International audienceAbstract We present a self-consistent Monte Carlo model of particle acceleration by relativistic shock waves. The model includes the magnetic field amplification in the shock upstream by cosmic ray driven plasma instabilities. The parameters of the Monte Carlo model are obtained based on PIC calculations. We present the spectra of accelerated particles simulated in the frame of the model
Context. The diffusive shock acceleration mechanism has been widely accepted as the acceleration mec...
International audienceWe review the physics of relativistic shocks, which are often invoked as the s...
International audienceUsing our new 3-D relativistic particle-in-cell (PIC) code parallelized with M...
International audienceAbstract We present a self-consistent Monte Carlo model of particle accelerati...
This paper presents a new method of Monte-Carlo simulations of test particle Fermi acceleration at r...
Monte Carlo techniques are used to model nonlinear particle acceleration in parallel collisionless s...
In this paper I present Monte Carlo results for shock acceleration at an ultrarelativistic shock for...
52 pages, published in Space Science Review, "Jets and Winds in Pulsar Wind Nebulae, Gamma-ray Burst...
Context. Solar energetic particles observed in association with coronal mass ejections (CMEs) are pr...
Monte Carlo computations for highly relativistic parallel shock particle acceleration are presented ...
Obtaining good statistics for accelerated particle spectra, angular distributions and time distribut...
We simulate time-dependent particle acceleration in the blast wave of a young supernova remnant (SNR...
We have used Monte Carlo simulations to study the properties of parti-cle acceleration in relativist...
Abstract: The question of the origin of ultra-high-energy cosmic rays at relativistic shock waves is...
Recent PIC simulations using injected relativistic electron-ion (electro-positron) jets into ambient...
Context. The diffusive shock acceleration mechanism has been widely accepted as the acceleration mec...
International audienceWe review the physics of relativistic shocks, which are often invoked as the s...
International audienceUsing our new 3-D relativistic particle-in-cell (PIC) code parallelized with M...
International audienceAbstract We present a self-consistent Monte Carlo model of particle accelerati...
This paper presents a new method of Monte-Carlo simulations of test particle Fermi acceleration at r...
Monte Carlo techniques are used to model nonlinear particle acceleration in parallel collisionless s...
In this paper I present Monte Carlo results for shock acceleration at an ultrarelativistic shock for...
52 pages, published in Space Science Review, "Jets and Winds in Pulsar Wind Nebulae, Gamma-ray Burst...
Context. Solar energetic particles observed in association with coronal mass ejections (CMEs) are pr...
Monte Carlo computations for highly relativistic parallel shock particle acceleration are presented ...
Obtaining good statistics for accelerated particle spectra, angular distributions and time distribut...
We simulate time-dependent particle acceleration in the blast wave of a young supernova remnant (SNR...
We have used Monte Carlo simulations to study the properties of parti-cle acceleration in relativist...
Abstract: The question of the origin of ultra-high-energy cosmic rays at relativistic shock waves is...
Recent PIC simulations using injected relativistic electron-ion (electro-positron) jets into ambient...
Context. The diffusive shock acceleration mechanism has been widely accepted as the acceleration mec...
International audienceWe review the physics of relativistic shocks, which are often invoked as the s...
International audienceUsing our new 3-D relativistic particle-in-cell (PIC) code parallelized with M...