pith:RLKGU3OB
Correlation between Ultrahigh-Energy Neutrino KM3-230213A and Gamma-Ray Bursts
The 220 PeV neutrino KM3-230213A correlates with a larger set of gamma-ray bursts once directional uncertainties are included.
arxiv:2604.13879 v2 · 2026-04-15 · astro-ph.HE · gr-qc · hep-ph
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\pithnumber{RLKGU3OBYLZJJZ464XF5REZKDR}
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Record completeness
Claims
Our analysis identifies a larger set of correlated GRBs. For each associated GRB, we compute the LV scale, integrating uncertainties from redshift measurements and neutrino energy determinations to enhance the robustness of our findings.
That directional overlap within quoted angular uncertainties implies a physical association rather than chance coincidence, and that any arrival-time difference is attributable to Lorentz violation rather than production delays or propagation effects unrelated to LV.
Correlations are identified between the ultra-high-energy neutrino KM3-230213A and multiple gamma-ray bursts, yielding Lorentz violation scales that fold in redshift and energy uncertainties.
Receipt and verification
| First computed | 2026-05-25T02:01:20.265327Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
8ad46a6dc1c2f294e79ee5cbd8932a1c678ff3d5db29d435926e8690b4d7b057
Aliases
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/RLKGU3OBYLZJJZ464XF5REZKDR \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 8ad46a6dc1c2f294e79ee5cbd8932a1c678ff3d5db29d435926e8690b4d7b057
Canonical record JSON
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"license": "http://creativecommons.org/licenses/by/4.0/",
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"submitted_at": "2026-04-15T13:41:28Z",
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