We report studies on first-order Fermi acceleration in parallel modified shock waves with a large scattering center compression ratio expected from turbulence transmission models. Using a Monte Carlo technique we have modeled particle acceleration in shocks with a velocity ranging from nonrelativistic to ultrarelativistic and a thickness extending from nearly steplike to very wide structures exceeding the particle diffusion length by orders of magnitude. The nonrelativistic diffusion approximation is found to be surprisingly accurate in predicting the spectral index of a thick shock with large compression ratio even in the cases involving relativistic shock speeds
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
We consider the acceleration of charged particles near ultrarelativistic shocks, with Lorentz factor...
We report studies on first-order Fermi acceleration in parallel modified shock waves with a large s...
Shocks in relativistic jets are regions where cosmic ray acceleration takes place mainly via two kin...
First-order Fermi acceleration processes at ultrarelativistic shocks are studied with Monte Carlo si...
Monte Carlo computations for highly relativistic parallel shock particle acceleration are presented ...
Abstract: The question of the origin of ultra-high-energy cosmic rays at relativistic shock waves is...
We apply a semi-classical approach of handling waves as quasiparticle gas in a slowly varying flow ...
Using an eigenfunction expansion to solve the transport equation,complemented by Monte-Carlo simulat...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
We consider the acceleration of charged particles near ultrarelativistic shocks, with Lorentz factor...
We report studies on first-order Fermi acceleration in parallel modified shock waves with a large s...
Shocks in relativistic jets are regions where cosmic ray acceleration takes place mainly via two kin...
First-order Fermi acceleration processes at ultrarelativistic shocks are studied with Monte Carlo si...
Monte Carlo computations for highly relativistic parallel shock particle acceleration are presented ...
Abstract: The question of the origin of ultra-high-energy cosmic rays at relativistic shock waves is...
We apply a semi-classical approach of handling waves as quasiparticle gas in a slowly varying flow ...
Using an eigenfunction expansion to solve the transport equation,complemented by Monte-Carlo simulat...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
11 pages; 10 figures; submitted to MNRASThis paper presents numerical simulations of test particle F...
We consider the acceleration of charged particles near ultrarelativistic shocks, with Lorentz factor...