The Registered Wide-Binary Target under a Local a0: A Conditional Charge Meter, and the EFE-Present Exact Two-Body Solve

Two refereed results about the hash-frozen Gaia DR4 wide-binary registration of the a0 = kappa c sqrt(G rho_Lambda) framework (the registration itself is untouched). (1) Because the framework's a0 is a local quantity set by the dark sector's pressure at the local shift-charge density, the now-settled steady-state-continuity reading of the solar-circle charge flow makes the registered velocity-boost target a CONDITIONAL charge meter: at the charge floor the target moves by less than the frozen band's own width at every corner of the solar-overdensity bracket and both footings; at the ceiling the move is corner-split (-0.004 sparse to -0.093/-0.109 dense) -- DR4 measures the charge only if the solar-circle overdensity sits toward the dense corner, and settling that overdensity is the named prerequisite. (2) The full nonlinear AQUAL two-body problem in a uniform external field (colinear, machinery-gated) shows the exact pair boost is 0.71-0.99x the linear per-star response at 5-30 kAU: the EFE-free benchmark correction (1.41-1.74x) overcorrects with the external field on. Both directions stated: the registered band top is conservative (a no-verdict above 1.23 less likely), AND the per-pair signal sits at or below the registered floor over most anchor separations (a reading below the band more likely). Every quantitative claim is reproduced by committed scripts.

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Publication Details

Journal
Zenodo (CERN European Organization for Nuclear Research)
Published
2026-08-14
DOI
https://doi.org/10.5281/zenodo.21937975
Primary Topic
Gamma-ray bursts and supernovae
Type
preprint
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preprint

The Registered Wide-Binary Target under a Local a0: A Conditional Charge Meter, and the EFE-Present Exact Two-Body Solve

Carl P. Zimmerman
Zenodo (CERN European Organization for Nuclear Research)
Gamma-ray bursts and supernovae
preprint

The Registered Wide-Binary Target under a Local a0: A Conditional Charge Meter, and the EFE-Present Exact Two-Body Solve

Carl P. Zimmerman
preprint en

Abstract

Two refereed results about the hash-frozen Gaia DR4 wide-binary registration of the a0 = kappa c sqrt(G rho_Lambda) framework (the registration itself is untouched). (1) Because the framework's a0 is a local quantity set by the dark sector's pressure at the local shift-charge density, the now-settled steady-state-continuity reading of the solar-circle charge flow makes the registered velocity-boost target a CONDITIONAL charge meter: at the charge floor the target moves by less than the frozen band's own width at every corner of the solar-overdensity bracket and both footings; at the ceiling the move is corner-split (-0.004 sparse to -0.093/-0.109 dense) -- DR4 measures the charge only if the solar-circle overdensity sits toward the dense corner, and settling that overdensity is the named prerequisite. (2) The full nonlinear AQUAL two-body problem in a uniform external field (colinear, machinery-gated) shows the exact pair boost is 0.71-0.99x the linear per-star response at 5-30 kAU: the EFE-free benchmark correction (1.41-1.74x) overcorrects with the external field on. Both directions stated: the registered band top is conservative (a no-verdict above 1.23 less likely), AND the per-pair signal sits at or below the registered floor over most anchor separations (a reading below the band more likely). Every quantitative claim is reproduced by committed scripts.

Zenodo (CERN European Organization for Nuclear Research)
Ad-Tech (United States) (US)
Gamma-ray bursts and supernovae
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