arXiv (All)
open access
The quasinormal modes of Kerr-Newman black holes: a separated approach
We compute Kerr-Newman quasinormal modes using a recently found exact separation of the gravitoelectric perturbation equations. For each spin-label $ς=\pm1$, a matrix angular ordinary differential equation and a scalar second-order radial ordinary differential equation define a joint spectral proble
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
- Charged particle interference in Kerr-Newman spacetime based on teleparallel gravity#1037662
- Spectral Inheritance and the First Kerr Datum in Generalized Trace Dynamics: The gyromagnetic ratio, black-hole entropy, and the missing localization profile#341856
- Avoided crossings and resonances in black hole ringdown with coupled fields: A case study of the Einstein-Maxwell-axion system#1128672
- Perturbations and quasinormal modes of black holes in general relativity coupled to nonlinear electrodynamics#1083760
- Quasinormal Modes of Reissner-Nordström Black Holes in Modified Gravity#1155328
Record · ID 1216517
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