arXiv (All)
open access
Tidal Heating of Stellar Clusters in Fuzzy Dark Matter Halos
astrophysics-of-galaxiescosmology-and-nongalactic-astrophysicsgeneral-relativity-and-quantum-cosmologyhigh-energy-physics-phenomenology
Ultra-faint dwarf galaxies serve as powerful testing grounds for wave dark matter models through dynamical stellar heating. Previous simulation-based work derived a lower bound on the fuzzy dark matter particle mass using a diffusion approximation valid only when the de Broglie wavelength is much sm
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
- Halo mass, star formation, and morphology in galaxies: A morphology-dependent connection between halo environment and star formation activity#972670
- The central densities of Milky Way-mass galaxies in cold and self-interacting dark matter models#1249981
- Understanding the Formation of Ultra-diffuse Galaxies through Systematic Observations#234098
- The Dependence of Tidally-Induced Star Formation on Cluster Density#639545
- Path Measures for Stochastic Galaxy Formation on Layered Halo Graphs#1076834
Record · ID 1389258
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