by Pierre Cristofari, A. Albert, A. Carramiñana, S. Casanova, B. L. Dingus, M. A. DuVernois, N. Fraija, H. Fleischhack, J. A. Goodman, T. Greenshaw, J. P. Harding, A. Haungs, B. Hona, P. Huentemeyer, V. Joshi, H. Li, K. Malone, J. Martínez-Castro, M. A. Mostafá, C. Rivière, A. C Rovero, T. Sako, A. Sandoval, M. Santander, K. Satalecka, H. Schoorlemmer, A. J. Smith, W. Springer, A. Viana, H. Zhou, and A. Zepeda
Published onMay 31, 2019
Where are the pevatrons?
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Abstract
The search for cosmic particle accelerators capable of reaching the PeV range, PeVatrons, is a crucial science target of the very-high-energy community. Such accelerators are essential in the context of the problem of the origin of Galactic cosmic rays, and in order to understand the mechanisms involved in the production of PeV particles.
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