Third road to the OPERA: a tunnel after all?
Giovanni Amelino-Camelia

TL;DR
This paper explores the possibility that the OPERA neutrino anomaly may be due to known physical effects related to tunneling and evanescence, rather than new physics, and proposes experimental tests and theoretical models for these effects.
Contribution
It introduces a hypothesis that the OPERA result could be explained by known effects like tunneling time and postselection, offering a semi-heuristic formula and testable predictions.
Findings
The OPERA neutrino early arrival could be explained by tunneling-related effects.
A semi-heuristic formula for rock dwell time aligns with OPERA measurements.
Effects similar to OPERA's could occur with anti-neutrinos and are relevant at Planck scale.
Abstract
The debate on OPERA focused on two extremes: either "OPERA is wrong" or our formulation of the laws of physics needs a major overhaul. I here argue that some effort should be directed toward manifestations of laws that are already known, but whose implications are poorly understood in OPERA-type contexts. My preferred example of this sort is that the OPERA result might be the first observation of a previously unnoticed effect, belonging to a family of effects which includes those responsible for the well-known peculiar properties of the "tunneling time". Tentative support for this specific hypothesis comes from the presence of evanescence and "postselection", and the observation that the fraction of neutrinos absorbed in rock on the way from CERN to LNGS is of a few parts in , i.e. comparable to the fraction of the overall travel time by which OPERA neutrinos are found to reach…
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Dark Matter and Cosmic Phenomena · Particle Detector Development and Performance
