arXiv (All)
open access
Photon-Return and Polar-Focusing Crossovers near Extremal Kerr
How precisely must a photon's impact parameter be tuned for it to complete $n$ windings around a nearly extremal Kerr black hole before escaping, and how does the same near extremal scaling control the focusing of neighboring rays? For equatorial prograde returns we find, with $κ=\sqrt{1-a^2/M^2}$ a
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
- How much of the black hole ringdown is sourced within the light ring?#794248
- How much of the black hole ringdown is sourced within the light ring?#790229
- Anti-Aggregative Therapy and Laser Iridectomy#1030953
- The entropy of black hole under second-order deviation from equilibrium#1076908
- Jet Feedback and the Self-Regulated Growth of Black Holes Embedded in AGN Disks#1110545
Record · ID 1357503
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