Roberto Aloisio
country of citizenship: Italy
occupation: astrophysicist
Articles 54
-
Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants
-
The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) observatory
-
Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre
-
Indirect dark matter searches at ultrahigh energy neutrino detectors
-
Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation
-
Monte Carlo studies for the optimisation of the Cherenkov Telescope Array layout
-
Origin of the Cosmic Ray Galactic Halo Driven by Advected Turbulence and Self-Generated Waves
-
Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7−3946
-
SimProp v2r4: Monte Carlo simulation code for UHECR propagation
-
XIPE: the x-ray imaging polarimetry explorer
-
Future prospects of testing Lorentz invariance with UHECRs
-
Nonlinear cosmic ray Galactic transport in the light of AMS-02 and Voyager data
-
Cosmogenic neutrinos and ultra-high energy cosmic ray models
-
Propagation of Ultra High Energy Cosmic Rays and the Production of Cosmogenic Neutrinos
-
Super Heavy Dark Matter in light of BICEP2, Planck and Ultra High Energy Cosmic Rays Observations
-
Ultra high energy cosmic rays: implications of Auger data for source spectra and chemical composition
-
XIPE: the X-ray imaging polarimetry explorer
-
Propagation of galactic cosmic rays in the presence of self-generated turbulence
-
Analytic calculations of the spectra of ultra-high energy cosmic ray nuclei. I. The case of CMB radiation
-
Analytic calculations of the spectra of ultra high energy cosmic ray nuclei. II. The general case of background radiation
-
SimProp: a simulation code for ultra high energy cosmic ray propagation
-
Transition from galactic to extragalactic cosmic rays
-
Ultra High Energy Cosmic Rays: Anisotropies and spectrum
-
Ultra high energy cosmic rays: The disappointing model
-
The problem of superluminal diffusion of relativistic particles and its phenomenological solution
-
Signatures of the transition from galactic to extragalactic cosmic rays
-
PHENOMENOLOGY OF SPACE TIME FLUCTUATIONS
-
Deformed special relativity as an effective theory of measurements on quantum gravitational backgrounds
-
Modified special relativity on a fluctuating spacetime
-
Status of superheavy dark matter
-
A note on DSR-like approach to space–time
-
Approaching space-time through velocity in doubly special relativity
Human - wd:Q58316535