The Necessity Depth Field: Dark Gravity as the Large-Scale Signature of FCLT Organizational Pressure
Abstract
Dark matter remains one of the most significant unresolved problems in cosmology. Despite overwhelming indirect evidence from galactic rotation curves, gravitational lensing, and large-scale structure formation, no dark matter particle has been directly detected in five decades of searching. This paper proposes a Fibonacci Causal Loop Theory (FCLT) alternative: the Necessity Depth Field (NDF). The NDF is the large-scale organizational pressure gradient generated by the FCLT necessity recursion S(n) = S(n-1) + S(n-2) operating through the S(0) non-local substrate. Because S(0) underlies all points in spacetime simultaneously and is pre-geometric, the NDF is not attached to baryonic matter — it is a structural field arising from the phi-deviation gradient of the matter distribution itself. This paper demonstrates that the NDF predicts qualitatively correct behavior for galactic rotation curves, gravitational lensing anomalies, and the early-universe deficit of apparent dark matter. Existing FCLT data from 9,912 NSA galaxies showing a 19.9% monotonic phi-deviation gradient provides the empirical foundation. Prediction 13 is formally stated: the apparent dark matter density profile of galaxies will correlate with the phi-deviation gradient of galaxy morphology — galaxies with steeper necessity depth differentials between core and halo will show stronger NDF effects. This prediction is testable against existing galaxy rotation curve databases combined with NSA morphological data.
Fields of Study & Subjects
Cosmology and Gravitation Theories
Dark Matter and Cosmic Phenomena
Galaxies: Formation
Evolution
Phenomena
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 11 March 2026
- Language
- EN
- Document type
- Preprint