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 nearly universal merger rate of dark matter haloes in ΛCDM cosmology " Authors: Onsi Fakhouri and Chung-Pei Ma 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

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 386, Issue 2, pp

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

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

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