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

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 T...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	arXiv.org 2019-03
Hauptverfasser:	Schröder, Frank G, AbuZayyad, Tareq, Anchordoqui, Luis, Andeen, Karen, Bai, Xinhua, Segev BenZvi, Bergman, Doug, Coleman, Alan, Dembinski, Hans, DuVernois, Michael, Gaisser, Tom, Halzen, Francis, Haungs, Andreas, Kelley, John, Kolanoski, Hermann, McNally, Frank, Roth, Markus, Sarazin, Frederic, Seckel, Dave, Smida, Radomir, Soldin, Dennis, Tosi, Delia
Format:	Artikel
Sprache:	eng
Schlagworte:	Augers Cosmic ray showers Cosmic rays Galactic cosmic rays High energy astronomy Surface detectors
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Beschreibung
Zusammenfassung:	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.
ISSN:	2331-8422