Observation of classically `forbidden' electromagnetic wave propagation and implications for neutrino detection.
- Univ. of California, Irvine, CA (United States)
- Univ. of Kansas, Lawrence, KS (United States); National Research Nuclear Univ., Moscow (Russia)
- Uppsala Univ. (Sweden)
- Whittier College, Whittier, CA (United States)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Univ. of Mainz, Mainz (Germany)
- Univ. of Nebraska, Lincoln, NE (United States)
- Friedrich-Alexander Univ. at Erlangen-Nurnberg, Erlangen (Germany)
- Univ. of Kansas, Lawrence, KS (United States)
- National Taiwan Univ., Taipei (Taiwan)
- Humboldt Univ. of Berlin (Germany); Deutsches Elektronen-Synchrotron (DESY), Hamburg (Germany)
- Univ. of Wisconsin, Madison, WI (United States)
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 describing such shadowing, we report on experimental results that, somewhat unexpectedly, demonstrate the existence of electromagnetic wave transport modes from nominally shadowed regions. Finally, the fact that this shadow-signal propagation is observed both at South Pole and the Ross Ice Shelf in Antarctica suggests that the effect may be a generic property of polar ice, with potentially important implications for experiments seeking to detect neutrinos.
- Research Organization:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC)
- Grant/Contract Number:
- AC02-05CH11231
- OSTI ID:
- 1532333
- Journal Information:
- Journal of Cosmology and Astroparticle Physics, Vol. 2018, Issue 07; ISSN 1475-7516
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
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