Simulation Study of the Observed Radio Emission of Air Showers by the IceTop Surface Extension
Alan Coleman (for the IceCube Collaboration)

TL;DR
This study evaluates the potential of an upgraded IceTop surface array with radio antennas and scintillators for improved cosmic-ray air shower detection, using prototype measurements and simulations to enhance primary particle characterization.
Contribution
It introduces a novel hybrid detection approach combining radio and scintillator measurements with existing IceTop tanks, validated through prototype data and simulations.
Findings
Radio signals observed in the 70-350 MHz band match simulations.
Prototype measurements confirm the analysis chain's validity.
Enhanced array improves primary particle characterization capabilities.
Abstract
Multi-detector observations of individual air showers are critical to make significant progress to precisely determine cosmic-ray quantities such as mass and energy of individual events and thus bring us a step forward in answering the open questions in cosmic-ray physics. An enhancement of IceTop, the surface array of the IceCube Neutrino Observatory, is currently underway and includes adding antennas and scintillators to the existing array of ice-Cherenkov tanks. The radio component will improve the characterization of the primary particles by providing an estimation of X and a direct sampling of the electromagnetic cascade, both important for per-event mass classification. A prototype station has been operated at the South Pole and has observed showers, simultaneously, with the tanks, scintillator panels, and antennas. The observed radio signals of these events are…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Neutrino Physics Research · Dark Matter and Cosmic Phenomena
