activity
20042025
most citedPropagation of galactic cosmic rays in the presence of self-generated turbulence

75 citations · 224 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2025★ 1 cited

Update on testing of air-shower modelling using combined data of the Pierre Auger Observatory and phenomenological consequences

Jakub Vícha

The combined data of Fluorescence and Surface Detectors of the Pierre Auger Observatory has recently provided the strongest constraints on the validity of predictions from current…

astro-ph.IM2019★ 72 cited

Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout

A. Acharyya, I. Agudo, E. O. Angüner +467

The Cherenkov Telescope Array (CTA) is the major next-generation observatory for ground-based very-high-energy gamma-ray astronomy. It will improve the sensitivity of current groun…

astro-ph.HE2015★ 59 cited

Cosmogenic neutrinos and ultra-high energy cosmic ray models

R. Aloisio, D. Boncioli, A di Matteo +3

We use an updated version of {\it SimProp}, a Monte Carlo simulation scheme for the propagation of ultra-high energy cosmic rays, to compute cosmogenic neutrino fluxes expected on…

astro-ph.HE2013★ 75 cited

Propagation of galactic cosmic rays in the presence of self-generated turbulence

R. Aloisio, P. Blasi

Cosmic rays propagating in the Galaxy may excite a streaming instability when their motion is super-alfvenic, thereby producing the conditions for their own diffusion. In this pape…

gr-qc2004★ 17 cited

Approaching Space Time Through Velocity in Doubly Special Relativity

R. Aloisio, A. Galante, A. F. Grillo +2

We discuss the definition of velocity as dE/dp, where E,p are the energy and momentum of a particle, in Doubly Special Relativity (DSR). If this definition matches dx/dt appropriat…