Galaxy clusters are the largest objects in the Universe kept together by gravity. Most of their
baryonic content is made of a magnetized diffuse plasma. We investigate the impact of such …

Interactions of ultra-high-energy cosmic rays (UHECRs) in the surroundings of their
accelerators can naturally explain the observed spectrum and composition of UHECRs …

We predict the arrival distribution of ultra–high-energy cosmic rays (UHECRs) above 4× 10
19 eV with the event number expected by future experiments in the next few years. We …

Ultrahigh-energy cosmic rays (UHECRs) are known to come from outside of our Galaxy, but
their origin still remains unknown. The Telescope Array (TA) experiment recently identified a …

We study the propagation of ultra-high-energy cosmic rays (UHECRs) with E> 10 18 eV in
the Galactic magnetic field (GMF). We present numerical simulations for the propagation of …

The quest for the origin (s) of ultra-high-energy cosmic rays (UHECRs) continues to be a far-
reaching pillar of high energy astrophysics. The source scrutiny is mostly based on three …

We present a new method for calculating arrival distribution of ultra–high-energy cosmic
rays (UHECRs), including modifications by the Galactic magnetic field. We perform …

We study how the properties of transient sources of ultra-high-energy cosmic rays
(UHECRs) can be accessed by exploiting UHECR experiments, taking into account the …

We estimate the local number density of sources of ultra-high-energy cosmic rays (UHECRs)
based on the statistical features of their arrival direction distribution. We calculate the arrival …

We investigate the possibility that observations of ultra-high-energy cosmic rays (UHECRs)
in the near future may be able to unveil their local source distribution, which will reflect …