arXiv (All)
open access
Probing hairy Kerr black holes through quasi-periodic oscillations II: a study based on the resonance models
Hairy black holes (BHs), characterized by nontrivial scalar or matter fields, introduce additional degrees of freedom beyond mass, charge, and spin, providing a framework for testing deviations from the Kerr paradigm. We investigate a class of rotating hairy black holes constructed within the gravit
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
- From Scalar Clouds to Rotating Hairy Black Holes#11567
- Hidden Symmetries and Higher Dimensional Rotating Black Holes#417726
- Evolution and disruption of circular orbits during dynamic black hole scalarization#1064083
- Chaos bound for spinning particles in a hairy black hole with two photon spheres#1115747
- Disk warping and black hole X-ray binaries: I. Tentative unification of low-frequency quasi-periodic oscillations#415097
Record · ID 1248658
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