01 / Problem
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Paper 040 / June 14, 2026
Solar-System and Binary Timing Bounds on Jefimenko-Style Cogravity
A parameterized observational program for translational mass currents and retarded-source corrections
01 / Abstract
Abstract
This proposal turns Jefimenko-style cogravity into an observational parameter program. It introduces source, force, and propagation parameters for the Maxwell-like mass-current equations, then maps them to precession, light-deflection, ranging, ephemeris, and binary-timing residuals. The paper argues that observable residuals and equivalence classes are safer than field-name debates, because weak-field gravitoelectromagnetic variables are convention-dependent. The deliverable is a bounds ledger that tells laboratory experiments which parameter space remains worth testing.
02 / Frame
Research Frame
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\[
\begin{aligned}
\nabla\cdot\gfield &= -4\pi G\rho,\\
\nabla\cdot\kfield &=0,\\
\nabla\times\gfield&=-\partial_t\kfield,\\
\nabla\times\kfield&=-\beta_S\frac{4\pi G}{c_g^2}\J+\frac{1}{c_g^2}\partial_t\gfield,
\end{aligned}
\]
\[
\mathbf a=\gfield+\beta_F\vvec\times\kfield.
\]
03 / Structure
Paper Structure
The manuscript follows the JMP0X1B discipline: state the problem, formalize the model, name the claims, and publish enough source material for review and revision.
02 / Model
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03 / Claims
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04 / Evidence Plan
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04 / Files
Paper Files
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