Microphysics of weakly magnetized relativistic collisionless shock waves, corroborated by
recent high performance numerical simulations, indicates the presence of a microturbulent …

Collisionless relativistic shocks have been the focus of intense theoretical and numerical
investigations in recent years. The acceleration of particles, the generation of …

ABSTRACT Particle-in-cell (PIC) simulations of relativistic shocks are in principle capable of
predicting the spectra of photons that are radiated incoherently by the accelerated particles …

The study of the Brownian motion of a charged particle in electric and magnetic fields has
many important applications in plasma and heavy ions physics, as well as in astrophysics. In …

We numerically calculate the radiation spectrum from relativistic electrons moving in small-
scale turbulent magnetic fields expected in high-energy astrophysical sources. Such a …

Using a numerical method, we examine the radiation spectra from relativistic electrons
moving in Langmuir turbulence, which are expected to exist in high energy astrophysical …

Relativistic sources, eg gamma-ray bursts, pulsar wind nebulae and powerful active galactic
nuclei produce relativistic outflows that lead to the formation of collisionless shock waves …

We present the results of the first principle numerical calculations for the radiation spectrum
from relativistic electrons moving in a turbulent electromagnetic field and its applications to …

This paper summarizes recent progresses in our theoretical understanding of particle
acceleration at relativistic shock waves and it discusses two salient consequences:(1) the …

We present the results of the first principle numerical calculations for the radiation spectrum
from relativistic electrons moving in a turbulent electromagnetic field and its applications to …