13075x May 2026

The paper determines the merger rates of dark matter haloes as a function of halo mass, merger mass ratio, and redshift.

It utilizes the massive public database of the Millennium Simulation to track merger trees over a wide dynamic range in time and mass. 13075x

The authors found that the merger rate per unit redshift is nearly universal and independent of redshift, scaling simply with halo mass and mass ratio. The paper determines the merger rates of dark

Monthly Notices of the Royal Astronomical Society (MNRAS), Vol. 386, Issue 2, pp. 577–592 (May 2008) Full DOI: 10.1111/j.1365-2966.2008.13075.x 📝 Summary of Content merger mass ratio

This is highly influential in astrophysics for understanding how galaxies and large-scale structures formed and grew in the universe! The Massively Accreting Cluster A2029 - OSTI.GOV