Cosmic rays: the spectrum and chemical composition from 1010 to 1020 eV

The production of energetic particles in the universe remains one of the great mysteries of modern science. The mechanisms of acceleration in astrophysical sources and the details about the propagation through the galactic and extragalactic media are still to be defined. In recent years, the cosmic ray flux has been measured with high precision in the energy range from 10(10) to 10(20.5) eV by several experiments using different techniques. In some energy ranges, it has been possible to determine the flux of individual elements (hydrogen to iron nuclei). This paper explores an astrophysical scenario in which only our Galaxy and the radio galaxy Cen A produce all particles measured on Earth in the energy range from 10(10) to 10(20.5) eV. Data from AMS-02, CREAM, KASCADE, KASCADE-Grande and thePierre Auger Observatories are considered. The model developed here is compared to the total and if available to the individual particle flux of the experiments considered. The flux of each element as determined by AMS-02, CREAM, KASCADE and KASCADE-Grande and the mass sensitivity parameter X-max measured by the Pierre Auger Observatory above 10 eV are also explored within the framework of the model. The transition from 1016 to 1018 eV is carefully analyzed. It is shown that the flux measured in this energy range suggest the existence of an extra component of cosmic rays yet to be understood.