A physical model for the 0 < z < 8 redshift evolution of the galaxy UV luminosity and stellar mass functions
Sandro Tacchella, Michele Trenti, C. Marcella Carollo

TL;DR
This paper introduces a physical model linking galaxy UV luminosity and stellar mass evolution from redshift 0 to 8 to dark matter halo assembly and gas infall, successfully fitting observed functions without requiring evolving star formation efficiency.
Contribution
The model provides a unified framework for galaxy evolution driven by dark matter halo growth, calibrated at z=4, and predicts the evolution of galaxy properties across cosmic time.
Findings
Model fits the z=4 luminosity and stellar mass functions.
Accurately predicts evolution of galaxy functions from z=0 to 8.
Highlights dark matter halo build-up as primary driver of galaxy evolution.
Abstract
We present a model to understand the redshift evolution of the UV luminosity and stellar mass functions of Lyman Break Galaxies. Our approach is based on the assumption that the luminosity and stellar mass of a galaxy is related to its dark matter halo assembly and gas infall rate. Specifically, galaxies experience a burst of star formation at the halo assembly time, followed by a constant star formation rate, representing a secular star formation activity sustained by steady gas accretion. Star formation from steady gas accretion is the dominant contribution to the galaxy UV luminosity at all redshifts. The model is calibrated by constructing a galaxy luminosity versus halo mass relation at via abundance matching. After this luminosity calibration, the model naturally fits the stellar mass function, and correctly predicts the evolution of both luminosity and stellar mass…
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