Cold collapse and the core catastrophe

Details Cold collapse and the core catastrophe Cold collapse and the core catastrophe

1999-03-11

arxiv.org/abs/astro-ph/9903164v1

Mon.Not.Roy.Astron.Soc.310:1147-1152,1999

Astronomy and Astrophysics

Astrophysics

Latex 13 pages, 4 figures. Submitted to MNRAS. High resolution colour version of figure 4 and other N-body images here: http

Scientific paper

10.1046/j.1365-8711.1999.03039.x

We show that a universe dominated by cold dark matter fails to reproduce the rotation curves of dark matter dominated galaxies, one of the key problems that it was designed to resolve. We perform numerical simulations of the formation of dark matter halos, each containing \gsim 10^6 particles and resolved to 0.003 times the virial radius, allowing an accurate comparison with rotation curve data. A good fit to both galactic and cluster sized halos can be achieved using the density profile rho(r) \propto [(r/r_s)^1.5(1+(r/r_s)^1.5)]^-1, where r_s is a scale radius. This profile has a steeper asymptotic slope, rho(r) \propto r^-1.5, and a sharper turnover than found by lower resolution studies. The central structure of relaxed halos that form within a hierarchical universe has a remarkably small scatter (unrelaxed halos would not host disks). We compare the results with a sample of dark matter dominated, low surface brightness (LSB) galaxies with circular velocities in the range 100-300 km/s. The rotation curves of disks within cold dark matter halos rise too steeply to match these data which require a constant mass density in the central regions. The same conclusion is reached if we compare the scale free shape of observed rotation curves with the simulation data. It is important to confirm these results using stellar rather than HI rotation curves for LSB galaxies. We test the effects of introducing a cut-off in the power spectrum that may occur in a universe dominated by warm dark matter. In this case halos form by a monolithic collapse but the final density profile hardly changes, demonstrating that the merger history does not play a role in determining the halo structure.

Affiliated with

Also associated with

No associations

Rating

Cold collapse and the core catastrophe does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Cold collapse and the core catastrophe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cold collapse and the core catastrophe will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-266913