The halo model and numerical simulations

Details The halo model and numerical simulations The halo model and numerical simulations

2000-12-28

arxiv.org/abs/astro-ph/0012518v2

Astrophys.J.550:L129-L132,2001

Astronomy and Astrophysics

Astrophysics

4 pages, 3 figures, matches version accepted by ApJL

Scientific paper

10.1086/319644

Recently there has been a lot of attention focussed on a virialized halo-based approach to understanding the properties of the matter and galaxy power spectrum. A key ingredient in this model is the number and distribution of galaxies within dark matter halos as a function of mass. This quantity has been predicted from semi-analytic modeling and from fits to observational data. Here we present predictions for the occupation number and spatial distribution of sub-halos based on a high-resolution hydrodynamical simulation including cooling, star-formation and feedback.

Affiliated with

Also associated with

No associations

Rating

The halo model and numerical simulations 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 halo model and numerical simulations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The halo model and numerical simulations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-233140