arXiv (All)
open access
A Novel Implementation of Self-Interacting Dark Matter in AREPO
cosmology-and-nongalactic-astrophysicshigh-energy-astrophysical-phenomenahigh-energy-physics-phenomenologyhigh-energy-physics-theory
Self-interacting dark matter (SIDM) influences halo structure through collisional heat transport and may solve several small-scale puzzles in structure formation. SIDM creates thermalized cores in low-mass haloes, which may account for the observed cored dwarf galaxies. During late-time gravothermal
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Baryon-Accelerated Core Collapse in SIDM Halos and its Imprint on Galactic Disks#972652
- Intracluster Light as a Probe for Dark Matter: Exploring Self-interacting Dark Matter and Cold Dark Matter with C-EAGLE Sims#985039
- Halo mass, star formation, and morphology in galaxies: A morphology-dependent connection between halo environment and star formation activity#972670
- Lower central dark matter densities in nearby galaxies than predicted by simulations#1122747
- Distinguishing cold and self-interacting dark matter through topological analysis#785230
Record · ID 1142497
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive