Towards the First Galaxies

TL;DR

This paper reviews recent advances in understanding the formation of the first galaxies at high redshifts through numerical simulations, focusing on physical processes like cooling, radiation, and supernova feedback, and discusses observational prospects.

Contribution

It synthesizes recent simulation-based insights into early galaxy assembly, highlighting the roles of HD cooling, UV radiation, and supernova feedback in their evolution.

Findings

HD cooling influences primordial gas collapse

UV radiation impacts star formation and galaxy growth

Supernova feedback shapes early galaxy properties

Abstract

The formation of the first galaxies at redshifts z~10-15 signaled the transition from the simple initial state of the universe to one of ever increasing complexity. We here review recent progress in understanding their assembly process with numerical simulations, starting with cosmological initial conditions and modelling the detailed physics of star formation. In particular, we study the role of HD cooling in ionized primordial gas, the impact of UV radiation produced by the first stars, and the propagation of the supernova blast waves triggered at the end of their brief lives. We conclude by discussing promising observational diagnostics that will allow us to probe the properties of the first galaxies, such as their contribution to reionization and the chemical abundance pattern observed in extremely low-metallicity stars.