Predictions for the abundance of high-redshift galaxies in a fuzzy dark matter universe
Predictions for the abundance of high-redshift galaxies in a fuzzy dark matter universe
During the last decades, rapid progress has been made in measurements of the rest-frame ultraviolet (UV) luminosity function (LF) for high-redshift galaxies ($z \geq 6$). The faint-end of the galaxy LF at these redshifts provides powerful constraints on different dark matter models that suppress small-scale structure formation. In this work …