion-induced linear polarization and sets |g_aγγ| < 1.7e-12 GeV^-1 at 95% CL for m_a < 2e-7 eV.

  2. Carpet-3 detection of a photon-like air shower with estimated primary energy above 100 TeV in a spatial and temporal coincidence with GRB 221009A

    astro-ph.HE 2025-02 conditional novelty 6.0 of 10

    Carpet-3 reports a photon-like air shower with estimated energy around 300 TeV arriving from the direction of GRB 221009A about 75 minutes after the trigger, with a coincidence probability of about 0.9 percent.

  3. Self-organized critical characteristics of teraelectronvolt photons from GRB 221009A

    astro-ph.HE 2024-12 conditional novelty 5.0 of 10

    Waiting times of TeV photons from GRB 221009A show power-law and scale-invariant statistics, which the authors interpret as self-organized critical behavior with non-independent photon emission.

  4. Lecture Notes: WISPs in gamma-ray astrophysics

    astro-ph.HE 2025-05 unverdicted novelty 1.0 of 10

    The paper is a pedagogical review of axion-like particle searches in gamma-ray astrophysics, with tutorial derivations and a notebook-based analysis of NGC 1275, and it contains no new research result.

Pith tools