activity
20012010
most citedOn astrophysical solution to ultra high energy cosmic rays

492 citations · 976 across the 8 of their papers we have counts for

collaborators

8 papers

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-ph2008★ 55 cited

Analytic calculations of the spectra of ultra-high energy cosmic ray nuclei. I. The case of CMB radiation

R. Aloisio, V. Berezinsky, S. Grigorieva

We present a systematic study of different methods for the analytic calculation of ultra-high energy nuclei diffuse spectra. Nuclei propagating in the intergalactic space are photo…

astro-ph2007★ 3 cited

On the status of the dip in UHECR spectrum

V. Berezinsky, A. Gazizov, S. Grigorieva

The status of the pair-production dip as a spectral feature, produced by interaction of Ultra High Energy extragalactic protons with CMB is discussed.

astro-ph2006★ 152 cited

A dip in the UHECR spectrum and the transition from galactic to extragalactic cosmic rays

R. Aloisio, V. Berezinsky, P. Blasi +3

The dip is a feature in the diffuse spectrum of ultra-high energy (UHE) protons caused by electron-positron pair production on the cosmic microwave background (CMB) radiation. For…

astro-ph2005★ 199 cited

Dip in UHECR spectrum as signature of proton interaction with CMB

V. Berezinsky, A. Z. Gazizov, S. I. Grigorieva

Ultrahigh energy (UHE) extragalactic protons propagating through cosmic microwave radiation (CMB) acquire the spectrum features in the form of the dip, bump (pile-up protons) and t…

astro-ph2004★ 26 cited

Propagation and Signatures of Ultra High Energy Cosmic Rays

V. Berezinsky, A. Gazizov, S. Grigorieva

We study the extragalactic protons with universal spectrum, which is independent of mode of propagation, when distance between sources is less than the propagation lengths, such as…