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arxiv: 1907.04244 · v1 · pith:6KJPFWFVnew · submitted 2019-07-09 · ✦ hep-ex · hep-ph

Search for Lorentz Violation Using High-Energy Atmospheric Neutrinos In IceCube

Pith reviewed 2026-05-24 23:57 UTC · model grok-4.3

classification ✦ hep-ex hep-ph
keywords Lorentz violationIceCubeatmospheric neutrinoshigh-energy neutrinoshigh-dimensional operatorsneutrino constraints
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The pith

Analysis of two years of IceCube data places some of the strongest constraints on Lorentz violation for high-dimensional operators using atmospheric neutrinos.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

The paper examines high-energy atmospheric neutrinos detected by IceCube to test for Lorentz violation. These neutrinos serve as sensitive probes because their high energies make effects from high-dimensional operators more detectable. The analysis of two years of data yields no evidence of violation but produces tight limits on the relevant parameters. A reader would care because any Lorentz violation would point to physics beyond the standard model, and this uses an existing large dataset in a targeted way to search for it.

Core claim

High-energy atmospheric neutrinos observed by the IceCube Neutrino Observatory are extremely sensitive probes of Lorentz violation. Analyzing two years of IceCube data in the search for LV places some of the strongest constraints on LV when considering high-dimensional operators.

What carries the argument

High-energy atmospheric neutrinos detected in IceCube, used as probes whose long baselines and high energies amplify potential Lorentz-violating effects from high-dimensional operators.

If this is right

  • No signal of Lorentz violation appears in the analyzed dataset.
  • The resulting limits on high-dimensional LV coefficients rank among the strongest existing bounds.
  • Additional IceCube data would allow these constraints to be tightened further.
  • The same dataset and method remain available for testing other possible LV signatures.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • These limits could restrict classes of quantum-gravity models that predict Lorentz violation at accessible energies.
  • The technique of using atmospheric neutrinos for LV searches could be adapted to other large neutrino detectors.
  • Cross-checks with cosmic-ray or accelerator data might test whether the IceCube constraints hold across different energy regimes.

Load-bearing premise

The IceCube data and standard neutrino flux models accurately capture all relevant effects without unmodeled systematics that could mimic or hide Lorentz violation signals.

What would settle it

An observed pattern of neutrino arrival directions or energies showing an anomalous dependence that matches a specific high-dimensional Lorentz-violating term but cannot be reproduced by standard atmospheric neutrino flux and oscillation calculations.

Figures

Figures reproduced from arXiv: 1907.04244 by Carlos A. Arg\"uelles.

Figure 1
Figure 1. Figure 1: (left). At high energies, where m2 2E is negligible, the ντ appearance probability is given by 5 P (νµ → ντ ) ∼ [PITH_FULL_IMAGE:figures/full_fig_p002_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: Constraints on Lorentz violation dimension six operator. Left: Constraints in term of the LV strength (horizontal axis) and the ratio of diagonal to total strength (vertical axis). The best-fit point of the analysis is marked by the standard yellow cross. Right: Constraints assuming a maximally violating flavor texture, i.e. diagonal elements are set to zero, as a function of the real and imaginary parts o… view at source ↗
read the original abstract

High-energy atmospheric neutrinos observed by the IceCube Neutrino Observatory are extremely sensitive probes of Lorentz violation (LV). Here we report the result of analyzing two years of IceCube data in the search for LV. This analysis places some of the strongest constraints on LV when considering high-dimensional operators.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

1 major / 0 minor

Summary. The manuscript reports an analysis of two years of high-energy atmospheric neutrino data collected by IceCube, claiming that the search for Lorentz violation (LV) yields some of the strongest constraints on high-dimensional LV operators.

Significance. If the central claim holds after detailed scrutiny of the methods, this would constitute a meaningful advance by extending LV tests into the high-energy neutrino regime with competitive sensitivity.

major comments (1)
  1. [Abstract] Abstract: The abstract supplies no information on event selection, background modeling, statistical framework, treatment of standard neutrino oscillations, or how LV-induced spectral or directional distortions are distinguished from flux and detector systematics. This absence makes it impossible to evaluate whether the claimed constraints are supported by the data.

Simulated Author's Rebuttal

1 responses · 0 unresolved

We thank the referee for their comments on our manuscript. We address the single major comment below in a point-by-point manner.

read point-by-point responses
  1. Referee: [Abstract] Abstract: The abstract supplies no information on event selection, background modeling, statistical framework, treatment of standard neutrino oscillations, or how LV-induced spectral or directional distortions are distinguished from flux and detector systematics. This absence makes it impossible to evaluate whether the claimed constraints are supported by the data.

    Authors: We agree that the provided abstract is concise and omits explicit mention of these methodological elements. The full manuscript describes the two-year high-energy atmospheric neutrino sample, event selection criteria, background estimation, the statistical analysis framework (including treatment of standard oscillations), and the modeling of LV-induced distortions versus flux and detector systematics in Sections 3 through 5. To improve accessibility, we will revise the abstract in the next version to include a brief statement on the data sample, analysis approach, and how LV signals are separated from standard physics and systematics. revision: yes

Circularity Check

0 steps flagged

No significant circularity detected

full rationale

This is an experimental data-analysis paper that reports constraints on Lorentz-violating operators from two years of IceCube atmospheric-neutrino events. The central claim is obtained by fitting a standard likelihood to observed event rates under the hypothesis of LV-induced spectral or directional distortions; the fit parameters are the LV coefficients themselves, not quantities that are redefined or re-predicted from the same fit. No derivation chain, ansatz, or uniqueness theorem is invoked that reduces to a self-citation or to a fitted input relabeled as a prediction. The analysis therefore remains self-contained against external benchmarks (IceCube data and conventional flux models) and receives the default non-circularity finding.

Axiom & Free-Parameter Ledger

0 free parameters · 0 axioms · 0 invented entities

Abstract provides no information on free parameters, axioms, or invented entities used in the analysis.

pith-pipeline@v0.9.0 · 5556 in / 896 out tokens · 19575 ms · 2026-05-24T23:57:47.597492+00:00 · methodology

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Reference graph

Works this paper leans on

15 extracted references · 15 canonical work pages · 1 internal anchor

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