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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

Frank G. Schröder , 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
This is my paper · ORCID
classification astro-ph.HEastro-ph.IM
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.

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Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. The Forward Physics Facility at the HL-LHC and its Synergies with Astroparticle Physics

    astro-ph.HE 2024-12 unverdicted novelty 2.0 of 10

    A proceedings review of the Forward Physics Facility, arguing that its planned far-forward hadron and neutrino measurements would reduce model uncertainties in ultra-high-energy cosmic-ray and neutrino astrophysics.

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