135 citations · 763 across the 41 of their papers we have counts for
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Limits on the ions temperature anisotropy in turbulent intracluster medium
R. Santos-Lima, H. Yan, E. M. de Gouveia Dal Pino +1
Turbulence in the weakly collisional intracluster medium of galaxies (ICM) is able to generate strong thermal velocity anisotropies in the ions (with respect to the local magnetic…
Features of collisionless turbulence in the intracluster medium from simulated Faraday Rotation maps
M. S. Nakwacki, G. Kowal, R. Santos-Lima +2
Observations of the intracluster medium (ICM) in galaxy clusters suggest for the presence of turbulence and the magnetic fields existence has been proved through observations of Fa…
Magnetic field amplification and evolution in turbulent collisionless MHD: an application to the ICM
R. Santos-Lima, E. M. de Gouveia Dal Pino, G. Kowal +3
The amplification and maintenance of the observed magnetic fields in the ICM are usually attributed to the turbulent dynamo action. This is generally derived employing a collisiona…
The role of pressure anisotropy in the turbulent intracluster medium
M. S. Nakwacki, E. M. de Gouveia Dal Pino, G. Kowal +1
In low-density plasma environments, such as the intracluster medium (ICM), the Larmour frequency is much larger than the ion-ion collision frequency. In such a case, the thermal pr…
Dynamo in the Intra-Cluster Medium: Simulation of CGL-MHD Turbulent Dynamo
R. Santos-Lima, E. M. de Gouveia Dal Pino, A. Lazarian +2
The standard magnetohydrodynamic (MHD) description of the plasma in the hot, magnetized gas of the intra-cluster (ICM) medium is not adequate because it is weakly collisional. In s…