HγC X: Projected Accumulation Geometry and Weak-Field Lensing in the HγC Framework
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Abstract
We extend the HγC framework to the interpretation of weak-field lensing observables. Previous work established a minimal geometric bridge by embedding the effective accumulation potential ΦA = αA into an emergent weak-field metric, thereby providing a common description of slow massive motion and leading-order null propagation. Building on that result, we argue that weak-field lensing in the HγC framework should not be interpreted simply as a direct tracer of the instantaneous baryonic distribution, but rather as a probe of projected accumulation geometry. The central reason is that the effective gravitational response of the accumulation sector is profile-dependent. It is governed not by local baryonic source…
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Topics
Keywords
- Gravitational lens
- Weak gravitational lensing
- Galaxy
- Baryon
- Offset (computer science)
- Non-equilibrium thermodynamics
- Gravitation
- Strong gravitational lensing
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