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Complex analysis of Askaryan radiation: Ultrahigh energy cosmic-ray reconstruction

Jordan C. Hanson* and Damian Ibáñez-Rodriguéz

  • Department of Physics and Astronomy, Whittier College, Whittier, California, USA

  • *Contact author: jhanson2@whittier.edu
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Phys. Rev. D 114, 043046 – Published 18 August, 2026

DOI: https://doi.org/10.1103/l1vl-j7mk

Abstract

Ultrahigh energy cosmic rays (UHECR) can produce relativistic cascades that emit radio-frequency (RF) pulses in the 0.1–1 GHz bandwidth via two distinct effects: the geomagnetic effect, and the Askaryan effect. The geomagnetic effect occurs when the magnetic field of the Earth causes cascade charges to form a transverse current that radiates linearly polarized radiation aligned with the Lorentz force direction. The Askaryan effect is caused by the net negative charge excess in the cascade that radiates linearly polarized radiation along the Cherenkov cone. When UHECR cascades enter solid, RF transparent matter at altitudes where the cascade develops, Askaryan radiation created in the solid medium can propagate to RF detectors. The Askaryan Radio Array (ARA) at the South Pole has observed 13 UHECR candidates in precisely this fashion. We present an analytical model that confirms the events are UHECRs. The model includes Askaryan radiation created within the ice sheet and the ARA RF channel response. The coherently summed waveforms (CSWs) from the UHECR candidates match our model with correlation coefficients between 0.69 and 0.86, and with minimal fractional power differences. Finally, we demonstrate how to obtain the Askaryan E→-field from our model, and that it matches the results from the ARA collaboration.

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Phys. Rev. D 114, 043046– Published 18 August, 2026
  • Received 27 March 2026
  • Accepted 15 July 2026
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