From 3K to 10²⁰eV

1998/12/24 by Luis A. Anchordoqui, Anchordoqui, Luis A.
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/9812445

PhD Thesis (summary)

arxiv created 1998/12/24 · arxiv updated 2009/12/01

Abstract

The problem of predicting the upper cut-off of the cosmic ray spectrum is re-examined. Some aspects of extremely high energy interactions and their implications for the interpretation of giant air showers are also discussed.

Related

• Cosmic Ray Energy Spectrum from Measurements of Air Showers
• The energy spectrum of ultraheavy nuclei above 10²⁰ eV
• Deficit of Ultrahigh Energy Extensive Air Showers
• Heavy Ions Interpretation of Highest Energy Cosmic Rays
• The possible feature of the energy spectrum of the primary cosmic rays at ultra-high energies