Kavli Affiliate: Mark Vogelsberger | Summary:Cosmological simulations within the standard cold dark matter (CDM) paradigm systematically predict higher values of the dimensionless bar-speed parameter, $boldsymbolR equiv R_mathrmcr/R_mathrmbar$ (where $R_mathrmcr$ and $R_mathrmbar$ denote the corotation radius and the bar radius, respectively), than those inferred from observations of local galaxies, a discrepancy known as the fast-bar tension. […]
Continue.. The AIDA-TNG project: Galactic bar pattern speeds in self-interacting dark matter