We investigate the class of spacetime metrics compatible with a scalar-first formulation of physics in which a temporal field Θ(xμ) governs dynamical structure. Rather than assuming a metric or deriving one from a complete action principle, we ask a more constrained question: what forms of metric tensor are admissible when constructed from a scalar field and its first derivatives, subject to covariance, non-degeneracy, Lorentzian signature, and weak-field consistency? We show that, at first-derivative order, the most general symmetric rank-2 tensor constructed from a scalar field consists of a conformal term and a gradient-based disformal correction. Gradient-only constructions are excluded on both geometric and physical grounds: they are intrinsically degenerate and fail to reproduce the observed 1/r scaling of gravitational phenomena. This leaves the disformal class as the minimal admissible structure within the stated assumptions. We further interpret the Temporal Self-Consistency Principle (TSCP) as a stability constraint on scalar field configurations, requiring that admissible geometries remain well-behaved under perturbations. This provides a physically motivated restriction on the relative contributions of conformal and gradient terms, without invoking a fully specified variational theory. The result is a constrained framework in which the spacetime metric is not derived uniquely, but restricted to a specific functional class that any scalar-temporal theory must realize. This establishes a structural foundation for Time–Scalar Field Theory and clarifies the requirements that a complete action-based formulation must satisfy.
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Jordan Gabriel Farrell (Sat,) studied this question.
www.synapsesocial.com/papers/69c37b81b34aaaeb1a67dfa3 — DOI: https://doi.org/10.5281/zenodo.19187591
Jordan Gabriel Farrell
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