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

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

Related papers

• Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds
• Two sets of potential-density basis pairs for the study of radial perturbations in collisionless spherical stellar systems
• Constraining reionization-era Ly alpha escape with JELS-MUSE: a highly complete H alpha-selected sample at z about6.1
• Deriving volume density profiles of filaments from observed surface densities
• Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos
• MEGATRON: how the first stars can create an iron metallicity plateau in the smallest dwarf galaxies