Computer Simulations of Cosmic Reionization

Understand

The cosmic reionization of hydrogen was the last major phase transition in the evolution of the universe, which drastically changed the ionization and thermal conditions in the cosmic gas.

• To the best of our knowledge today, this process was driven by the ultra-violet radiation from young, star-forming galaxies and from first quasars.
• We review the current observational constraints on cosmic reionization, as well as the dominant physical effects that control the ionization of intergalactic gas.
• We then focus on numerical modeling of this process with computer simulations.