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A Window on the Ultra-High Energy Universe

Published online by Cambridge University Press:  30 March 2016

Pasquale Blasi*
Affiliation:
INAF/Osservatorio Astrofisico di ArcetriLargo E. Fermi, 5 – 150125 Firenze, Italy

Abstract

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Cosmic rays with energy around and in excess of 1020 eV have been detected. Despite the uncertainties associated with the difficult measurements of extremely low fluxes (about a particle per square kilometer per century) the same existence of such high energy cosmic rays raises important questions that deserve an appropriate answer. I briefly summarize here what are these questions and how to look for the answers.

Type
I. Joint Discussions
Copyright
Copyright © Astronomical Society of Pacific 2005

References

Ave, M., Hinton, J.A., Vazquez, R.A., Watson, A.A., Zas, E. 2002, Phys. Rev., D65, 063007 Google Scholar
Bird, D.J., et al 1993, Phys. Rev. Lett., 71, 3401 CrossRefGoogle Scholar
Blasi, P. & De Marco, , Astropart. Phys., in press (preprint astro-ph/0307067)Google Scholar
Blasi, P., Epstein, R.I., & Olinto, A.V. 2000, ApJ Lett., 533, 123 Google Scholar
De Marco, D., Blasi, P., & Olinto, A.V. 2003, Astropart. Phys., 20, 53 Google Scholar
Finley, C.B., & Westerhoff, S. 2003, preprint astro-ph/0309159Google Scholar
Greisen, K. 1966, Phys. Rev. Lett., 16, 748 Google Scholar
Zatsepin, G.T., & and Kuzmin, V.A. 1966, Soc. Phys. JETP Lett., 4, 78 Google Scholar