This research demonstrates that turbulence in galaxy clusters generates radio halos through synchrotron radiation from cosmic ray electrons. By linking large-scale astrophysical processes to familiar physical principles, it explains the origin of cluster emissions and advances understanding of how galaxy clusters form, merge, and evolve.

Dark matter makes up most of the universe but cannot be directly observed. This research studies how dark matter halos evolve using cosmological simulations and the principle of maximum entropy. Results show halo entropy increases over time, indicating their evolution toward equilibrium follows fundamental thermodynamic principles.