General Relativity as the Einstein Limit of Time-Density

We develop a time-density approach to gravity in which general relativity emerges as a controlled Einstein limit through two independent constructions. In both, the central field is a scalar time-density quantity defined operationally via local clock-rate comparisons, rather than introduced as an auxiliary field. In Pathway A (Clock-Induced Geometry), spacetime geometry is reconstructed from clock-synchronization consistency on a pre-geometric manifold. This yields a disformal metric structure in which the temporal and spatial sectors become distinguished through an operationally selected timelike direction. In its derived isotropic-coordinate weak-field sector, the construction reproduces the standard Solar System post-Newtonian behavior, with γ = 1 and, subject to an explicit second-order matching condition on the exterior profile, β = 1; it admits a covariant completion with a controlled tensor gravitational-wave sector, with the additional scalar-mode dispersion analysis reserved for future work. In Pathway B (Time-Density Coupled Gravity), the metric and the time-density field coexist as dynamical partners in a covariant theory. The operational meaning of the scalar, together with an explicit universal minimal matter-coupling condition, selects the Jordan frame as the physical matter frame. Solar System viability is achieved through an intrinsic Yukawa-type screening mechanism of the scalar mode, so that the theory approaches the Einstein limit in the appropriate screened regime. A unifying weak-field result — the Time-Strain Hierarchy — organizes redshift, acceleration, tidal response, light bending, and the temporal Ricci projection under a single strain variable. Across the analyzed regimes, both pathways are compatible with the standard weak-field tests of general relativity and recover Einstein-limit behavior in a controlled way. The paper therefore establishes weak-field consistency and Einstein-limit recovery for the time-density framework, while leaving full strong-field completion, cosmological solution space, and global observational closure to future work.