A new analytic Askaryan model including ice propagation and RF response matches Monte Carlo simulations with correlations above 0.94 and rejects thermal noise at very low rates.
Time Domain Response of the ARIANNA Detector
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abstract
The Antarctic Ross Ice Shelf Antenna Neutrino Array (ARIANNA) is a high-energy neutrino detector designed to record the Askaryan electric field signature of cosmogenic neutrino interactions in ice. To understand the inherent radio-frequency (RF) neutrino signature, the time-domain response of the ARIANNA RF receiver must be measured. ARIANNA uses Create CLP5130-2N log-periodic dipole arrays (LPDAs). The associated effective height operator converts incident electric fields to voltage waveforms at the LDPA terminals. The effective height versus time and incident angle was measured, along with the associated response of the ARIANNA RF amplifier. The results are verified by correlating to field measurements in air and ice, using oscilloscopes. Finally, theoretical models for the Askaryan electric field are combined with the detector response to predict the neutrino signature.
fields
astro-ph.HE 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
An analytical model of Askaryan radiation plus detector response is shown to match 13 ARA UHECR candidate waveforms with correlations 0.69-0.86.
citing papers explorer
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Complex Analysis of Askaryan Radiation: UHE-$\nu$ Identification and Reconstruction using the Hilbert Envelope of Observed Signals
A new analytic Askaryan model including ice propagation and RF response matches Monte Carlo simulations with correlations above 0.94 and rejects thermal noise at very low rates.
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Complex Analysis of Askaryan Radiation: UHECR Reconstruction with Askaryan Radio Array
An analytical model of Askaryan radiation plus detector response is shown to match 13 ARA UHECR candidate waveforms with correlations 0.69-0.86.