The Mass-To-Light Function: Antibias and Omega_m
N.A. Bahcall, R. Cen, R. Dav\'e, J.P. Ostriker, Q. Yu (Princeton, University Observatory)

TL;DR
This study uses cosmological simulations to analyze the mass-to-light ratio across different scales, revealing antibias in high-density regions and constraining the universe's matter density to Omega = 0.16.
Contribution
It provides the first comprehensive comparison of simulated and observed mass-to-light functions from galaxies to superclusters, constraining Omega_m.
Findings
Mass-to-light ratio increases with scale and flattens at large scales.
High-density regions show higher M/L_B values, indicating antibias.
Estimated Omega_m = 0.16 +/- 0.05.
Abstract
We use large-scale cosmological simulations to estimate the mass-to-light ratio of galaxy systems as a function of scale, and compare the results with observations of galaxies, groups, clusters, and superclusters of galaxies. We find remarkably good agreement between observations and simulations. Specifically, we find that the simulated mass-to-light ratio increases with scale on small scales and flattens to a constant value on large scales, as suggested by observations. We find that while mass typically follows light on large scales, high overdensity regions --- such as rich clusters and superclusters of galaxies --- exhibit higher M/L_B values than average, while low density regions exhibit lower M/L_B values; high density regions are thus antibiased in M/L_B, with mass more strongly concentrated than blue light. This is true despite the fact that the galaxy mass density is unbiased…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Impact of Light on Environment and Health
