We discuss particle acceleration by strong and weak MHD turbulence in magnetic pressure (low-beta) and gaseous pressure (high-beta) dominated plasmas. We consider the acceleration by large scale compressions in both slow and fast particle diffusion limits. We compare the results with the acceleration rate that arises from resonance scattering and Transit-Time Damping (TTD). We establish that fast modes accelerate particles more efficiently than slow modes. We find that particle acceleration by pitch-angle scattering and TTD dominates acceleration by slow or fast modes when the spatial diffusion rate is small. When the rate of spatial diffusion of particles is high, we establish a substantial enhancement of the efficiency of particle acceler...
We use analytic estimates and numerical simulations of test particles interacting with mag-netohydro...
We use exact orbit integration to investigate particle acceleration in a Gauss field proxy of magnet...
Plasma waves at frequencies well below the gyrofrequency of resonant particles cause particle diffus...
International audienceNonthermal acceleration of particles in magnetohydrodynamic (MHD) turbulence p...
We investigate the interaction between low-frequency magnetohydrodynamic (MHD) turbulence and a dist...
24 pages, 15 figures, published, changes in v2: analytical estimations and numerical measurements re...
Phys. Rev. D, submitted; 22 pages, 11 figures; comments welcomeWe discuss the physics of stochastic ...
In this Letter we analyze the energy distribution evolution of test particles injected in three dime...
International audienceThe efficiency of particle acceleration at shock waves in relativistic, magnet...
International audienceCollisionless, magnetized turbulence offers a promising framework for the gene...
Turbulence is ubiquitous in astrophysics. It radically changes many astrophysical phenomena, in part...
International audienceThis work provides a concrete implementation of E. Fermi's model of particle a...
The effect of compressibility in a charged particle energization by magnetohydrodynamic (MHD) fields...
We perform numerical experiments of test particle acceleration on turbulent magnetic and electric fi...
One of the main features of astrophysical shocks is their ability to accelerate particles to extreme...
We use analytic estimates and numerical simulations of test particles interacting with mag-netohydro...
We use exact orbit integration to investigate particle acceleration in a Gauss field proxy of magnet...
Plasma waves at frequencies well below the gyrofrequency of resonant particles cause particle diffus...
International audienceNonthermal acceleration of particles in magnetohydrodynamic (MHD) turbulence p...
We investigate the interaction between low-frequency magnetohydrodynamic (MHD) turbulence and a dist...
24 pages, 15 figures, published, changes in v2: analytical estimations and numerical measurements re...
Phys. Rev. D, submitted; 22 pages, 11 figures; comments welcomeWe discuss the physics of stochastic ...
In this Letter we analyze the energy distribution evolution of test particles injected in three dime...
International audienceThe efficiency of particle acceleration at shock waves in relativistic, magnet...
International audienceCollisionless, magnetized turbulence offers a promising framework for the gene...
Turbulence is ubiquitous in astrophysics. It radically changes many astrophysical phenomena, in part...
International audienceThis work provides a concrete implementation of E. Fermi's model of particle a...
The effect of compressibility in a charged particle energization by magnetohydrodynamic (MHD) fields...
We perform numerical experiments of test particle acceleration on turbulent magnetic and electric fi...
One of the main features of astrophysical shocks is their ability to accelerate particles to extreme...
We use analytic estimates and numerical simulations of test particles interacting with mag-netohydro...
We use exact orbit integration to investigate particle acceleration in a Gauss field proxy of magnet...
Plasma waves at frequencies well below the gyrofrequency of resonant particles cause particle diffus...