arXiv (All)
open access
Irreducible-Mass Balance for Magnetized Null Horizons with an Internal Current Sheet
We begin with a general question: how does the irreducible mass of a magnetized black hole change when the horizon is not stationary? The null Raychaudhuri equation gives an exact area balance for any smooth null horizon, without assuming stationarity or axisymmetry. When the horizon is axisymmetric
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
- A weak Ly α halo for an extremely bright little red dot. Indications of enshrouded supermassive black hole growth#388329
- Schwinger instability for near-extremal charged BTZ black hole#1130451
- Magnetization of Iron Meteorites up to the Meter in Size as Possible Analogs for Asteroid Psyche#218645
- Reissner-Nordstrom in the Bertotti-Robinson-Bonnor-Melvin electromagnetic field#820884
- Overmassive black holes and little red dots naturally form in simulations#1035369
Record · ID 984372
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