Part I–IV
No-Singularity Gravity from Structural Stability
A regular black-hole metric with finite curvature invariants at the core, geodesic completeness, and observational consequences compared against Schwarzschild, Hayward, and Bardeen-type models.
16 chapters · 0 appendices
Chapters
- No-Singularity Gravity from Structural Stability521w
- Structural Stability as a Guiding Principle419w
- Regular Interior Geometry413w
- Weak-Field Consistency549w
- Strong-Field Regime613w
- Photon Dynamics and Black Hole Shadow622w
- Image Asymmetry and Effective Spin-Like Signatures667w
- Numerical Methods589w
- Observational Implications1,002w
- Discussion516w
- Appendices613w
- Mathematical Details605w
- Conclusion standalone0w
- Conclusion405w
- PrePhysical Selection: World Choice1,315w
- Ontological Refutation of Infinite Many-Worlds1,668w