Abundance of Field Galaxies
Anatoly Klypin, Igor Karachentsev, Dmitry Makarov, Olga Nasonova

TL;DR
This study measures galaxy abundance in the Local Volume, revealing discrepancies with LCDM and WDM models, especially for dwarf galaxies, highlighting a significant overabundance problem in current cosmological theories.
Contribution
First detailed measurement of galaxy velocity function in the Local Volume down to dwarf galaxy scales, challenging standard dark matter models.
Findings
LCDM accurately predicts galaxy abundance for V>60 km/s but overestimates for V=30-50 km/s.
WDM models cannot reconcile the observed velocity function.
The observed shallow slope of the velocity function conflicts with LCDM predictions.
Abstract
We present new measurements of the abundance of galaxies with a given circular velocity in the Local Volume: a region centered on the Milky Way Galaxy and extending to distance 10Mpc. The sample of 750 mostly dwarf galaxies provides a unique opportunity to study the abundance and properties of galaxies down to absolute magnitudes MB= -10, and virial masses Mvir= 1e9Msun. We find that the standard LCDM model gives remarkably accurate estimates for the velocity function of galaxies with circular velocities V>60kms and corresponding virial masses Mvir> 3e10Msun, but it badly fails by over-predicting 5 times the abundance of large dwarfs with velocities V= 30-50kms. The Warm Dark Matter models cannot explain the data either, regardless of mass of the WDM particle. Just as in previous observational studies, we find a shallow asymptotic slope dN/dlog V = V**alpha, alpha =-1 of the velocity…
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