Abstract: Recent high precision measurements of the Ultra High Energy Cosmic-ray spectrum have been done by the Hires, Pierre Auger and Telescope Array Observatories. The agreement between the published spectra is remarkably good despite the possibility that each experiment is exposed to a different source population. If the highest energetic particles are not all heavy and if the magnetic field strength is not extreme quasi-linear propagation of particles from source to Earth is a reasonable assumption. In this work we evaluate the effect of different source population visible from different latitudes in the measured energy spectra. We simulated the propagation of particles in the Universe given a chosen composition and source distribution...
Abstract: The flux of ultra-high energy (UHE) cosmic rays (CRs) depends on the cosmic distribution o...
The discovery of cosmic rays with ultra-high energies has opened a window to observe the far and unk...
International audienceWe study the propagation of cosmic rays at the highest energies of different c...
Abstract: We have published the energy spectrum of ultra-high energy cosmic rays (UHECRs) for E> ...
The measurement of the energy spectrum of ultra-high-energy cosmic rays (UHECRs) is of crucial impor...
International audienceThe energy spectrum of ultra-high energy cosmic rays (UHECRs) provides essenti...
Abstract: The study of the elemental composition and spectra of cosmic rays will provide very crucia...
Abstract: This work presents comparative analysis of cosmic rays intensity results got at different ...
In this work, ultra-high energy cosmic rays are studied based on ten years of data taken with the Pi...
The energy spectrum of ultra-high energy cosmic rays is the most emblematic observable for describin...
The Pierre Auger Observatory (PAO) and Telescope Array (TA) collaborations report significant differ...
Abstract: We predict the arrival direction distribution of cosmic rays as a function of rapidity und...
Abstract: The hypothesis is considered that the present, local Galactic cosmic ray spectrum is, due ...
Abstract: The discrepancies in the results produced by the two most commonly used Monte Carlo progra...
Abstract: The flux of ultra-high energy (UHE) cosmic rays (CRs) depends on the cosmic distribution o...
The discovery of cosmic rays with ultra-high energies has opened a window to observe the far and unk...
International audienceWe study the propagation of cosmic rays at the highest energies of different c...
Abstract: We have published the energy spectrum of ultra-high energy cosmic rays (UHECRs) for E> ...
The measurement of the energy spectrum of ultra-high-energy cosmic rays (UHECRs) is of crucial impor...
International audienceThe energy spectrum of ultra-high energy cosmic rays (UHECRs) provides essenti...
Abstract: The study of the elemental composition and spectra of cosmic rays will provide very crucia...
Abstract: This work presents comparative analysis of cosmic rays intensity results got at different ...
In this work, ultra-high energy cosmic rays are studied based on ten years of data taken with the Pi...
The energy spectrum of ultra-high energy cosmic rays is the most emblematic observable for describin...
The Pierre Auger Observatory (PAO) and Telescope Array (TA) collaborations report significant differ...
Abstract: We predict the arrival direction distribution of cosmic rays as a function of rapidity und...
Abstract: The hypothesis is considered that the present, local Galactic cosmic ray spectrum is, due ...
Abstract: The discrepancies in the results produced by the two most commonly used Monte Carlo progra...
Abstract: The flux of ultra-high energy (UHE) cosmic rays (CRs) depends on the cosmic distribution o...
The discovery of cosmic rays with ultra-high energies has opened a window to observe the far and unk...
International audienceWe study the propagation of cosmic rays at the highest energies of different c...