High-Energy Galactic Cosmic Rays (Astro2020 Science White Paper)

Frank G. Schröder; Tareq AbuZayyad; Luis Anchordoqui; Karen Andeen; Xinhua Bai; Segev BenZvi; Doug Bergman; Alan Coleman; Hans Dembinski; Michael DuVernois; Tom Gaisser; Francis Halzen; Andreas Haungs; John Kelley; Hermann Kolanoski; Frank McNally; Markus Roth; Frederic Sarazin; Dave Seckel; Radomir Smida; Dennis Soldin; Delia Tosi

arXiv · 1903.07713

High-Energy Galactic Cosmic Rays (Astro2020 Science White Paper)

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Abstract

The origin of the highest energy Galactic cosmic rays is still not understood, nor is the transition to EeV extragalactic particles. Scientific progress requires enhancements of existing air-shower arrays, such as: IceCube with its surface detector IceTop, and the low-energy extensions of both the Telescope Array and the Pierre Auger Observatory.

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Frank G. Schröder, Tareq AbuZayyad, Luis Anchordoqui, Karen Andeen, Xinhua Bai, Segev BenZvi, Doug Bergman, Alan Coleman, Hans Dembinski, Michael DuVernois, Tom Gaisser, Francis Halzen, Andreas Haungs, John Kelley, Hermann Kolanoski, Frank McNally, Markus Roth, Frederic Sarazin, Dave Seckel, Radomir Smida, Dennis Soldin, Delia Tosi. 2019-03-18. High-Energy Galactic Cosmic Rays (Astro2020 Science White Paper). https://arxiv.org/abs/1903.07713

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