The Gaia DR3 catalog of over one million wide binaries opens a precise window onto gravity in the weak-field regime (a ≲ 10⁻¹⁰ m/s²), yet whether the observed velocity excess reflects modified gravity or unresolved systematics remains contested. This paper shows that the Temporal Equivalence Principle (TEP v0. 8 Jakarta) —in which a conformal scalar field modulates matter proper time as dτ/dt ≈ A (φ) (with A (φ) = exp (βφ/MPl) ) with the Cepheid-calibrated response scale denoted κCep, while the wide-binary transition is parameterized independently by the velocity-profile saturation amplitude αₛat, not by a bare scalar coupling—addresses that tension through smooth Temporal Shear recovery in weak-field environments. This paper tests whether the Gaia wide-binary anomaly is better described as smooth Temporal Shear recovery in weak-field environments. From 341, 315 high-purity systems, the analysis identifies a screening transition at Rₛ = 2, 646 ± 182 AU (statistical; ± 609 AU total), strongly preferred over both a flat Newtonian profile (Δχ² = 14, 845) and a constant boost (Δχ² = 3, 583). At large separation the profile saturates at αₛat = 0. 366 ± 0. 012, roughly 35–40% above the Keplerian baseline. Broader smooth-transition fits preserve the same few-thousand-AU onset. The signal also shows the environmental ordering required by TEP. With a non-circular metallicity guardrail that uses a conservative external βMLR prior unless independent spectroscopic metallicities are cached, the lower-density high-|Z| population transitions at smaller radius than the higher-density midplane (Rₛ = 4, 662 ± 196 versus 7, 131 ± 1, 341 AU), confirmed by a solar-track control (Rₛ = 4, 145 ± 276 versus 6, 856 ± 920 AU; permutation p < 10⁻⁴ for the full sample and p < 10⁻³ for the solar track). Scrambling tests and phase-mixed Newtonian orbital forward models fail to reproduce the observed screening preference. The wide-binary anomaly is therefore not a generic low-acceleration excess but a structured, environmentally modulated screening transition—one whose morphology, onset scale, and environmental ordering are quantitatively consistent with the conformal scalar field of TEP and are not reproduced by the Newtonian orbital-projection or MOND/EFE parameterizations tested here. Website: https: //mlsmawfield. com/tep/wb/Code Availability: https: //github. com/matthewsmawfield/TEP-WB DOI: 10. 5281/zenodo. 19102061 Keywords: Temporal Equivalence Principle – wide binaries – Gaia DR3 – weak-field gravity – Temporal Shear recovery – environmental transition morphology – Temporal Topology – Temporal Shear – modified gravity – MOND Open Science Statement: This work is a preprint and is open to community review, ideas, and collaboration. All materials required for full reproducibility—including data downloads, analysis scripts, code, and manuscripts—are open-source. Feedback and contributions to further test these results are welcome.
Building similarity graph...
Analyzing shared references across papers
Loading...
Matthew Lukin Smawfield
Building similarity graph...
Analyzing shared references across papers
Loading...
Matthew Lukin Smawfield (Wed,) studied this question.
www.synapsesocial.com/papers/69f4427a967e944ac5566079 — DOI: https://doi.org/10.5281/zenodo.19883316
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: