arXiv (OAI Expanded)
open access
Modeling Globular Cluster Stellar Streams with a Basis-Expansion N-body Code
Globular cluster stellar streams probe galaxy-formation processes and can potentially reveal the distribution of dark matter in galaxies. In many theoretical studies, streams are modeled with particle-spray or direct N-body codes. But particle-spray methods abstract away the internal dynamics of the
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
- Self-interacting dark matter delays bar growth in an isolated gas-rich galactic disk: torque-resolved numerical evidence#1012531
- Eliminating Dark Matter: Wave Geometry in the Time Field Model as an Alternative for Galactic Dynamics#721777
- Universal Resonance Theory (URT): A 12.8 Hz Wave Unifying Dark Matter, Dark Energy, and Consciousness#693012
- A machine learning-based method for populating dark matter halos in N-body simulations with substructure#1154335
- A New Dark Matter Model for Galaxies#639549
Record · ID 1084137
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