This paper derives a concrete observational prediction of the Breathing Universe effective field framework by analyzing the propagation of gravitational waves in the presence of a scalar vacuum-tension background. In earlier work, vacuum-tension imbalance was formulated as a covariant scalar order parameter H(x) within a scalar–tensor effective field theory that preserves general covariance and recovers General Relativity in the infrared regime. Building on that dynamical formulation, the present analysis studies tensor perturbations propagating through a slowly varying background configuration of the vacuum-tension field. Linearization of the coupled scalar–tensor system shows that the scalar background modifies the propagation operator for gravitational waves. Within the effective field theory regime k much smaller than the cutoff scale M*, these corrections produce a modified dispersion relation containing both background-dependent speed shifts and higher-derivative dispersive terms. The resulting propagation law implies frequency-dependent gravitational-wave velocities. Over astrophysical propagation distances this leads to an accumulated phase drift between frequency components of the signal. The magnitude of the effect is estimated for representative parameter ranges and compared with the sensitivity of current and planned gravitational-wave observatories, including LIGO, Virgo, KAGRA, LISA, the Einstein Telescope, and Cosmic Explorer. Because General Relativity predicts strictly non-dispersive gravitational-wave propagation in vacuum, the predicted dispersion provides a direct empirical test of vacuum-tension dynamics. Continued observational confirmation of the standard dispersion relation progressively constrains the parameter space of the effective theory, while detection of frequency-dependent propagation would indicate additional dynamical structure in the vacuum sector. The analysis therefore establishes a clear experimental pathway for testing and potentially falsifying the Breathing Universe effective field formulation.
Ivo Gerlach Angela Noel Cerfontaine (Fri,) studied this question.
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