The nearly universal merger rate of dark matter haloes in ΛCDM cosmology

We construct merger trees from the largest data base of dark matter haloes to date provided by the Millennium Simulation to quantify the merger rates of haloes over a broad range of descendant halo mass (1012≲M0≲ 1015MȮ), progenitor mass ratio (10−3≲ξ≤ 1), and redshift (0 ≤z≲ 6). We find the mean m...

Full description

Saved in:
Bibliographic Details
Published inMonthly notices of the Royal Astronomical Society Vol. 386; no. 2; pp. 577 - 592
Main Authors Fakhouri, Onsi, Ma, Chung-Pei
Format Journal Article
LanguageEnglish
Published Oxford, UK Blackwell Publishing Ltd 2008
Subjects
Online AccessGet full text
ISSN0035-8711
1365-2966
DOI10.1111/j.1365-2966.2008.13075.x

Cover

More Information
Summary:We construct merger trees from the largest data base of dark matter haloes to date provided by the Millennium Simulation to quantify the merger rates of haloes over a broad range of descendant halo mass (1012≲M0≲ 1015MȮ), progenitor mass ratio (10−3≲ξ≤ 1), and redshift (0 ≤z≲ 6). We find the mean merger rate per halo, B/n, to have very simple dependence on M0, ξ, and z, and propose a universal fitting form for B/n that is accurate to 10–20 per cent. Overall, B/n depends very weakly on the halo mass (∝M0.080) and scales as a power law in the progenitor mass ratio (∝ξ−2) for minor mergers (ξ≲ 0.1) with a mild upturn for major mergers. As a function of time, we find the merger rate per Gyr to evolve roughly as (1 +z) n m with nm= 2–2.3, while the rate per unit redshift is nearly independent of z. Several tests are performed to assess how our merger rates are affected by e.g. the time interval between Millennium outputs, binary versus multiple progenitor mergers, and mass conservation and diffuse accretion during mergers. In particular, we find halo fragmentations to be a general issue in merger tree construction from N-body simulations and compare two methods for handling these events. We compare our results with predictions of two analytical models for halo mergers based on the extended Press–Schechter (EPS) model and the coagulation theory. We find that the EPS model overpredicts the major merger rates and underpredicts the minor merger rates by up to a factor of a few.
Bibliography:ark:/67375/HXZ-JKP4BD7S-0
istex:A9F12D6ACBA6323FAA1DB10EF4D273DA79C3FDE2
ObjectType-Article-1
SourceType-Scholarly Journals-1
ObjectType-Feature-2
content type line 23
ISSN:0035-8711
1365-2966
DOI:10.1111/j.1365-2966.2008.13075.x