A Covariant Phenomenological Framework for Gravity: Emergent Pressure from Vacuum Dilatancy in a Relativistic Viscous Continuum

Read the full article See related articles

Discuss this preprint

Start a discussion What are Sciety discussions?

Listed in

This article is not in any list yet, why not save it to one of your lists.
Log in to save this article

Abstract

We present a covariant phenomenological framework for gravitational phenomena, interpreting the effects of general relativity (GR) as emergent spatial pressure'' resulting from mass-induced vacuum dilatancy''---a relativistic hydrodynamic perturbation---in a Lorentz-invariant viscous continuum. Mass sources a dynamic dilation of the vacuum, generating pressure gradients that drive geodesic motion toward regions of lower resistance, providing a mechanistic description of gravity without invoking geometric curvature directly. The model is derived from a diffeomorphism-invariant action principle, extending the Einstein-Hilbert Lagrangian with a scalar field kinetic term representing superfluid-like vacuum dynamics and a coupling to matter. Dissipative effects are incorporated via a Rayleigh dissipation function, yielding the relativistic Navier-Stokes equations through variation. Key parameters are \( \alpha = \eta / (\rho_0 c r_s) \) and \( \beta = 4\pi G \rho_0 / c^2 \), where \( \eta \) is the vacuum viscosity and \( \rho_0 \) the vacuum energy density. The viscous stress tensor \( \tau_{\mu\nu} \) ensures energy-momentum conservation to second order in gradients, with dissipation negligible on solar-system scales (\( t_\mathrm{drag} \sim 4.20 \times 10^{23} \) years) but relevant for cosmological gravitational waves. The framework reproduces GR predictions with high fidelity: Mercury's perihelion advance of $42.98''$/century \cite{park2019}, light deflection of $1.75''$ \cite{dyson1920}, and the LIGO GW150914 signal \cite{abbott2016}, with discrepancies \( <0.05\% \). SymPy-validated derivations, Bayesian inference (\( \gamma = 1.00 \pm 0.01 \)), and Monte Carlo error analyses confirm robustness. Novel predictions include LISA-detectable gravitational wave phase damping (\( \mathcal{O}(10^{-3}) \) radians), a MOND-like acceleration scale \( a_0 \approx 1.9 \times 10^{-10} \) m/s\( ^2 \) from \( \Lambda \) without dark matter, and $5-10%$ enhancements in cluster gravitational lensing. This approach avoids MOND's ad hoc phenomenology and TeVeS's instabilities, maintaining local Lorentz invariance through dynamical entrainment of the continuum, and offers a pathway toward quantum gravity unification.

Article activity feed