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Report of the Topical Group on Cosmic Probes of Fundamental Physics for for Snowmass 2021
Rana X. Adhikari, Luis A. Anchordoqui, Ke Fang +118
Cosmic Probes of Fundamental Physics take two primary forms: Very high energy particles (cosmic rays, neutrinos, and gamma rays) and gravitational waves. Already today, these probe…
Neutrino propagation in the Earth and emerging charged leptons with
Diksha Garg, Sameer Patel, Mary Hall Reno +22
Ultra-high-energy neutrinos serve as messengers of some of the highest energy astrophysical environments. Given that neutrinos are neutral and only interact via weak interactions,…
EUSO-SPB2: A sub-orbital cosmic ray and neutrino multi-messenger pathfinder observatory
A. Cummings, J. Eser, G. Filippatos +3
The next generation of ultra-high energy cosmic ray (UHECR) and very-high energy neutrino observatories will address the challenge of the extremely low fluxes of these particles at…
The All-sky Medium Energy Gamma-ray Observatory eXplorer (AMEGO-X) Mission Concept
Regina Caputo, Marco Ajello, Carolyn Kierans +52
The All-sky Medium Energy Gamma-ray Observatory eXplorer (AMEGO-X) is designed to identify and characterize gamma rays from extreme explosions and accelerators. The main science th…
EAS optical Cherenkov signatures of tau neutrinos for space and suborbital detectors
Mary Hall Reno, Tonia M. Venters, John F. Krizmanic
Multi-messenger observations of transient astrophysical sources have the potential to characterize the highest energy accelerators and the most extreme environments in the Universe…
Neutrino Target-of-Opportunity Observations with Space-based and Suborbital Optical Cherenkov Detectors
Tonia M. Venters, Mary Hall Reno, John F. Krizmanic
Cosmic-ray accelerators capable of reaching ultra-high energies are expected to also produce very-high energy neutrinos via hadronic interactions within the source or its surroundi…