The Surface Array of IceCube-Gen2

Abstract

The science goals of IceCube-Gen2 include multi-messenger astronomy, astroparticle and particle physics. To this end, the observatory will include several detection methods including a surface array and in-ice optical sensors. The array will have an approximately 8 km 2 surface coverage consisting of elevated scintillator panels and radio antennas to detect air showers in the energy range of several 100 TeV to a few EeV. The observatory's design is unique in that the measurements using the surface array can be combined with the observations of ≥ 300 GeV muons, produced in the hadronic cascades, using the optical detectors in the ice. This allows for an enhanced ability to study cosmic-ray and hadronic physics as well as to boost the sensitivity for astrophysical neutrinos from the southern sky by reducing the primary background, atmospheric muons. We will present the baseline design of the surface array and highlight the expected scientific capabilities.

Snowmass UHECR Whitepaper: Requirements on Future Instrumentation

“…For the next generation, IceCube-Gen2 will have a unique role beyond its main purpose as neutrino observatory [36]. For cosmic rays in the energy range up to a few EeV, it will be the only experiment that combines a deep optical detector for TeV muons with a multi-detector surface array, providing hybrid detection of air-showers with elevated scintillators and radio antennas.…”