U. Latif

TL;DR: In this paper, the authors present an overview of a next-generation instrument, IceCube-Gen2, which will sharpen our understanding of the processes and environments that govern the universe at the highest energies.

TL;DR: In this article, the authors present an overview of a next-generation instrument, IceCube-Gen2, which will sharpen our understanding of the processes and environments that govern the Universe at the highest energies.

TL;DR: The ARIANNA project as discussed by the authors uses a surface array of independent radio detector stations in Antarctica for the detection of ultra-high energy neutrinos (UHE) with the potential to reveal the sources of UHE cosmic rays especially if combined with observations in the electromagnetic spectrum and gravitational waves.

TL;DR: The NuPhase detector as mentioned in this paper was installed at an Askaryan Radio Array (ARA) station during the 2017/18 Austral summer season and achieved a trigger threshold of 1.6 for neutrino interactions that are in the far field of the array.

TL;DR: NuRadioMC as discussed by the authors is a Monte Carlo framework designed to simulate ultra-high energy neutrino detectors that rely on the radio detection method, which exploits the radio emission generated in the electromagnetic component of a particle shower following a Neutrino interaction.