A Study of Warm Dark Matter, the Missing Satellites Problem, and the UV Luminosity Cut-Off
Bruce Hoeneisen

TL;DR
This paper extends warm dark matter predictions below the velocity dispersion cut-off to address the Missing Satellites Problem and UV luminosity cut-off, aligning theory with observations and deriving the Tully-Fisher relation from first principles.
Contribution
It introduces an extension of the Press-Schechter formalism for warm dark matter to lower masses, providing new insights into satellite counts and luminosity limits.
Findings
Predictions match observed satellite counts.
Predictions align with UV luminosity cut-off constraints.
Derived the Tully-Fisher relation from fundamental principles.
Abstract
In the warm dark matter scenario, the Press-Schechter formalism is valid only for galaxy masses greater than the "velocity dispersion cut-off". In this work we extend the predictions to masses below the velocity dispersion cut-off, and thereby address the "Missing Satellites Problem", and the rest-frame ultra-violet luminosity cut-off required to not exceed the measured reionization optical depth. We find agreement between predictions and observations of these two phenomena. As a by-product, we obtain the empirical Tully-Fisher relation from first principles.
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Advanced Thermodynamics and Statistical Mechanics · Stellar, planetary, and galactic studies
