CGI-RSR-000035 | Horizon calculations ordinarily begin after a horizon-bearing background, flow, or characteristic structure has already been specified. Here we ask an upstream question: can a minimal deterministic source generate its own scale, transition, one-way characteristic surface, intrinsic dynamics, and radiative response?
CGI-RSR-000031 | We establish a dynamical mechanism by which coherence-driven structure formation produces the inverse-square scaling behavior associated with galactic rotation curves and gravitational lensing.
CGI-RSR-000030 | The paper establishes the following chain:
conserved outward flux -> rho(r) ~ r^-2 -> gravitational potential -> approximately constant lensing deflection. The resulting lensing behavior is consistent with the leading-order predictions of standard halo models used to interpret gravitational lensing observations.
CGI-RSR-000029 | The paper establishes the following chain: conserved outward flux -> rho(r) ~ r^-2 -> M(r) ~ r -> v(r) approximately constant. Under general conditions, inverse-square density profiles and flat galactic rotation curves arise as direct consequences of flux conservation in
three-dimensional space.
CGI-RSR-000023 | We investigate horizon-like emission from a deterministic, curvature-bound coherence field within the Coherence Geometry (CG) framework. A reduced multi-phase model with ordinary wave propagation, phase locking, and higher-spatial-derivative curvature stiffness is evolved outside a prescribed spherical core. Energy transport is measured using the complete radial Noether current.
CGI-BKS-0002 | Part II of the Coherence Geometry Foundations working reference text. It examines how quantum-like linear dynamics, causal and relativistic structure, residual coherence strain and cosmological background terms, electromagnetic field structure, thermodynamic behavior, and macroscopic transport can be represented as domain-level projections of the shared-amplitude, multi-phase coherence framework.
CGI-RSR-000001:
We present a constrained dynamical dark-energy parameterization that provides a fit-ready alternative to standard phenomenological models used in late-time cosmology.