Constraints on the interpretation of the superluminal motion of neutrinos at OPERA
Walter Winter

TL;DR
This paper analyzes the OPERA neutrino experiment's superluminal results, demonstrating that the waveform's nonlinear structure constrains the fraction of neutrinos that can be superluminal, challenging certain hypotheses and limiting systematic errors.
Contribution
It provides quantitative constraints on the fraction of superluminal neutrinos based on waveform analysis, challenging sterile neutrino explanations and systematic error assumptions.
Findings
At least 17% of neutrinos must be superluminal at 3 sigma
The superluminal velocity is constrained to (v-c)/c = 4.5×10^{-5}
Waveform shape limits the possible systematic errors
Abstract
Various approaches aim to describe the recent analysis by the OPERA experiment, which indicates that neutrinos travel faster than the speed of light. We demonstrate that any such theoretical or experimental explanation must not destroy the complicated (nonlinear) structure of the proton waveform recovered in the neutrino signal. As one example, consider that only a fraction of the neutrinos travel faster than the speed of light, such as sterile neutrinos. We fit the OPERA data including this fraction as a free variable, assuming that the OPERA result is correct. In our analysis, the best-fit values are 50% of the neutrinos being superluminal and (v-c)/c = 4.5 10^{-5}, where the neutrino velocity increases as the fraction of superluminal neutrinos decreases. The minimal fraction of superluminal neutrinos is found to be 17% (3 sigma), which is constrained by the non-linearity of the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
