The first-order Fermi acceleration process at an ultra-relativistic shock wave is expected to create a particle spectrum with the unique asymptotic spectral index $\sigma_{\gamma \,\gg\, 1} \approx 2.2$. Below, we discuss this result and differences in its various derivations, which – explicitly or implicitly – always require highly turbulent conditions downstream of the shock. In the presence of medium amplitude turbulence the generated particle spectrum can be much steeper than the above asymptotic one. We also note problems with application of the pitch angle diffusion model for particle transport near the ultra-relativistic shocks
A property common to several different astrophysical sources of high-energy gamma-rays is the presen...
Using an eigenfunction expansion to solve the transport equation,complemented by Monte-Carlo simulat...
The first-order Fermi process at relativistic shocks requires the generation of strong turbulence in...
Diffusive shock acceleration at collisionless shocks remains the most likely process for acceleratin...
We consider the acceleration of charged particles near ultra-relativistic shocks, with Lorentz facto...
4 pages, 2 figures; to appear in ApJ LettersIt is shown that Fermi acceleration at an ultra-relativi...
We consider the acceleration of charged particles near ultrarelativistic shocks, with Lorentz factor...
We consider particle acceleration of the Fermi type at the ultra-relativistic shock bounding an expa...
Gamma-ray data from Fermi-LAT show a bi-lobular structure extending up to 50 degrees above and below...
We report studies on first-order Fermi acceleration in parallel modified shock waves with a large s...
The process of cosmic ray acceleration up to energies in excess of $10^{20}$ eV at relativistic shoc...
The spectral index $s$ of particles diffusively accelerated in a relativistic shock depends on the u...
We determine the spectrum of particles accelerated at shocks with arbitrary speed and arbitrary scat...
Abstract: The question of the origin of ultra-high-energy cosmic rays at relativistic shock waves is...
First-order Fermi acceleration processes at ultrarelativistic shocks are studied with Monte Carlo si...
A property common to several different astrophysical sources of high-energy gamma-rays is the presen...
Using an eigenfunction expansion to solve the transport equation,complemented by Monte-Carlo simulat...
The first-order Fermi process at relativistic shocks requires the generation of strong turbulence in...
Diffusive shock acceleration at collisionless shocks remains the most likely process for acceleratin...
We consider the acceleration of charged particles near ultra-relativistic shocks, with Lorentz facto...
4 pages, 2 figures; to appear in ApJ LettersIt is shown that Fermi acceleration at an ultra-relativi...
We consider the acceleration of charged particles near ultrarelativistic shocks, with Lorentz factor...
We consider particle acceleration of the Fermi type at the ultra-relativistic shock bounding an expa...
Gamma-ray data from Fermi-LAT show a bi-lobular structure extending up to 50 degrees above and below...
We report studies on first-order Fermi acceleration in parallel modified shock waves with a large s...
The process of cosmic ray acceleration up to energies in excess of $10^{20}$ eV at relativistic shoc...
The spectral index $s$ of particles diffusively accelerated in a relativistic shock depends on the u...
We determine the spectrum of particles accelerated at shocks with arbitrary speed and arbitrary scat...
Abstract: The question of the origin of ultra-high-energy cosmic rays at relativistic shock waves is...
First-order Fermi acceleration processes at ultrarelativistic shocks are studied with Monte Carlo si...
A property common to several different astrophysical sources of high-energy gamma-rays is the presen...
Using an eigenfunction expansion to solve the transport equation,complemented by Monte-Carlo simulat...
The first-order Fermi process at relativistic shocks requires the generation of strong turbulence in...