arXiv (All)
open access
Perturbations of Kerr-Newman black holes: separation and mode stability
We study linearized perturbations of the subextremal Kerr-Newman black hole solution of the Einstein-Maxwell equations. We show how to overcome what Chandrasekhar called the "apparent indissolubility of the coupling between the spin-1 and spin-2 fields" by using a matrix integrating factor for suita
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
- Five-dimensional Geometry from Spinning Amplitudes#785176
- Five-dimensional Geometry from Spinning Amplitudes#783586
- Spin-curvature effects in slowly rotating black hole spacetime#1050543
- Binary-black hole spin population results may be driven by prior degeneracies#997744
- The Force of Gravity as the Sum of Anti-Correlated Spins: A Complete Crossover Derivation Reconciling Quantum Mechanics, Classical Gravity, and General Relativity#197914
Record · ID 1118734
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