Neutrino oscillations as a novel probe for a minimal length

TL;DR

This paper proposes using neutrino oscillation measurements to detect effects of a minimal length scale predicted by quantum gravity, highlighting potential observable deviations at high energies.

Contribution

It introduces a modified neutrino survival probability model incorporating a minimal length and discusses its implications for current and future neutrino experiments.

Findings

Current data bounds minimal length scale to 0 GeV.

High-energy neutrino oscillations are suppressed by minimal length effects.

Potential for observing quantum gravity effects with neutrino telescopes.

Abstract

We suggest that the presence of a quantum gravity induced minimal length can be explored using neutrino oscillation probabilities. Neutrinos seem ideally suited for this investigation because they can propagate freely over large distances and can therefore pile up minimal length effects beyond detectable thresholds. We determine the modified survival probability in a scenario with a minimal length and find deviations from the classical behaviour for high energies. We find that for the currently available experimental statistics the deviations from the standard oscillations do only allow for a bound of $\ell^{-1}\gtrsim 10 \mathrm{GeV}$ from MINOS data. On the other hand, oscillations of high-energy neutrinos emitted by galactic and extragalactic sources are strongly suppressed, leading to a possible observation of quantum gravity effects at neutrino telescopes such as IceCube and ANTARES.