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 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 13075x
" The nearly universal merger rate of dark matter haloes in ΛCDM cosmology " Authors: Onsi Fakhouri and Chung-Pei Ma This is highly influential in astrophysics for understanding
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 paper determines the merger rates of dark matter haloes as a function of halo mass, merger mass ratio, and redshift.
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.
It utilizes the massive public database of the Millennium Simulation to track merger trees over a wide dynamic range in time and mass.