activity
19942012
most citedUltra High Energy Cosmic Rays: The disappointing model

119 citations · 694 across the 19 of their papers we have counts for

collaborators

19 papers

astro-ph.HE2012★ 88 cited

Transition from galactic to extragalactic cosmic rays

R. Aloisio, V. Berezinsky, A. Gazizov

The study of the transition between galactic and extragalactic cosmic rays can shed more light on the end of the Galactic cosmic rays spectrum and the beginning of the extragalacti…

astro-ph.HE2011★ 15 cited

Disappointing model for ultrahigh-energy cosmic rays

R. Aloisio, V. Berezinsky, A. Gazizov

Data of Pierre Auger Observatory show a proton-dominated chemical composition of ultrahigh-energy cosmic rays spectrum at (1 - 3) EeV and a steadily heavier composition with energy…

astro-ph.CO2010★ 48 cited

Analytic calculations of the spectra of ultra high energy cosmic ray nuclei. II. The general case of background radiation

R. Aloisio, V. Berezinsky, S. Grigorieva

We discuss the problem of ultra high energy nuclei propagation in extragalactic background radiations. The present paper is the continuation of the accompanying paper I where we ha…

astro-ph.GA2010★ 17 cited

Annihilations of superheavy dark matter in superdense clumps

V. Berezinsky, V. Dokuchaev, Yu. Eroshenko +2

Superheavy dark matter (SHDM) exchanges energy with its environment much slower than particles with masses close to the electroweak (EW) scale and has therefore different small-sca…

astro-ph.HE2009★ 119 cited

Ultra High Energy Cosmic Rays: The disappointing model

R. Aloisio, V. Berezinsky, A. Gazizov

We develop a model for explaining the data of Pierre Auger Observatory (Auger) for Ultra High Energy Cosmic Rays (UHECR), in particular, the mass composition being steadily heavier…

astro-ph2008★ 48 cited

Superluminal problem in diffusion of relativistic particles and its phenomenological solution

R. Aloisio, V. Berezinsky, A. Gazizov

We discuss the superluminal problem in the diffusion of ultra high energy protons with energy losses taken into account. The phenomenological solution of this problem is found with…