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Preprint . 2026
License: CC BY
Data sources: ZENODO
ZENODO
Preprint . 2026
License: CC BY
Data sources: Datacite
ZENODO
Preprint . 2026
License: CC BY
Data sources: Datacite
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Aether-Lagrangian Rotation Curves from Scalar Length Density in the Aether Physics Model

Authors: Thomson, David;

Aether-Lagrangian Rotation Curves from Scalar Length Density in the Aether Physics Model

Abstract

Description This preprint derives a closed-form galactic rotation-curve term from the Aether Physics Model (APM) galactic Aether Lagrangian by treating the scalar field $\Phi$ as a length density (unbound-string density) with dimension $[\Phi]=\mathrm{mass}/\mathrm{length}$. In the Newtonian weak-field limit, the scalar sector contributes an effective gravitating mass density through the standard energy-to-mass bridge\[\rho_\Phi = \frac{u_\Phi}{c^2}, \qquadu_\Phi = \frac{1}{2}(\nabla \Phi)^2 + \frac{1}{2}m_\Phi^2 \Phi^2.\]Within the steady-state, approximately spherical-halo limit, requiring an asymptotically flat circular speed selects a minimal sourced profile with\[\frac{d\Phi}{dr} = \frac{\Phi_0}{r+r_c},\]which yields a cored logarithmic field\[\Phi(r) = \Phi_0 \ln\!\left(1+\frac{r}{r_c}\right) + \Phi(0),\]an effective density scaling $\rho_\Phi \propto (r+r_c)^{-2}$, and an analytic halo rotation term\[v_\Phi^2(r)= v_\infty^2\left[1+\frac{r_c}{r}-\frac{r_c^2}{r(r+r_c)}-\frac{2r_c}{r}\ln\!\left(1+\frac{r}{r_c}\right)\right],\qquadv_\infty^2=\frac{2\pi G\Phi_0^2}{c^2}.\]To test this steady-state prediction on a comparatively regular external spiral, the paper ingests SPARC rotation-curve decomposition data for NGC~3198 and constructs the predicted total curve from the published SPARC baryonic components plus the APM scalar-halo term. The same term is then applied to a Milky Way worked example, where residuals are interpreted in the context of known non-equilibrium structure (bar/spiral non-axisymmetry, warp/flare, accretion debris, and tracer-dependent systematics), emphasizing that the analytic reduction is explicitly steady-state and weak-field. The paper also records falsifiable extensions that follow from the Lagrangian structure: (i) a Yukawa-scale outer cutoff when $m_\Phi \neq 0$, and (ii) potential electromagnetic/polarization signatures in environments where the APM electromagnetic couplings become non-negligible. Finally, it states a torsion-sourcing extension mechanism derived from the bipolar-trumpet coil toy model for black-hole torsion filaments and polar jets, introduced as a future-testable correction channel in torsion-active galactic-center environments without altering the present equilibrium derivation. What is included Newtonian-limit derivation of an analytic scalar-halo rotation term from the APM galactic Aether Lagrangian. Closed-form mapping between the sourced scalar profile, implied source function $S(r)=\nabla^2\Phi$, enclosed scalar mass $M_\Phi(r)$, and the halo rotation term $v_\Phi(r)$. SPARC-based worked example for NGC~3198 using published baryonic decomposition velocities. Milky Way contrast-case demonstration emphasizing limitations of steady-state assumptions in a dynamically complex system. Explicit statements of falsifiable extensions (nonzero $m_\Phi$, electromagnetic/polarization channels, and torsion-sourced corrections). Notes on units Computations in the worked examples are performed in standard astrophysical units (kpc, km/s, $M_\odot$) for rotation-curve modeling. Where relevant to the APM ledger, the paper also highlights the Gaussian-cgs bookkeeping identity $c^2 = A_u \,\mathrm{curl}_{\mathrm{ref}}$ used to clarify the mapping between scalar energy density and gravitating mass density.

Keywords

unbound strings, length density, polar jets, Aether Lagrangian, SPARC, NGC 3198, scalar field, Aether Physics Model, torsion filaments, Milky Way, APM, QMU, Quantum Measurement Units, galactic rotation curves, dark matter phenomenology

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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