The Nearly Universal Merger Rate of Dark Matter Haloes in Lambda-CDM Cosmology
Onsi Fakhouri (UCB), Chung-Pei Ma (UCB)

TL;DR
This study uses the Millennium simulation to derive a universal, accurate formula for dark matter halo merger rates across a wide range of masses, redshifts, and progenitor ratios, revealing weak mass dependence and specific scaling behaviors.
Contribution
It provides the first comprehensive, universal fitting formula for halo merger rates based on large simulation data, improving upon previous analytical models.
Findings
Merger rate per halo scales weakly with mass (M0^0.08).
Merger rate scales as xi^-2 for minor mergers.
Merger rate per Gyr evolves as (1+z)^2-2.3.
Abstract
We construct merger trees from the largest database 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 (1e12 < M0 < 1e15 Msun), progenitor mass ratio (1e-3 < xi < 1), and redshift (0 < z < 6). We find the mean merger rate per halo, B/n, to have very simple dependence on M0, xi, and z, and propose a universal fitting form for B/n that is accurate to 10-20%. Overall, B/n depends very weakly on the halo mass (proportional to M0^0.08) and scales as a power law in the progenitor mass ratio (proportional to xi^-2) for minor mergers (xi < 0.1) with a mild upturn for major mergers. As a function of time, we find the merger rate per Gyr to evolve as (1+z)^n with n=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…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
