The Universal Specific Merger Rate of Dark Matter Halos
Fuyu Dong, Donghai Zhao, Jiaxin Han, Zhaozhou Li, Yipeng Jing, Xiaohu, Yang

TL;DR
This study reveals a universal form for the specific merger rate of dark matter halos, depending only on mass ratio, independent of host mass or redshift, indicating self-similar halo growth across cosmologies.
Contribution
It introduces a universal specific merger rate function for dark matter halos, independent of mass and redshift, supported by high-resolution simulations across different cosmologies.
Findings
The specific merger rate is universal and depends only on the mass ratio.
The universal merger rate predicts a redshift- and mass-independent un-evolved subhalo mass function.
Halo growth is self-similar and proportional to the mass accretion history.
Abstract
We employ a set of high resolution N-body simulations to study the merger rate of dark matter halos. We define a specific merger rate by normalizing the average number of mergers per halo with the logarithmic mass growth change of the hosts at the time of accretion. Based on the simulation results, we find that this specific merger rate, , has a universal form, which is only a function of the mass ratio of merging halo pairs, , and does not depend on the host halo mass, , or redshift, , over a wide range of masses () and merger ratios (). We further test with simulations of different and , and get the same specific merger rate. The universality of the specific merger rate shows that halos in the universe are built up…
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.
