arXiv (All)
open access
The Depletion of Collisionless Dark Matter Spikes
astrophysics-of-galaxiescosmology-and-nongalactic-astrophysicsgeneral-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomena
Dense concentrations of dark matter surrounding black holes provide a compelling opportunity to probe the nature of dark matter. In the classic Gondolo--Silk model, the adiabatic growth of a massive black hole in a dark matter cusp produces a steep density spike ($ρ\propto r^{-7/3}$), potentially in
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
- Assessing an Alternative Cosmology#100340
- Dark-Sector Effects on the Phase Structure of Nonlinear Magnetic AdS Black Holes#927476
- The Cosmological Simulation Code OpenGadget3 - Implementation of Self-Interacting Dark Matter#1035421
- Touching Reality#716026
- Reconstructing the Projected Dark Matter Field across 0.1-100 Mpc Scales from the SDSS Survey#1013892
Record · ID 1131496
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