arXiv (All)
open access
On the quasiblack-hole limit of rotating charged fluids
We investigate the extremal quasiblack-hole (QBH) limit of stationary, axisymmetric charged perfect fluids in rigid or differential rotation, with and without pressure. We emphasize Weyl-type configurations, whose redshift factor is functionally related to the generalized electromagnetic potential.
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
- Four Possible Ways to Model Rotating Universe#101409
- A strongly hyperbolic viscous relativistic hydrodynamics theory with first-order charge current#924510
- A strongly hyperbolic viscous relativistic hydrodynamics theory with first-order charge current#920279
- Scale invariant solutions in relativistic hydrodynamics#999241
- Critical behavior and critical exponents of rotating QCD matter#1129360
Record · ID 1130944
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