Simulation of the propagation of CR air shower cores in ice
Simon De Kockere, Krijn D. de Vries, Nick van Eijndhoven

TL;DR
This paper presents detailed simulations of cosmic-ray-induced particle cascades in ice, exploring their radio emission and implications for neutrino detection and calibration in polar ice-based observatories.
Contribution
It introduces the first detailed simulation framework combining CORSIKA and Geant4 for in-ice cosmic-ray cascades and analyzes their radio emission characteristics.
Findings
In-ice cosmic-ray cascades produce signals similar to neutrino interactions.
Radio emission from these cascades can be detected via Askaryan effect.
These events can serve as natural calibration sources for neutrino detectors.
Abstract
Currently new radio detection techniques are being explored to detect astrophysical neutrinos beyond the PeV scale interacting in polar ice. Due to the long attenuation length of radio waves in a medium, it can be expected that such instruments will also be sensitive to the radio emission of cosmic ray air showers. Furthermore, cosmic ray air showers hitting a high-altitude layer of ice will initiate an in-ice particle cascade, also leading to radio emission. We present the first results of detailed simulations of the in-ice continuation of these cosmic-ray-induced particle cascades, using a combination of the CORSIKA Monte Carlo code and the Geant4 simulation toolkit. We give an overview of the general features of such particle cascades and present a parameterization in terms of Xmax of the longitudinal and lateral particle distributions. We discuss the feasibility of observing the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
