The production of energetic particles is explored for collisionless shocks and magnetic reconnection by using full particle simulations and analytic study, and it is argued that “surfing acceleration ” can provide the quick and strong energiztion than that believed before. Large amplitude and small scale electrostatic field, which is a necessary condition for the strong surfing acceleration, can be easily generated in cosmic plasmas. Therefore, non-adiabatic particles trapped by the potential well of the large amplitude wave are capable of reaching relativistic energies. 1
On the basis of numerical calculations it is considered the highly relativistic surfatron accelerati...
We examine limits to the energy to which cosmic rays can be accelerated by relativistic shocks, show...
We suggest a physical mechanism whereby the acceleration time of cosmic rays (CRs) by shock waves ca...
Often in laboratory, space and astrophysical plasma, high energy populations are observed. Two puzzl...
The acceleration of particles to high energy by relativistic plasma waves has received a great deal ...
International audienceWe discuss a new acceleration or energization mechanism of charged particles i...
The phenomenon of trapping of weakly relativistic charged particles (with kinetic energies on the or...
Magnetic reconnection is thought to be the driver for many explosive phenomena in the universe. The ...
Particle acceleration by means of nonlinear plasma wave interactions is of great topical interest. A...
International audienceWe review the physics of relativistic shocks, which are often invoked as the s...
The maximum energy to which cosmic rays can be accelerated at weakly magnetised ultrarelativistic sh...
When electrons that are trapped by strong electrostatic waves are carried across a magnetic field, t...
Resonant interactions between an electromagnetic wave packet and charged particles based on numerica...
Our numerical simulations show that the reconnection of magnetic field becomes fast in the presence ...
A new particle acceleration process in a developing Alfv´en turbulence in the course of successive p...
On the basis of numerical calculations it is considered the highly relativistic surfatron accelerati...
We examine limits to the energy to which cosmic rays can be accelerated by relativistic shocks, show...
We suggest a physical mechanism whereby the acceleration time of cosmic rays (CRs) by shock waves ca...
Often in laboratory, space and astrophysical plasma, high energy populations are observed. Two puzzl...
The acceleration of particles to high energy by relativistic plasma waves has received a great deal ...
International audienceWe discuss a new acceleration or energization mechanism of charged particles i...
The phenomenon of trapping of weakly relativistic charged particles (with kinetic energies on the or...
Magnetic reconnection is thought to be the driver for many explosive phenomena in the universe. The ...
Particle acceleration by means of nonlinear plasma wave interactions is of great topical interest. A...
International audienceWe review the physics of relativistic shocks, which are often invoked as the s...
The maximum energy to which cosmic rays can be accelerated at weakly magnetised ultrarelativistic sh...
When electrons that are trapped by strong electrostatic waves are carried across a magnetic field, t...
Resonant interactions between an electromagnetic wave packet and charged particles based on numerica...
Our numerical simulations show that the reconnection of magnetic field becomes fast in the presence ...
A new particle acceleration process in a developing Alfv´en turbulence in the course of successive p...
On the basis of numerical calculations it is considered the highly relativistic surfatron accelerati...
We examine limits to the energy to which cosmic rays can be accelerated by relativistic shocks, show...
We suggest a physical mechanism whereby the acceleration time of cosmic rays (CRs) by shock waves ca...