Prefer a chat interface with context about you and your work?
Compressible turbulence in galaxy clusters: physics and stochastic particle re-acceleration
We attempt to explain the non-thermal emission arising from galaxy clusters as a result of the re-acceleration of electrons by compressible turbulence induced by cluster mergers. In our model intracluster medium (ICM) is represented by a high beta plasma in which turbulent motions are driven at large scales. The corresponding …