The Peaks Formalism and the Formation of Cold Dark Matter Haloes

Details The Peaks Formalism and the Formation of Cold Dark Matter Haloes The Peaks Formalism and the Formation of Cold Dark Matter Haloes

2010-11-10

arxiv.org/abs/1011.2493v2

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

13 pages, 11 figures, published in MNRAS

Scientific paper

10.1111/j.1365-2966.2011.18282.x

We use two cosmological simulations of structure formation to study the conditions under which dark matter haloes emerge from the linear density field. Our analysis focuses on matching sites of halo collapse to local density maxima, or "peaks", in the initial conditions of the simulations and provides a crucial test of the central ansatz of the peaks formalism. By identifying peaks on a variety of smoothed, linearly extrapolated density fields we demonstrate that as many as ~70% of well-resolved dark matter haloes form preferentially near peaks whose characteristic masses are similar to that of the halo, with more massive haloes showing a stronger tendency to reside near peaks initially. We identify a small but significant fraction of haloes that appear to evolve from peaks of substantially lower mass than that of the halo itself. We refer to these as "peakless haloes" for convenience. By contrasting directly the properties of these objects with the bulk of the proto-halo population we find two clear differences: 1) their initial shapes are significantly flatter and more elongated than the predominantly triaxial majority, and 2) they are, on average, more strongly compressed by tidal forces associated with their surrounding large scale structure. Using the two-point correlation function we show that peakless haloes tend to emerge from highly clustered regions of the initial density field implying that, at fixed mass, the accretion geometry and mass accretion histories of haloes in highly clustered environments differ significantly from those in the field. This may have important implications for understanding the origin of the halo assembly bias, of galaxy properties in dense environments and how environment affects the morphological transformation of galaxies near groups and rich galaxy clusters.

Affiliated with

Also associated with

No associations

Rating

The Peaks Formalism and the Formation of Cold Dark Matter 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 The Peaks Formalism and the Formation of Cold Dark Matter Haloes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Peaks Formalism and the Formation of Cold Dark Matter Haloes will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-429798