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Aims: morpholgies, number and energy distributions of Cosmological ShockWaves from a set of ENZO cosmological simulations are produced, along with astudy of the connection with Cosmic Rays processes in different environments.Method: we perform cosmological simulations with the public release of the PPMcode ENZO, adopt a simple and physically motivated numerical setup to followthe evolution of cosmic structures at the resolution of 125kpc per cell, andcharacterise shocks with a new post processing scheme. Results: we estimate theefficency of the acceleration of Cosmic Ray particles and present the firstcomparison of our results with existing limits from observations of galaxyclusters.

Cosmological Shocks in Eulerian Simulations: Main Properties and Cosmic Rays Acceleration