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

Alan Coleman; Andreas Haungs; Dave Seckel; Delia Tosi; Dennis Soldin; Doug Bergman; Francis Halzen; Frank G. Schr\"oder; Frank McNally; Frederic Sarazin

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

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arxiv 1903.07713 v1 pith:OWABNFGO submitted 2019-03-18 astro-ph.HE astro-ph.IM

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

Frank G. Schr\"oder , Tareq AbuZayyad , Luis Anchordoqui , Karen Andeen , Xinhua Bai , Segev BenZvi , Doug Bergman , Alan Coleman

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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

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keywords cosmicgalacticraysair-showerarrayarraysastro2020auger

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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.

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

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