Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias

arXiv:2309.01039 · astro-ph.GA, astro-ph.CO · Submitted 2024-01-13 · Read on arXiv

Kai Wang, H. J. Mo, Yangyao Chen, Huiyuan Wang, Xiaohu Yang, Jiaqi Wang, Yingjie Peng, Zheng Cai

astro-ph.GA, astro-ph.CO

Submitted: 2024-01-13

Updated: 2026-08-19

Comments: 20 pages, 12 + 10 figures, MNRAS accepted!

Journal ref: MNRAS, Volume 528, Issue 2, February 2024, Pages 2046-2065

DOI: 10.1093/mnras/stae163

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Clustering — 9× in this paper · explained in 2 episodes
• Entanglement — 2× in this paper · explained in 3 episodes
• Gravitational Lensing — 2× in this paper · explained in 2 episodes
• Trace — 2× in this paper · explained in 2 episodes
• Accuracy — 1× in this paper · explained in 1 episode
• Aperture — 1× in this paper · explained in 1 episode
• Higher-order statistics — 1× in this paper · explained in 2 episodes
• Homogeneity — 1× in this paper · explained in 2 episodes
• National Science Foundation of China — 1× in this paper

Sources

• The Prime Focus Spectrograph Galaxy Evolution Survey

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