What question did this study set out to answer?

This paper aims to reconcile the observed galactic rotation curves with baryonic mass without invoking dark matter.

June 19, 2026Open Access

Galactic Kinematics without Dark Matter: Unifying the Radial Acceleration and Baryonic Tully-Fisher Relations via Continuum Field Entropy and the Demise of the 4.0 Slope

Puntos clave

This paper aims to reconcile the observed galactic rotation curves with baryonic mass without invoking dark matter.
Utilized the Continuum Field Entropy framework to derive galactic gravitational fields.
Employed Markov Chain Monte Carlo (MCMC) Bayesian inference for empirical validation across 175 SPARC galaxies.
Applied Orthogonal Distance Regression to extract an empirical slope for the Baryonic Tully-Fisher Relation.
Achieved an empirical slope of S ≈ 3.37, rejecting the idealized slope of 4.0.
Isolated optical retardation factor γ_opt ≈ 0.185 and shear-thickening power-law scaling α ≈ 2.33.
Demonstrated tight intrinsic scatter of 0.0965 dex in radial acceleration across observed galaxies.

Resumen

**Preprint | Continuum Field Entropy Empirical Validation Series** **Submitted to The Astrophysical Journal (ApJ) | Manuscript #AAS78163** The observed discrepancy between the baryonic mass of galaxies and their rotation curves is traditionally attributed to collisionless dark matter halos. Concurrently, standard cosmological models and phenomenological theories (e. g. , MOND) rigidly mandate a Baryonic Tully-Fisher velocity slope of S ≡ 4. 0, forcing spatial dependencies to completely cancel out to achieve perfectly flat infinite rotation curves. This paper presents an alternative, unified empirical test utilizing the Continuum Field Entropy (CFE) framework. By deriving the galactic gravitational field as an exact solution to a scalar-tensor variational action operating on a non-linear Cosserat continuum, we successfully reproduce the Radial Acceleration Relation (RAR) across 175 SPARC galaxies without dark matter. A full Hierarchical Markov Chain Monte Carlo (MCMC) Bayesian inference isolates an optical retardation factor γₒpt ≈ 0. 185 and a shear-thickening power-law scaling of α ≈ 2. 33, achieving a remarkably tight intrinsic scatter of 0. 0965 dex. Applying these exact covariant limits (αβ ≈ 0. 44) to the deep-field BTFR regime, we prove mathematically that the covariant asymptotic limit collapses natively to Mb ∝ Vf^ (~3. 4), explicitly rejecting the idealized 4. 0 asymptote. We validate this derivation against rigorous Orthogonal Distance Regressions of the SPARC deep-field halos, extracting an empirical slope of S ≈ 3. 37. By preserving a residual spatial dependence (R⁰. 21), the CFE framework uniquely predicts the kinematic micro-decay observed at the extreme edges of galactic halos. **Project Integration: **This document is a standalone validation report. The underlying universal field equations, foundational axioms, and the complete multi-disciplinary validation framework can be found in the primary master manuscript (DOI: 10. 5281/zenodo. 20619635).

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