Prefer a chat interface with context about you and your work?
Constrained simulations of the magnetic field in the local Universe and the propagation of ultrahigh energy cosmic rays
We use simulations of LSS formation to study the build-up of magnetic fields (MFs) in the ICM. Our basic assumption is that cosmological MFs grow in a MHD amplification process driven by structure formation out of a seed MF present at high z. Our LCDM initial conditions for the density …