Observation of classically `forbidden' electromagnetic wave propagation and implications for neutrino detection
S. W. Barwick, E. C. Berg, D. Z. Besson, G. Gaswint, C. Glaser, A., Hallgren, J. C. Hanson, S. R. Klein, S. Kleinfelder, L. K\"opke, I., Kravchenko, R. Lahmann, U. Latif, J. Nam, A. Nelles, C. Persichilli, P., Sandstrom, J. Tatar, E. Unger

TL;DR
This paper reports the unexpected observation of electromagnetic wave propagation in regions previously thought to be shadowed in Antarctic ice, which could significantly impact neutrino detection experiments.
Contribution
It demonstrates experimentally that electromagnetic waves can propagate through forbidden zones in ice, challenging existing models of radio wave propagation in neutrino detection.
Findings
Electromagnetic waves can travel in shadowed regions of ice.
Shadow-signal propagation observed at South Pole and Ross Ice Shelf.
Implications for improving neutrino detection sensitivity.
Abstract
Ongoing experimental efforts in Antarctica seek to detect ultra-high energy neutrinos by measurement of radio-frequency (RF) Askaryan radiation generated by the collision of a neutrino with an ice molecule. An array of RF antennas, deployed either in-ice or in-air, is used to infer the properties of the neutrino. To evaluate their experimental sensitivity, such experiments require a refractive index model for ray tracing radio-wave trajectories from a putative in-ice neutrino interaction point to the receiving antennas; this gives the degree of signal absorption or ray bending from source to receiver. The gradient in the density profile over the upper 200 meters of Antarctic ice, coupled with Fermat's least-time principle, implies ray "bending" and the existence of "forbidden" zones for predominantly horizontal signal propagation at shallow depths. After re-deriving the formulas…
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