Searching for Traces of Planck-Scale Physics with High Energy Neutrinos
Floyd W. Stecker (NASA/UCLA), Sean T. Scully (JMU), Stefano Liberati, (SISSA), and David Mattingly (UNH)

TL;DR
This paper investigates how high energy neutrino observations can test Lorentz invariance violation potentially caused by quantum gravity, analyzing the effects of different operators on neutrino spectra and comparing with IceCube data.
Contribution
It introduces a Monte Carlo framework to model superluminal neutrino propagation with Lorentz violation operators and compares predictions with IceCube observations to constrain Planck-scale physics.
Findings
Potential neutrino flux pileup below 2 PeV if CPT-even operators dominate.
No clear drop-off signature if CPT-odd operators dominate.
Constraints on Lorentz violation parameters from IceCube data.
Abstract
High energy cosmic neutrino observations provide a sensitive test of Lorentz invariance violation, which may be a consequence of quantum gravity theories. We consider a class of non-renormalizable, Lorentz invariance violating operators that arise in an effective field theory description of Lorentz invariance violation in the neutrino sector inspired by Planck-scale physics and quantum gravity models. We assume a conservative generic scenario for the redshift distribution of extragalactic neutrino sources and employ Monte Carlo techniques to describe superluminal neutrino propagation, treating kinematically allowed energy losses of superluminal neutrinos caused by both vacuum pair emission and neutrino splitting. We consider EFTs with both non-renormalizable CPT-odd and non-renormalizable CPT-even operator dominance. We then compare the spectra derived using our Monte Carlo calculations…
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Taxonomy
TopicsNoncommutative and Quantum Gravity Theories · Neutrino Physics Research
