Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-06-25
Mon.Not.Roy.Astron.Soc.370:1247-1256,2006
Astronomy and Astrophysics
Astrophysics
11 Pages, 7 figs, Monthly Notices style
Scientific paper
10.1111/j.1365-2966.2006.10564.x
This paper aims at quantifying discreetness effects, born of finite particle number, on the dynamics of dark matter haloes forming in the context of cosmological simulations. By generalising the standard calculation of two body relaxation to the case when the size and mass distribution are variable, and parametrising the time evolution using established empirical relations, we find that the dynamics of a million particle halo is noise-dominated within the inner percent of the final virial radius. Far larger particle numbers (~ 10^8) are required for the RMS perturbations to the velocity to drop to the 10 % level there. The radial scaling of the relaxation time is simple and strong: t_relax ~ r^2, implying that numbers >> 10^8 are required to faithfully model the very inner regions; artificial relaxation may thus constitute an important factor, contributing to the contradictory claims concerning the persistence of a power law density cusp to the very centre. The cores of substructure haloes can be many relaxation times old. Since relaxation first causes their expansion before recontraction occurs, it may render them either more difficult or easier to disrupt, depending on their orbital parameters. It may thus modify the characteristics of the subhalo distribution and effects of interactions with the parent. We derive simple closed form formulas for the characteristic relaxation times, as well as for the weak N-scaling reported by Diemand et al. when the main contribution comes from relaxing subhaloes (abridged).
No associations
LandOfFree
Two Body Relaxation in Simulated Cosmological Haloes 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 Two Body Relaxation in Simulated Cosmological Haloes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Two Body Relaxation in Simulated Cosmological Haloes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-577772