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Discrepancies Between Limits and Measurements of Warm Dark Matter Properties
Bruce Hoeneisen
A limit on the expansion parameter a_hNR at which dark matter becomes non-relativistic has been obtained from the observed minimum halo mass hosting Milky Way satellites. This limi…
Are James Webb Space Telescope observations consistent with warm dark matter?
Bruce Hoeneisen
We compare observed with predicted distributions of galaxy stellar masses and galaxy rest-frame ultra-violet luminosities per unit bandwidth , in the redshift range $…
Understanding the Formation of Galaxies with Warm Dark Matter
Bruce Hoeneisen
The formation of galaxies with warm dark matter is approximately adiabatic. The cold dark matter limit is singular and requires relaxation. In these lecture notes we develop, step-…
A Study of Warm Dark Matter, the Missing Satellites Problem, and the UV Luminosity Cut-Off
Bruce Hoeneisen
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 predictio…