Why do galaxies have extended flat rotation curves?
Bruce Hoeneisen

TL;DR
This paper explores why galaxies exhibit extended flat rotation curves by examining galaxy formation with warm dark matter, suggesting halos are in thermal equilibrium at large radii, which challenges current understanding.
Contribution
It proposes a theoretical explanation for the formation of galaxy halos in thermal equilibrium with warm dark matter in an expanding universe.
Findings
Galaxies' halos are in thermal equilibrium at large radii.
Flat rotation curves extend out to ~1 Mpc without decline.
Galaxy formation in warm dark matter context explains observed dynamics.
Abstract
Recent observations by Mistele et al. show that the circular velocity curves of isolated galaxies remain flat out to the largest radii probed so far, i.e. Mpc. The velocity decline beyond the expected virial radius is not observed. These results imply that the galaxy halo is in thermal equilibrium even at large radii where particles did not have time to relax. The galaxies must have already formed in the isothermal state. How is this possible? In the present note we try to understand the formation of galaxies with warm dark matter in the expanding universe.
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Taxonomy
TopicsAstronomy and Astrophysical Research · Geophysics and Gravity Measurements · Scientific Research and Discoveries
