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 matter haloes as a function of halo mass, merger mass ratio, and redshift. 13075x
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 The authors found that the merger rate per
The identifier refers to the last part of a Digital Object Identifier (DOI) for a specific academic paper. The paper associated with this identifier is: 🌌 The Paper The Massively Accreting Cluster A2029 - OSTI
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
" The nearly universal merger rate of dark matter haloes in ΛCDM cosmology " Authors: Onsi Fakhouri and Chung-Pei Ma
It utilizes the massive public database of the Millennium Simulation to track merger trees over a wide dynamic range in time and mass.