The impact of evolving cosmic filaments on mass and spin evolution of dark matter halos

arXiv:2606.19443 · astro-ph.CO, astro-ph.GA · Submitted 2026-06-17 · Read on arXiv

Hannah Jhee, Hyunmi Song, Clotilde Laigle, Christophe Pichon, Corentin Cadiou, Ena Choi

astro-ph.CO, astro-ph.GA

Submitted: 2026-06-17

Comments: 14 pages, 9 figures, submitted to MNRAS

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

Terminology

• Core — 24× in this paper · explained in 2 episodes
• Alignment — 20× in this paper · explained in 1 episode
• Trace — 10× in this paper · explained in 2 episodes
• National Research Foundation of Korea — 2× in this paper
• Selection Bias — 2× in this paper · explained in 4 episodes
• Ab Initio — 1× in this paper · explained in 1 episode
• Abundance — 1× in this paper · explained in 1 episode
• Anisotropy — 1× in this paper · explained in 3 episodes
• Mass Segregation — 1× in this paper · explained in 2 episodes

Sources

• Cosmic Web Dynamics: Forces and Strains

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