Advancing QCD toward astroparticle applications generates new challenges for perturbation theory, such as the presence of large evolution scales with sizeable scaling violations involving both the initial and the final state of a collision. Possible applications in the context of Ultra High Energy Cosmic Rays (UHECR) of these effects are discussed
AbstractThe pseudorapidity measurements at LHC, although in the central region only, allows us to pe...
We review the physics of the highest energy cosmic rays, i.e. those astrophysical particles with ene...
We present a brief introduction to the physics of Ultra High Energy Cosmic Rays (UHECRs), concentrat...
Recently, models proposing superheavy particles $X$ as source of ultrahigh energy cosmic rays have a...
The supersymmetric evolution of the fragmentation functions (or timelike evolution) within N=1 $QCD$...
It has not yet been elucidated whether the observed flux suppression for ultra-high energy cosmic ra...
Contribution à la conférence ICFP 2012, International Conference on New Frontiers in Physics, Kolymb...
Cosmic rays may provide opportunities for probing fundamental physics. For example, ultrahigh-energy...
With the present understanding of data, the observed flux suppression for ultra-high energy cosmic r...
While several arguments can be proposed against the existence of particles with energy in excess of ...
The most energetic particles ever detected exceed $10^{20}$ eV in energy. Their existence represents...
The pseudorapidity measurements at LHC, although in the central region only, allows us to perform pr...
Measurements of proton and nuclear collisions at the Large Hadron Collider at nucleon-nucleon c.m. e...
In this work we present a detailed computation of the spectra of UHECR in the top-down scenario. We ...
The differences between contemporary Monte Carlo generators of high energy hadronic interactions are...
AbstractThe pseudorapidity measurements at LHC, although in the central region only, allows us to pe...
We review the physics of the highest energy cosmic rays, i.e. those astrophysical particles with ene...
We present a brief introduction to the physics of Ultra High Energy Cosmic Rays (UHECRs), concentrat...
Recently, models proposing superheavy particles $X$ as source of ultrahigh energy cosmic rays have a...
The supersymmetric evolution of the fragmentation functions (or timelike evolution) within N=1 $QCD$...
It has not yet been elucidated whether the observed flux suppression for ultra-high energy cosmic ra...
Contribution à la conférence ICFP 2012, International Conference on New Frontiers in Physics, Kolymb...
Cosmic rays may provide opportunities for probing fundamental physics. For example, ultrahigh-energy...
With the present understanding of data, the observed flux suppression for ultra-high energy cosmic r...
While several arguments can be proposed against the existence of particles with energy in excess of ...
The most energetic particles ever detected exceed $10^{20}$ eV in energy. Their existence represents...
The pseudorapidity measurements at LHC, although in the central region only, allows us to perform pr...
Measurements of proton and nuclear collisions at the Large Hadron Collider at nucleon-nucleon c.m. e...
In this work we present a detailed computation of the spectra of UHECR in the top-down scenario. We ...
The differences between contemporary Monte Carlo generators of high energy hadronic interactions are...
AbstractThe pseudorapidity measurements at LHC, although in the central region only, allows us to pe...
We review the physics of the highest energy cosmic rays, i.e. those astrophysical particles with ene...
We present a brief introduction to the physics of Ultra High Energy Cosmic Rays (UHECRs), concentrat...