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April 3, 20260 citationsOpen Access

Gravity as Vacuum Overpressure: A Le Sage Mechanism from Massive Brans-Dicke Scalars

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DLDaniel Leonforte

Key Points

  • This research aims to reformulate gravity dynamics by viewing it as a pressure-mediated effect of vacuum defined by a massive Brans-Dicke scalar field.
  • Proposed a model using Vacuum Folding Dynamics (VFD) combining scalar field concepts with gravity.
  • Developed a prediction curve in parameter space influenced by vacuum pressure and scalar mass.
  • Evaluated the model against existing experimental bounds, specifically focusing on sub-millimeter scales.
  • Included an experimental proposal for testing predictions with a torsion-balance setup.
  • Predicted parameter curve lies significantly below current torsion-balance experimental limits.
  • Free Brans-Dicke parameter Omega_0 allows flexibility in predictions, constrained only by inverse-square law tests.
  • Sensitivity improvements in testing may either verify or rule out the proposed predictions within a defined range.

Abstract

We propose a reformulation of Vacuum Folding Dynamics (VFD) in which Newtonian gravity arises as a net inward force from isotropic vacuum pressure partially attenuated by matter — a modern Le Sage mechanism mediated by a massive Brans-Dicke scalar field. The scalar mass is fixed by a self-consistency condition linking the vacuum pressure to Newton's constant: mₛigma = f (Omega₀), where Omega₀ is the free Brans-Dicke parameter. Because the scalar is massive (Compton wavelength lambdaC ~ 0. 1–5 mm at the experimentally accessible sweet spot), solar-system PPN constraints such as Cassini do not apply, and Omega₀ remains free — bounded only by sub-centimetre inverse-square-law (ISL) tests (Omega₀ > ~50). The result is a one-parameter prediction curve in (alpha, lambda) space for a Yukawa-type fifth force, where alpha = 1/ (2*Omega₀ + 3) and lambda = hbar/ (mₛigma * c). The prediction curve lies a factor 5–20 below current Eöt-Wash torsion-balance bounds in the range lambda = 0. 1–5 mm, |alpha| = 10^-3–10^-2. The model is unscreened (no chameleon, symmetron, or Vainshtein mechanism), making it uniquely testable at laboratory scales. A sensitivity improvement of roughly one order of magnitude in sub-millimetre ISL experiments would either detect or definitively exclude the entire prediction curve. An exclusion plot (Figure 1) shows the VFD prediction curve against current Eöt-Wash bounds. A supplementary experimental proposal for torsion-balance tests is included. v6: Corrected numerical evaluation of Eq. 21 (factor 10 error in denominator), removed erroneous Eq. 26 (alphaₑff), removed inapplicable Cassini constraint, reformulated prediction as one-parameter curve.

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Cite This Study

Daniel Leonforte (2026) studied this question.

synapsesocial.com/papers/69cf5ebc5a333a821460d44ahttps://doi.org/10.5281/zenodo.19351439
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Also Consider

Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context:

  1. 1Emergent Tensor Gravity from Vacuum Entanglement Scattering2026
  2. 2Vacuum Folding Dynamics: Precision Observables and Experimental Windows2026
  3. 3Vacuum Folding Dynamics: Gravitation as Informational Underpressure2026
  4. 4Vacuum Folding Dynamics: Experimental Protocol for SRF Cavity Detection of Vacuum Scalar Oscillations2026
  5. 5Vacuum Folding Dynamics: Cosmological Signatures of Holographic Vacuum Screening2026