Zenodo (CERN)
open access
Dynamic Geometric Phase Transitions in the BH-WW Model: Enhanced Klein Throat Vacuum, Gradual Equatorial Gravitational Attenuation, and Forward-Evolved Galactic Morphology
In classical astrophysics, the differential rotation dynamics of spiral galaxies mandate that arms trail behind the direction of rotation (trailing arms) along the galactic disk. Conversely, observational astronomy has documented extraordinary configurations (notably in systems such as NGC 4622)
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
- Disk tilts in Milky Way-like galaxies and their link to mergers#1356562
- Eliminating Dark Matter: Wave Geometry in the Time Field Model as an Alternative for Galactic Dynamics#721777
- Slow stellar halo rotation as a signature of disc flips and GES-like mergers#984249
- Dynamical Activation of a Transition Scale in Galactic Rotation Curves#176250
- Bimodal Regime Structure in Galactic Rotation Curves: Evidence for Distinct Dynamical States and a Field-Based Interpretation of the Dark Matter Effect#164842
Record · ID 1368869
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