A model for the metallicity evolution of damped Lyman α systems

We apply a physically motivated stellar feedback model to analyse the statistical properties of damped Lyman α systems (DLAs) expected in the concordance cold dark matter (CDM) model. Our feedback model produces extended low-metallicity cold gaseous discs around small galaxies. Since the space density of galaxies with low circular speeds is high, these discs dominate the cross-section for the identification of DLAs at all redshifts. The combined effects of star formation, outflows and infall in our models result in mild evolution of the NH i weighted metallicity content in DLAs with redshift, consistent with observations. According to our model, DLAs contribute only a small fraction of the volume averaged star formation rate at redshifts z≲ 5. Our model predicts weak evolution in ΩH i over the redshift range z= 0–5. Furthermore, we show that the cosmological evolution of ΩH i and the cosmic star formation rate are largely disconnected and conclude that the evolution of ΩH i as a function of redshift is more likely to tell us about feedback processes and the evolution of the outer gaseous components of small galaxies than about the cosmic history of star formation.